CME Scoreboard
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CCMC CME Scoreboard
CME arrival time predictions from the research community:
The CME Scoreboard is part of the the CME Arrival Time and Impact Working Team in the Community-wide International Forum for Space Weather Modeling Capabilities Assessment.
The CME Scoreboard (developed at the Community Coordinated Modeling Center, CCMC) is a research-based forecasting methods validation activity which provides a central location for the community to:
- submit their forecast in real-time
- quickly view all forecasts at once in real-time
- compare forecasting methods when the event has arrived
Using this system:
- Anyone can view prediction tables
- Registered users can enter in your CME shock arrival time forecast after logging in:
- Registered Users: Begin by finding your CME under the "Active CMEs" section, then click "Add Prediction" and select your forecasting "Method Type" from the list.
- Power Users: If you do not see your CME listed under the "Active CMEs" section, click "Add CME" to get started (Email M. Leila Mays to request power user privileges). To enter the actual CME shock arrival time, click "Edit CME" after you are done entering your prediction(s).
- To register for an account, please email M. Leila Mays with your name, affiliation, and email address.
- Click here to see a list of registered methods. If you would like to register your prediction method, please send an email to M. Leila Mays or Yihua Zheng with your model/technique details.
- Click here for more detailed instructions.
Communication:
- To receive periodic announcements and/or automated email notifications when a new CME is added to the CME Scoreboard, you can subscribe to our mailing list by sending an email to M. Leila Mays with your name and email.
Resources:
Active CMEs:
|
CME: 2022-06-29T02:09:00-CME-001
|
|
CME Note: Visible in the NW in STEREO A COR2, possible faint partial halo in the N in SOHO LASCO C2. May be associated with filament eruption centered near N25E15, visible in SDO AIA 193 beginning 2022-06-28T21:48Z.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-07-03T05:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-06-29T13:03Z |
87.95
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-07-04T18:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-06-29T18:00Z |
120.00
|
----
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-07-03T23:30Z
|
----
|
----
|
--- |
--- |
Max Kp Range: 2.0 - 4.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
Past CMEs:
|
CME: 2022-06-19T21:53:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Visible in the NW in STEREO A COR2 and in the E in SOHO LASCO C2/C3. Overlaps with outflow from previous CME in SOHO imagery. May possibly be associated with filament eruption near N30E40, visible in STEREO A EUVI 195 beginning 2022-06-19T20:55Z and SDO AIA 131/171/193/304 beginning 2022-06-19T21:07Z. Some deflection in the SDO FOV. Very narrow event (perhaps 6-8 degrees half-width) and a very diffuse leading edge, apparently directed toward the narrow region between STEREO A and SOHO spacecraft. UPDATE (2022-06-23T13:00Z): The arrival of this CME at L1 may possibly have been detected by DSCOVR at 2022-06-22T11:27Z, but the magnetic signature is weak and the solar wind data inconclusive.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-06-22T12:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-06-20T11:37Z |
48.38
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-06-22T13:37Z
(-3.2h, +3.2h)
|
----
|
45.0
|
2022-06-20T14:27Z |
47.17
|
Max Kp Range: 4.0 - 6.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-06-22T12:48Z
|
----
|
45.0
|
--- |
--- |
Max Kp Range: 3.5 - 5.5
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-06-13T03:12:00-CME-001
|
| Actual Shock Arrival Time: 2022-06-15T04:01Z |
Observed Geomagnetic Storm Parameters:
Max Kp: 5.0
CME Note: This CME is seen as a partial halo to the east in SOHO LASCO C2/C3 and STEREO A COR2 coronagraph imagery. The source is an eruption from AR 3032 (N21E44) around 2022-06-13T02:45Z seen best in SDO AIA 131, 171, 193, and 304. The eruption is accompanied by an M3.4 flare from AR 3032, an opening of field lines, and post eruptive dimming and loops seen in SDO AIA 131, 171, and 193 starting to form around 05:00Z. The eruption is also seen about N30E30 in STEREO A EUVI 195 and 304, where an EUV wave is observed in STEREO A EUVI 195 around 03:25Z. L1 arrival signature: B total sharply increased to 14 nT at 04:01Z, accompanied by rotation of magnetic field components and a brief sharp increase in density and temperature. Solar wind velocity increased from around 475 km/s to around 620 km/s in as seen in DSCOVR data. Flux rope is seen some time after 07:00Z.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-06-15T00:21Z
(-7.0h, +7.0h)
|
-3.67
|
----
|
2022-06-13T13:36Z |
38.42
|
Max Kp Range: 6.0 - 8.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Mary Aronne (M2M) |
Detail
|
| 2022-06-15T12:00Z
(-7.0h, +7.0h)
|
7.98
|
25.0
|
2022-06-13T16:00Z |
36.02
|
Max Kp Range: 5.0 - 7.0
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-06-15T06:00Z
(-9.0h, +9.0h)
|
1.98
|
30.0
|
2022-06-13T17:45Z |
34.27
|
----
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-06-15T04:47Z
|
0.77
|
----
|
2022-06-13T17:50Z |
34.18
|
Max Kp Range: 5.0 - 7.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-06-14T15:00Z
(-6.0h, +6.0h)
|
-13.02
|
75.0
|
2022-06-13T22:06Z |
29.92
|
Max Kp Range: 4.0 - 5.0
|
Other (SIDC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-06-14T23:52Z
(-5.4h, +7.5h)
|
-4.15
|
100.0
|
2022-06-13T23:00Z |
29.02
|
Max Kp Range: 6.0 - 8.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-06-15T05:00Z
|
0.98
|
90.0
|
2022-06-14T00:50Z |
27.18
|
Max Kp Range: 4.0 - 6.0
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-06-14T20:07Z
(-4.0h, +12.0h)
|
-7.90
|
----
|
2022-06-14T09:00Z |
19.02
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-06-15T15:17Z
(-9.0h, +9.0h)
|
11.27
|
----
|
2022-06-14T09:03Z |
18.97
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-06-15T03:22Z
|
-0.65
|
64.0
|
--- |
--- |
Max Kp Range: 5.0 - 6.83333
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-06-04T03:48:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Visible in the NE of SOHO LASCO C2/C3 and the north of STEREO A COR2. Source is a filament eruption centered around N40E25 as seen from SDO AIA 191 and 304 imagery at 2022-06-04T02:00Z. The eruption can also be seen north of center disk from STEREO A EUVI 195.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-06-08T00:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-06-04T14:35Z |
81.42
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Mary Aronne (M2M) |
Detail
|
| 2022-06-07T18:00Z
(-12.0h, +12.0h)
|
----
|
20.0
|
2022-06-05T11:43Z |
54.28
|
Max Kp Range: 3.0 - 4.0
|
Other (SIDC)
|
Mary Aronne (M2M) |
Detail
|
| 2022-06-07T21:00Z
|
----
|
20.0
|
--- |
--- |
Max Kp Range: 2.5 - 3.5
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-06-02T06:09:00-CME-001
|
| Actual Shock Arrival Time: 2022-06-06T09:20Z |
Observed Geomagnetic Storm Parameters:
Max Kp: 3.0
CME Note: The likely source for this CME is a filament eruption which is centered around on S35W40 best seen in SDO AIA 193/171/304 A starting around 2022-06-02T05:20Z, though it was noted in SDO 171 that faint field lines were seen leaving the disk which were out-ahead of the eruption off the limb and not associated with the filamentary material. Clear arrival signature at L1: sudden increase in B total to approximately 11.5 nT (eventually going to over 14 nT), accompanied by a sharp temporary increase in density to 51 n(cm^-3) and ion temperature. Clear shock in the magnetic field, rotation of the Bz component (briefly reaching -11 nT), gradual rotation of Bx. Solar wind speed jumped from 260 km/s to approximately 315 km/s.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-06-05T23:00Z
(-6.0h, +12.0h)
|
-10.33
|
65.0
|
2022-06-02T05:07Z |
100.22
|
Max Kp Range: 4.0 - 5.0
Dst min. in nT: -90
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-06-05T16:58Z
(-12.0h, +12.0h)
|
-16.37
|
----
|
2022-06-02T12:00Z |
93.33
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-06-05T07:58Z
(-12.0h, +12.0h)
|
-25.37
|
----
|
2022-06-02T12:02Z |
93.30
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-06-05T01:00Z
(-12.0h, +12.0h)
|
-32.33
|
70.0
|
2022-06-02T12:06Z |
93.23
|
Max Kp Range: 4.0 - 6.0
|
Other (SIDC)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-06-05T19:48Z
(-7.0h, +7.0h)
|
-13.53
|
----
|
2022-06-02T16:17Z |
89.05
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-06-05T04:34Z
|
-28.77
|
----
|
2022-06-02T16:20Z |
89.00
|
Max Kp Range: 3.0 - 5.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-06-06T00:00Z
(-12.0h, +12.0h)
|
-9.33
|
40.0
|
2022-06-02T22:28Z |
82.87
|
Max Kp Range: 3.0 - 6.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-06-05T19:17Z
(-5.1h, +6.2h)
|
-14.05
|
71.0
|
2022-06-02T22:35Z |
82.75
|
Max Kp Range: 3.0 - 5.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-06-05T14:34Z
|
-18.77
|
61.5
|
--- |
--- |
Max Kp Range: 3.33333 - 5.33333
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-06-01T01:54:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: CME is seen to the west in STEREO A COR2 and SOHO LASCO C2 imagery. The source is likely the filament eruption seen in SDO AIA 193/304 near Active Region 3023 (S13W15) around 2022-06-01T00:30Z. Although there is a data gap in STEREO A EUVI 195 from 05-31T23:25Z to 06-01T01:55Z, a dimming region is seen in the west after imagery reappears. This agrees with the direction the CME is headed in STEREO A COR2 imagery. From LASSOS regarding L1 signature on 06-05: No ICME - per looking at the proton density (which keeps increasing during this time period) and ion temperature (which is not low as we can expect for a CME). The solar wind bulk speed is really low during this time which can be a reason for the observed higher proton density since slower solar wind is denser. Looking at the magnetic field components, there are traces of rotations but none of them are complete and coherent rotations.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-06-05T10:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-06-01T17:40Z |
88.33
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Mary Aronne (M2M) |
Detail
|
| 2022-06-05T10:00Z
|
----
|
----
|
--- |
--- |
Max Kp Range: 2.0 - 3.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-05-25T18:38:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Visible in the SW in STEREO A COR2 and in SOHO LASCO C2/C3. Moves quickly through C2 FOV. Associated with eruption in vicinity of AR 13016 (S18W42), visible in SDO AIA 131/171/193/304 and STEREO A EUVI 195/304 beginning 2022-05-25T18:01Z.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-05-28T15:23Z
|
----
|
----
|
2022-05-26T06:00Z |
57.38
|
Max Kp Range: 3.0 - 5.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-05-28T10:11Z
(-12.0h, +12.0h)
|
----
|
20.0
|
2022-05-26T12:56Z |
45.25
|
Max Kp Range: 3.0 - 6.0
|
Other (SIDC)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-05-28T02:00Z
(-9.0h, +9.0h)
|
----
|
70.0
|
2022-05-26T17:50Z |
32.17
|
Max Kp Range: 2.0 - 6.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-05-27T19:50Z
(-7.0h, +8.0h)
|
----
|
24.0
|
2022-05-26T22:10Z |
21.67
|
----
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-05-27T20:00Z
(-12.0h, +12.0h)
|
----
|
30.0
|
2022-05-26T22:35Z |
21.42
|
Max Kp Range: 3.0 - 4.0
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-05-27T21:20Z
(-12.0h, +12.0h)
|
----
|
----
|
2022-05-27T06:00Z |
15.33
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-05-28T10:42Z
(-12.0h, +12.0h)
|
----
|
----
|
2022-05-27T06:02Z |
28.67
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-05-28T05:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-05-27T12:09Z |
16.85
|
Max Kp Range: 3.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-05-28T04:03Z
|
----
|
36.0
|
--- |
--- |
Max Kp Range: 2.8 - 5.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-05-23T12:36:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: The likely source is an C5.2 class flare associated eruption from AR3017 (about N14W23). Brightening is seen SDO AIA 131 while an EUV wave is seen propagating to the south and east towards the central meridian.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-05-28T15:30Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-05-23T18:05Z |
117.42
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-05-29T11:26Z
(-12.0h, +12.0h)
|
----
|
5.0
|
2022-05-24T13:05Z |
118.35
|
Max Kp Range: 3.0 - 4.0
|
Other (SIDC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-05-29T01:28Z
|
----
|
5.0
|
--- |
--- |
Max Kp Range: 2.5 - 3.5
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-05-21T00:12:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: The likely source is an eruption from AR3011 (N18W31) which was associated with a C5.2 class flare occurring around 2022-05-20T23:30Z. After the brightening, filament material is ejected to the north and west as seen in SDO AIA 304A. Soon after this eruption, a complex signature is observed in SOHO running difference imagery with a large, faint and fast shock on the order of >1000 km/s emanating to the north which may or may not be associated with this flare. UPDATE (2022-05-24) from LASSOS Team: There is a structure in solar wind beginning before 2022-05-23T18:00Z with some elements of a weak flux rope signature (namely, smooth rotation), but it is very short and there is no magnetic amplification and the solar wind density, speed, and temperature are inconclusive. There may be a Solar Sector Boundary Crossing in this signature.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-05-23T07:00Z
(-12.0h, +12.0h)
|
----
|
20.0
|
2022-05-21T18:07Z |
36.88
|
Max Kp Range: 2.0 - 5.0
|
Other (SIDC)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-05-23T17:00Z
(-12.0h, +12.0h)
|
----
|
20.0
|
2022-05-21T18:11Z |
46.82
|
Max Kp Range: 2.0 - 5.0
|
Other (SIDC)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-05-24T11:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-05-22T18:37Z |
40.38
|
Max Kp Range: 3.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-05-23T16:19Z
(-15.6h, +17.8h)
|
----
|
66.0
|
2022-05-22T19:12Z |
21.12
|
Max Kp Range: 3.0 - 6.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-05-24T00:25Z
|
----
|
----
|
2022-05-22T19:35Z |
28.83
|
Max Kp Range: 3.0 - 5.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-05-24T00:00Z
(-6.0h, +6.0h)
|
----
|
30.0
|
2022-05-23T02:42Z |
21.30
|
Max Kp Range: 3.0 - 4.0
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-05-23T20:37Z
|
----
|
34.0
|
--- |
--- |
Max Kp Range: 2.66667 - 4.83333
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-05-17T09:23:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Visible in the NW of STEREO A COR2 and as a partial halo NNE in SOHO LASCO C2/C3. May be associated with an eruption from AR 13011 (N16E20), visible in SDO AIA 193 starting around 2022-05-17T08:21Z. Also associated with a double flare from AR 13011. UPDATE (2022-05-24) from LASSOS Team: Bz rotation at the end of 2022-05-21 but it is very short and there are no clear coincidental ICME signatures and no magnetic shock at L1 associated with it. If there is an ICME arrival, it comes at the back of a High Speed Stream, and the ICME signature is extremely weak.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-05-21T17:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-05-17T20:29Z |
92.52
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-05-21T17:00Z
|
----
|
----
|
--- |
--- |
Max Kp Range: 2.0 - 4.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-05-17T06:48:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: This CME is observed to the south in SOHO LASCO C2/C3. It is also observed to the SW in STEREO A COR2, but is partially obscured by streamer. The source signature for this CME is an eruption from Active Region 31010 (S16E21) with an associated C2.9 flare as seen in SDO AIA 131/193 starting around 2022-05-17T06:03Z. UPDATE (2022-05-24T11:30Z) from LASSOS Team: There is no clear magnetic shock at L1 associated with this ICME. If there is an ICME arrival, it comes at the back of a High Speed Stream, and the ICME signature is weak.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-05-20T05:30Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-05-17T16:50Z |
60.67
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Michelangelo Romano (M2M Office) |
Detail
|
| 2022-05-20T05:30Z
|
----
|
----
|
--- |
--- |
Max Kp Range: 3.0 - 5.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-05-10T14:48:00-CME-001
|
| Actual Shock Arrival Time: 2022-05-13T21:00Z |
Observed Geomagnetic Storm Parameters:
----
CME Note: Visible in the SE and S of SOHO LASCO C2 and C3 and the far south of STEREO A COR2. Associated with an X1.5 flare from AR 3006 starting at 2022-05-10T13:50Z and a subsequent EUV wave seen in AIA 193 and EUVI A 195. The associated eruption is characterized by dimming best seen in SDO AIA 193. It is also seen in STEREO A EUVI 195. It overlaps with the CME first visible in the southeast of SOHO LASCO C2 at 2022-05-10T15:12Z, causing some confusion in its analysis, as there are two simultaneous fronts seen in the first few images of LASCO C2 but only one front clearly seen in COR2A and C3. UPDATE (2022-05-24T) from LASSOS Team: Signature indicating possible interaction of this CME and SIR starting after ~2022-05-14T10:00Z. This interaction makes shock less clear. The SIR clears the region of material that might otherwise propagate the shock. The ICME possibly started before the SIR start - at the end of 2022-05-13 there is a smooth B-field signature indicative of an ICME.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-05-13T23:00Z
(-7.0h, +7.0h)
|
2.00
|
----
|
2022-05-10T20:45Z |
72.25
|
Max Kp Range: 3.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-05-13T17:00Z
(-7.0h, +7.0h)
|
-4.00
|
----
|
2022-05-10T23:52Z |
69.13
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-05-13T23:30Z
(-12.0h, +12.0h)
|
2.50
|
60.0
|
2022-05-11T13:15Z |
55.75
|
Max Kp Range: 3.0 - 6.0
|
Other (SIDC)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-05-14T04:00Z
(-7.0h, +7.0h)
|
7.00
|
----
|
2022-05-11T18:56Z |
50.07
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-05-13T22:52Z
|
1.87
|
60.0
|
--- |
--- |
Max Kp Range: 2.75 - 4.5
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-05-06T21:24:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Visible in the NE in SOHO LASCO C2/C3 and in the NNW in STEREO A COR2. Associated with field line rising faintly visible over NW limb in SDO AIA 171 beginning 2022-05-06T18:45Z. Associated with filament eruption centered near N40E40, visible in SDO AIA 304 beginning 2022-05-06T19:03Z. Complicated leading edge structure with two apparent leading edges, but the entire structure is moving together. Analysis of L1 signature on 05-10 and 05-11 by LASSOS: No CME on 05-10: magnetic field components do not display smooth rotations, the proton density is not low, and the ion temperature is really low but has been low starting with 05-08. 05-10: increases in the magnetic field, proton density, and bulk speed are probably happening because the faster solar wind is catching up to the slower solar wind and compression is happening at the interface. If we look at late 05-12 and beyond, the sharp increases on 05-11 are associated with a possible SIR (see around 12:00 on May 12).
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-05-11T11:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-05-07T12:25Z |
94.58
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-05-10T15:00Z
|
----
|
40.0
|
2022-05-07T22:05Z |
64.92
|
Max Kp Range: 5.0 - --
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-05-10T20:00Z
(-13.0h, +13.0h)
|
----
|
----
|
2022-05-08T00:30Z |
67.50
|
----
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-05-10T21:00Z
(-12.0h, +12.0h)
|
----
|
35.0
|
2022-05-09T10:22Z |
34.63
|
Max Kp Range: 3.0 - 5.0
|
Other (SIDC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-05-10T22:45Z
|
----
|
37.5
|
--- |
--- |
Max Kp Range: 3.33333 - 4.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-05-03T18:12:00-CME-001
|
| Actual Shock Arrival Time: 2022-05-08T06:24Z |
Observed Geomagnetic Storm Parameters:
Max Kp: 3.0
CME Note: CME is seen to the NE in SOHO LASCO C2/C3 and to the NW in STEREO A COR2 imagery. The source is likely the dimming seen near disk center above AR 3004 in SDO AIA 171 around 2022-05-03T15:00Z. This dimming is also observed to the west in STEREO A EUVI 195 around the same time. UPDATE (2022-05-09T16:27Z): Weak arrival signature indicated by sudden but weak field amplification (only to about 8.5 nT), accompanied by component rotation. Because the L1 solar wind is otherwise quiet, we can see an associated pileup beginning around 2022-05-08T08:03Z. The speed and temperature increase, but they're still pretty low at around 330-340 km/s and 25-35 kK, so these are inconclusive. There are potential signs of separate sheath and flux rope at 2022-05-08T06:24Z and 2022-05-08T12:43Z, respectively.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-05-08T08:00Z
(-7.0h, +7.0h)
|
1.60
|
----
|
2022-05-04T18:18Z |
84.10
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Mattie Anastopulos (M2M Office) |
Detail
|
| 2022-05-06T16:00Z
|
-38.40
|
----
|
2022-05-04T23:25Z |
78.98
|
Max Kp Range: 6.0 - 7.0
Dst min. in nT: -135
Dst min. time: 2022-05-07T12:00Z
|
Anemomilos
|
WKent Tobiska (SET SWD) |
Detail
|
| 2022-05-07T18:00Z
|
-12.40
|
40.0
|
2022-05-05T17:40Z |
60.73
|
Max Kp Range: -- - 5.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-05-08T09:00Z
(-7.0h, +7.0h)
|
2.60
|
----
|
2022-05-05T20:00Z |
58.40
|
----
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Mary Aronne (M2M) |
Detail
|
| 2022-05-07T16:52Z
|
-13.53
|
----
|
2022-05-06T03:04Z |
51.33
|
----
|
SPM
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-05-06T10:32Z
|
-43.87
|
----
|
2022-05-06T03:06Z |
51.30
|
----
|
SPM2
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-05-07T13:04Z
|
-17.33
|
40.0
|
--- |
--- |
Max Kp Range: 4.0 - 5.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-04-29T07:38:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Source is the eruption from AR 2996 (N25W40) starting around 2022-04-29T07:21Z seen in SDO AIA 131, 171, 193, and 304. Also visible on the NW limb of STA EUVI 195 around the same time. Post eruptive loops and dimming happens around 08:00Z. Associated with the M1.2 flare peaking at 07:30 from AR 2996.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-05-01T04:05Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-04-29T18:00Z |
34.08
|
Max Kp Range: 4.0 - 7.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-05-01T05:00Z
(-6.0h, +6.0h)
|
----
|
20.0
|
2022-04-29T19:57Z |
33.05
|
Max Kp Range: 4.0 - 7.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-05-01T23:43Z
|
----
|
----
|
2022-04-29T20:00Z |
51.72
|
Max Kp Range: 3.0 - 5.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-05-01T06:41Z
(-9.4h, +6.1h)
|
----
|
75.0
|
2022-04-29T23:04Z |
31.62
|
Max Kp Range: 3.0 - 7.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-05-02T05:00Z
(-12.0h, +12.0h)
|
----
|
20.0
|
2022-04-30T00:11Z |
52.82
|
Max Kp Range: 4.0 - 5.0
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-05-02T07:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-04-30T01:39Z |
53.35
|
----
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-05-01T16:34Z
|
----
|
38.3333
|
--- |
--- |
Max Kp Range: 3.6 - 6.2
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-04-27T14:53:00-CME-001
|
| Actual Shock Arrival Time: 2022-04-29T23:27Z |
Observed Geomagnetic Storm Parameters:
Max Kp: 5.0
CME Note: An eruption from the vicinity of AR2996 was observed using Stereo-A EUVI imagery around 2022-04-27T14:00Z, since a maneuver/calibration at SDO was occurring at the time of the eruption.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-04-30T08:30Z
(-7.0h, +7.0h)
|
9.05
|
----
|
2022-04-27T19:16Z |
52.18
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Mary Aronne (M2M) |
Detail
|
| 2022-04-30T08:43Z
(-1.0h, +1.0h)
|
9.27
|
6.0
|
2022-04-27T20:21Z |
51.10
|
Max Kp Range: 3.0 - 5.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Mattie Anastopulos (M2M Office) |
Detail
|
| 2022-04-29T22:39Z
|
-0.80
|
----
|
2022-04-27T21:00Z |
50.45
|
Max Kp Range: 3.0 - 5.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-04-29T18:35Z
(-9.0h, +9.0h)
|
-4.87
|
----
|
2022-04-27T21:00Z |
50.45
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-04-30T07:06Z
(-9.0h, +9.0h)
|
7.65
|
----
|
2022-04-27T21:00Z |
50.45
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-04-30T01:00Z
(-8.0h, +8.0h)
|
1.55
|
70.0
|
2022-04-28T00:52Z |
46.58
|
Max Kp Range: 4.0 - 6.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-04-29T22:00Z
(-6.0h, +6.0h)
|
-1.45
|
----
|
2022-04-28T02:39Z |
44.80
|
Max Kp Range: 5.0 - 6.0
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-04-30T04:00Z
|
4.55
|
70.0
|
2022-04-28T10:16Z |
37.18
|
Max Kp Range: 4.0 - 6.0
|
Cone+HAF (SEPC, NSSC, CAS)
|
Jingjing Wang (NSSC SEPC) |
Detail
|
| 2022-04-30T02:34Z
|
3.12
|
48.6667
|
--- |
--- |
Max Kp Range: 3.66667 - 5.5
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-04-27T08:48:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Source is the eruption from AR2996 around 2022-04-27T08:20Z seen in SDO AIA 131, 171, 193, and 304. Also seen in STA EUVI 195 and 304 in the NW quadrant. Associated with a C3.3 flare from AR2996.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-04-30T08:30Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-04-27T19:16Z |
61.23
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Mary Aronne (M2M) |
Detail
|
| 2022-04-30T08:43Z
(-1.0h, +1.0h)
|
----
|
6.0
|
2022-04-27T20:21Z |
60.37
|
Max Kp Range: 3.0 - 5.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Mattie Anastopulos (M2M Office) |
Detail
|
| 2022-04-30T08:36Z
|
----
|
6.0
|
--- |
--- |
Max Kp Range: 3.0 - 5.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-04-26T14:53:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: The eruption is likely associated with a small filament eruption from the vicinity of AR 2996 (N24W07) which erupts around 2022-04-26T14:24Z as seen in SDO AIA 304 with associated coronal dimming in SDO AIA 193.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-04-29T20:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-04-26T19:14Z |
72.77
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-04-29T06:06Z
|
----
|
----
|
2022-04-26T20:06Z |
58.00
|
Max Kp Range: 4.0 - 5.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-04-29T18:07Z
(-2.0h, +1.2h)
|
----
|
10.0
|
2022-04-26T23:27Z |
66.67
|
Max Kp Range: 3.0 - 5.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Mary Aronne (M2M) |
Detail
|
| 2022-04-29T10:01Z
(-9.0h, +9.0h)
|
----
|
----
|
2022-04-27T07:00Z |
51.02
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-04-29T12:03Z
(-9.0h, +9.0h)
|
----
|
----
|
2022-04-27T07:00Z |
53.05
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-04-29T13:15Z
|
----
|
10.0
|
--- |
--- |
Max Kp Range: 3.0 - 4.66667
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-04-21T02:36:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Visible in the NE of SOHO LASCO C2/C3 and the far north in STEREO A COR2. Associated with an M9.6 flare and eruption from AR 2933. The eruption is characterized by an EUV wave and opening field lines first seen around 2022-04-21T01:50Z and is followed by post eruptive arcades. It is also visible north of disk center as seen from STEREO A EUVI 195.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-04-25T00:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-04-21T16:26Z |
79.57
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-04-25T00:00Z
|
----
|
----
|
--- |
--- |
Max Kp Range: 2.0 - 3.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-04-11T06:00:00-CME-001
|
| Actual Shock Arrival Time: 2022-04-14T03:37Z |
Observed Geomagnetic Storm Parameters:
Max Kp: 6.0
CME Note: This CME is visible as a halo in SOHO LASCO C2/C3 and a partial halo in STEREO A COR2. The source is a C1.6 flare and eruption from an unnumbered region around S15E05. The eruption starts around 2022-04-11T05:00Z and is characterized by an EUV wave and dimming that is best seen in SDO AIA 193. The eruption can also be seen in SDO AIA 304. The eruption is visible in the SW quadrant of STEREO A EUVI imagery. As for the arrival, solar wind speed increased from ~400 km/s at 2022-04-14T03:00Z to 480 km/s at 09:20Z. Magnetic field components increase around 03:30Z with Btotal exceeding 10nT at 08:43Z, likely from the flux rope arrival. Density shows a gradual increase beginning at 03:30Z as well.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-04-14T08:00Z
(-7.0h, +7.0h)
|
4.38
|
----
|
2022-04-11T10:00Z |
65.62
|
Max Kp Range: -- - 6.0
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-04-14T09:56Z
(-7.0h, +7.0h)
|
6.32
|
----
|
2022-04-11T12:52Z |
62.75
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Mary Aronne (M2M) |
Detail
|
| 2022-04-14T04:31Z
|
0.90
|
----
|
2022-04-11T14:30Z |
61.12
|
Max Kp Range: 3.0 - 5.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-04-14T12:00Z
(-6.0h, +6.0h)
|
8.38
|
90.0
|
2022-04-11T17:02Z |
58.58
|
Max Kp Range: 4.0 - 6.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-04-14T09:34Z
(-10.2h, +12.2h)
|
5.95
|
100.0
|
2022-04-11T21:36Z |
54.02
|
Max Kp Range: 3.0 - 4.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-04-13T16:00Z
(-12.0h, +12.0h)
|
-11.62
|
80.0
|
2022-04-12T00:41Z |
50.93
|
Max Kp Range: 4.0 - 5.0
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-04-14T12:54Z
(-9.0h, +9.0h)
|
9.28
|
----
|
2022-04-12T07:00Z |
44.62
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-04-14T06:24Z
(-9.0h, +9.0h)
|
2.78
|
----
|
2022-04-12T07:00Z |
44.62
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-04-14T17:00Z
(-12.0h, +12.0h)
|
13.38
|
70.0
|
2022-04-12T08:21Z |
43.27
|
Max Kp Range: 3.0 - 5.0
|
Other (SIDC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-04-14T08:02Z
|
4.42
|
85.0
|
--- |
--- |
Max Kp Range: 3.33333 - 5.14286
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-04-09T09:12:00-CME-001
|
| Actual Shock Arrival Time: 2022-04-12T10:33Z |
Observed Geomagnetic Storm Parameters:
----
CME Note: Visible in the southwest of SOHO LASCO C2/C3 and STEREO A COR2. The source is a filament eruption seen slowly lifting off in the southwest of SDO AIA 304 starting around 2022-04-09T05:15Z. It is also visible in SDO AIA 193 and 171 and in the southwest of STEREO A EUVI 195. The CME sheath/shock arrived at 2022-04-12T10:33Z and the flux rope arrived at 2022-04-13T01:54Z. The flux rope arrival was used as the IPS entry arrival time in DONKI as the flux rope arrival was responsible for a 10nT threshold crossing in Btotal. Btotal had only reached a maximum Btotal of ~8nT for the shock arrival.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-04-12T22:00Z
(-7.0h, +7.0h)
|
11.45
|
----
|
2022-04-09T18:50Z |
63.72
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Mary Aronne (M2M) |
Detail
|
| 2022-04-13T02:00Z
(-6.0h, +6.0h)
|
15.45
|
40.0
|
2022-04-10T07:15Z |
51.30
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-04-13T22:00Z
(-12.0h, +12.0h)
|
35.45
|
30.0
|
2022-04-10T21:55Z |
36.63
|
Max Kp Range: 3.0 - 5.0
|
Other (SIDC)
|
Mary Aronne (M2M) |
Detail
|
| 2022-04-12T15:13Z
(-6.0h, +4.0h)
|
4.67
|
37.0
|
2022-04-11T13:00Z |
21.55
|
Max Kp Range: 3.0 - 4.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Mary Aronne (M2M) |
Detail
|
| 2022-04-13T03:18Z
|
16.75
|
35.6667
|
--- |
--- |
Max Kp Range: 2.75 - 4.25
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-04-04T11:36:00-CME-001
|
| Actual Shock Arrival Time: 2022-04-08T03:39Z |
Observed Geomagnetic Storm Parameters:
Max Kp: 4.0
CME Note: Partial halo CME mostly NE in SOHO LASCO C2/C3 and NE in COR2A. Its source is a filament eruption and opening field lines from the vicinity of AR 12983 (approximately N23E19). The arrival of this CME is marked by a weak shock with the magnetic field increasing to just above 10nT, and a jump in solar wind speed from ~365 km/s to 385 km/s and an increase in density to 15 particles/cc.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-04-08T06:00Z
(-7.0h, +7.0h)
|
2.35
|
----
|
2022-04-05T15:17Z |
60.37
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Michelangelo Romano (M2M Office) |
Detail
|
| 2022-04-08T00:23Z
(-6.1h, +8.9h)
|
-3.27
|
12.0
|
2022-04-06T04:16Z |
47.38
|
Max Kp Range: 2.0 - 4.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-04-08T03:11Z
|
-0.47
|
12.0
|
--- |
--- |
Max Kp Range: 2.0 - 3.5
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-04-03T16:38:00-CME-001
|
| Actual Shock Arrival Time: 2022-04-06T22:45Z |
Observed Geomagnetic Storm Parameters:
Max Kp: 3.0
CME Note: The source of this CME is a large filament eruption best seen in the SW quadrant of the Earth-facing disk in SDO/AIA 304 and along the western limb in a few frames of STEREO A EUVI 304. The CME is first visible to the SW in STEREO A COR2 followed by SOHO LASCO C2 and C3.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-04-06T12:00Z
|
-10.75
|
70.0
|
2022-04-03T05:44Z |
89.02
|
Max Kp Range: 4.0 - 6.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-04-05T22:00Z
(-12.0h, +12.0h)
|
-24.75
|
80.0
|
2022-04-04T11:08Z |
59.62
|
Max Kp Range: 4.0 - 6.0
|
Other (SIDC)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-04-06T09:44Z
(-7.0h, +7.0h)
|
-13.02
|
----
|
2022-04-04T21:38Z |
49.12
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-04-06T08:15Z
|
-14.50
|
----
|
2022-04-05T06:15Z |
40.50
|
Max Kp Range: 3.0 - 4.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-04-06T12:02Z
(-7.0h, +7.0h)
|
-10.72
|
----
|
2022-04-05T07:00Z |
39.75
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-04-06T13:42Z
(-9.0h, +9.0h)
|
-9.05
|
----
|
2022-04-05T07:00Z |
39.75
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-04-06T07:17Z
(-7.4h, +9.1h)
|
-15.47
|
100.0
|
2022-04-05T21:26Z |
25.32
|
Max Kp Range: 3.0 - 5.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-04-06T08:42Z
|
-14.05
|
83.3333
|
--- |
--- |
Max Kp Range: 3.4 - 5.2
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-04-02T13:38:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Large CME seen to the west in STEREO A COR2, in SOHO LASCO C2, and C3. The source of this CME is a M3.9 class flare from AR12975 peaking at 2022-04-02T13:55Z and the associated filament eruption. EUV wave is visible in SDO/AIA 171, 211, 193, and STEREO A EUVI 195. The eruption begins around 13:00Z.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-04-04T16:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-04-02T17:38Z |
46.37
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-04-04T12:47Z
|
----
|
----
|
2022-04-02T18:00Z |
42.78
|
Max Kp Range: 6.0 - 8.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-04-04T13:06Z
(-10.15h, +9.517h)
|
----
|
52.0
|
2022-04-03T01:18Z |
35.80
|
Max Kp Range: 3.0 - 5.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-04-04T01:48Z
(-9.0h, +9.0h)
|
----
|
----
|
2022-04-03T07:00Z |
18.80
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-04-04T22:41Z
(-9.0h, +9.0h)
|
----
|
----
|
2022-04-03T07:00Z |
39.68
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-04-04T13:16Z
|
----
|
52.0
|
--- |
--- |
Max Kp Range: 3.66667 - 5.66667
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-03-31T19:09:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Source is the M9.6-class flare from AR2975 peaking at 2022-03-31T18:35Z from N13W48. Associated eruption seen through the opening of field lines in STEREO A EUVI 195 from behind the west limb around 2022-03-31T19:15Z. Post eruptive darkening and an EUV wave is seen in SDO AIA 193 starting at 2022-03-31T18:31Z.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-04-04T03:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-04-01T14:12Z |
60.80
|
----
|
WSA-ENLIL + Cone (NASA M2M)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-04-05T03:32Z
(-12.0h, +12.0h)
|
----
|
15.0
|
2022-04-01T21:27Z |
78.08
|
Max Kp Range: 3.0 - 5.0
|
Other (SIDC)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-04-03T19:25Z
(-3.533h, +3.183h)
|
----
|
14.0
|
2022-04-02T03:31Z |
39.90
|
Max Kp Range: 2.0 - 4.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-04-04T08:39Z
|
----
|
14.5
|
--- |
--- |
Max Kp Range: 2.5 - 4.5
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-03-30T18:23:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Visible in the W in STEREO A COR2 and as an asymmetric halo slightly NW in SOHO LASCO C2/C3. Associated with X1.3 flare from AR 12975, eruption visible in SDO AIA 131/171/193/304 and STEREO A EUVI 195 beginning 2022-03-30T17:30Z.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-04-02T05:41Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-03-30T21:48Z |
55.88
|
Max Kp Range: 4.0 - 7.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-04-02T06:38Z
|
----
|
----
|
2022-03-30T22:30Z |
56.13
|
Max Kp Range: 4.0 - 6.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-04-02T06:21Z
|
----
|
----
|
2022-03-31T08:41Z |
45.67
|
----
|
SPM
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-04-02T02:37Z
|
----
|
----
|
2022-03-31T08:44Z |
41.88
|
----
|
SPM2
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-04-03T15:00Z
|
----
|
----
|
2022-03-31T09:26Z |
77.57
|
----
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-04-02T06:36Z
(-9.0h, +9.0h)
|
----
|
----
|
2022-03-31T22:30Z |
32.10
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-04-02T13:14Z
(-9.0h, +9.0h)
|
----
|
----
|
2022-03-31T22:30Z |
38.73
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-04-02T12:25Z
(-8.3h, +12.0h)
|
----
|
100.0
|
2022-04-01T01:42Z |
34.72
|
Max Kp Range: 3.0 - 5.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-04-01T23:30Z
(-12.0h, +12.0h)
|
----
|
15.0
|
2022-04-01T21:21Z |
2.15
|
Max Kp Range: 3.0 - 5.0
|
Other (SIDC)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-04-02T10:13Z
|
----
|
57.5
|
--- |
--- |
Max Kp Range: 3.5 - 5.75
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-03-28T20:23:00-CME-001
|
| Actual Shock Arrival Time: 2022-03-31T01:41Z |
Observed Geomagnetic Storm Parameters:
----
CME Note: This CME is observed as a halo structure in both SOHO LASCO C2/C3 and STEREO A COR2 white light coronagraph imagery. It is associated with an M1.0 flare from Active Region 12975 (N12W06) and eruption signature visible in SDO AIA 171/193 exhibiting a notable brightening/field line movement starting around 2022-03-28T19:03Z. The shock from the combined front of this CME and preceding 2022-03-28T12:09Z CME is observed around 2022-03-31T01:41Z, followed by the the first flux rope (possibly the flux rope for2022-03-28T12:09Z CME) starting around 2022-03-31T012:00Z. We are likely seeing the start of another flux rope (possibly for 2022-03-28T20:23Z CME) slightly after 2022-04-01T12:00Z when there is a sudden increase in the magnetic field and a drop in density.
The end of this second ICME seems to happen on the morning of 2022-04-02 when the field becomes more turbulent, and density increases (analysis by Tarik Salman, LASSOS).
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-03-31T11:39Z
(-7.0h, +7.0h)
|
9.97
|
----
|
2022-03-29T07:00Z |
42.68
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-03-31T16:10Z
(-9.0h, +9.0h)
|
14.48
|
----
|
2022-03-29T07:00Z |
42.68
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-03-31T01:00Z
(-7.0h, +7.0h)
|
-0.68
|
----
|
2022-03-29T07:31Z |
42.17
|
Max Kp Range: 4.0 - 7.0
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-03-31T23:05Z
(-12.0h, +12.0h)
|
21.40
|
70.0
|
2022-03-29T13:01Z |
36.67
|
Max Kp Range: 3.0 - 6.0
|
Other (SIDC)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-03-31T04:12Z
(-7.0h, +7.0h)
|
2.52
|
----
|
2022-03-29T15:45Z |
33.93
|
Max Kp Range: 5.0 - 7.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Michelangelo Romano (M2M Office) |
Detail
|
| 2022-03-31T10:07Z
|
8.43
|
----
|
2022-03-29T17:37Z |
32.07
|
Max Kp Range: 4.0 - 6.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-03-31T12:00Z
|
10.32
|
----
|
2022-03-29T19:56Z |
29.75
|
----
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-03-31T06:10Z
(-6.7h, +5.9h)
|
4.48
|
100.0
|
2022-03-30T00:16Z |
25.42
|
Max Kp Range: 5.0 - 7.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-31T02:00Z
|
0.32
|
70.0
|
2022-03-30T01:05Z |
24.60
|
Max Kp Range: 5.0 - 7.0
|
Cone+HAF (SEPC, NSSC, CAS)
|
Jingjing Wang (NSSC SEPC) |
Detail
|
| 2022-03-31T15:29Z
|
13.80
|
----
|
2022-03-30T07:11Z |
18.50
|
----
|
SPM
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-03-31T07:00Z
|
5.32
|
----
|
2022-03-30T07:19Z |
18.37
|
----
|
SPM2
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-03-31T14:00Z
(-9.0h, +9.0h)
|
12.32
|
30.0
|
2022-03-31T15:05Z |
-13.40
|
Max Kp Range: 4.0 - 6.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-03-31T10:14Z
|
8.55
|
67.5
|
--- |
--- |
Max Kp Range: 4.28571 - 6.57143
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-03-28T12:09:00-CME-001
|
| Actual Shock Arrival Time: 2022-03-31T01:41Z |
Observed Geomagnetic Storm Parameters:
Max Kp: 5.0
CME Note: This CME is visible as a halo in SOHO LASCO C2/C3 and STEREO A COR2 white light imagery. It is associated with an M4.0 flare and eruption from AR 12975 (N12W01). The eruption is characterized by an EUV wave and dimming that is best seen in SDO AIA 193 around 2022-03-28T11:21Z. The eruption is also visible in the northwest quadrant from the viewpoint of STEREO A EUVI 195. The shock from what is probably the combined front of this CME and the 2022-03-28T20:23Z CME was observed around 2022-03-31T01:41Z, it was followed by the sheath and the CME flux rope starting around 2022-03-31T012:00Z (a more coherent magnetic field, rotations, and the sudden drop in proton density at the transition between the sheath to the CME flux rope). We might be seeing the second flux rope (possibly for 2022-03-28T20:23Z CME) slightly after 2022-04-01T12:00Z when there is a sudden increase in the magnetic field and a drop in density. (analysis by Tarik Salman, LASSOS)
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-03-31T10:17Z
(-9.0h, +9.0h)
|
8.60
|
----
|
2022-03-28T12:00Z |
61.68
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-03-31T09:58Z
(-9.0h, +9.0h)
|
8.28
|
----
|
2022-03-28T12:00Z |
61.68
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-03-31T08:49Z
(-7.0h, +7.0h)
|
7.13
|
----
|
2022-03-28T16:20Z |
57.35
|
Max Kp Range: 4.0 - 6.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-03-31T05:08Z
|
3.45
|
----
|
2022-03-28T18:00Z |
55.68
|
Max Kp Range: 4.0 - 5.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-03-31T10:51Z
(-6.1h, +6.2h)
|
9.17
|
100.0
|
2022-03-29T00:41Z |
49.00
|
Max Kp Range: 3.0 - 6.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-03-31T03:00Z
|
1.32
|
----
|
2022-03-29T00:59Z |
48.70
|
----
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-03-31T12:00Z
|
10.32
|
80.0
|
2022-03-29T02:40Z |
47.02
|
Max Kp Range: 4.0 - 6.0
|
Cone+HAF (SEPC, NSSC, CAS)
|
Jingjing Wang (NSSC SEPC) |
Detail
|
| 2022-03-31T07:24Z
|
5.72
|
----
|
2022-03-29T03:01Z |
46.67
|
----
|
SPM
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-03-30T22:44Z
|
-2.95
|
----
|
2022-03-29T03:04Z |
46.62
|
----
|
SPM2
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-03-31T01:00Z
(-7.0h, +7.0h)
|
-0.68
|
----
|
2022-03-29T07:31Z |
42.17
|
Max Kp Range: 4.0 - 7.0
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-03-31T06:29Z
(-12.0h, +12.0h)
|
4.80
|
70.0
|
2022-03-29T13:01Z |
36.67
|
Max Kp Range: 3.0 - 5.0
|
Other (SIDC)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-03-31T04:12Z
(-7.0h, +7.0h)
|
2.52
|
----
|
2022-03-29T15:45Z |
33.93
|
Max Kp Range: 5.0 - 8.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Michelangelo Romano (M2M Office) |
Detail
|
| 2022-03-31T12:00Z
|
10.32
|
----
|
2022-03-29T19:50Z |
29.85
|
----
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-03-31T06:10Z
(-6.7h, +5.9h)
|
4.48
|
100.0
|
2022-03-30T00:16Z |
25.42
|
Max Kp Range: 5.0 - 7.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-31T06:51Z
|
5.17
|
87.5
|
--- |
--- |
Max Kp Range: 4.0 - 6.25
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-03-25T06:12:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: This CME is first visible to the East in SOHO LASCO C2/C3 and to the SW in STEREO A COR2. As the CME propagates out of the field of view, the halo feature becomes more clear in both SOHO and STEREO A coronagraphs. The source of this CME is the M1.4 class flare from AR12974 (~S19E36) that peaked at 2022-03-25T05:26Z (based off of GOES-17 data). The flare and the associated EUV wave (which, as seen in SDO/AIA 193/171 seems to be directed mostly towards the West) are clearly seen in SDO/AIA 193, 171, 211, and 94. The associated dimming is not pronounced. There is a data gap in STEREO A EUVI 195 during this event, but a change in the associated Active Region is visible after the data gap. UPDATE (2022-03-29T20:05Z) from Fernando: I do not see any signature of an ICME any of the days [2022-03-27 to 03-28]. There is a clear SIR crossing, though.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-03-27T06:00Z
|
----
|
----
|
2022-03-25T18:00Z |
36.00
|
----
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-27T21:20Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-03-25T18:21Z |
50.98
|
Max Kp Range: 4.0 - 6.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-03-28T14:00Z
(-12.0h, +12.0h)
|
----
|
----
|
2022-03-25T21:46Z |
64.23
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-03-28T03:57Z
|
----
|
----
|
2022-03-25T22:00Z |
53.95
|
Max Kp Range: 3.0 - 5.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-03-27T23:00Z
(-10.0h, +10.0h)
|
----
|
80.0
|
2022-03-26T00:20Z |
46.67
|
Max Kp Range: 2.0 - 6.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-03-27T22:25Z
(-6.2h, +4.1h)
|
----
|
100.0
|
2022-03-26T03:59Z |
42.43
|
Max Kp Range: 4.0 - 7.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-03-28T12:00Z
(-12.0h, +12.0h)
|
----
|
40.0
|
2022-03-26T12:23Z |
47.62
|
Max Kp Range: 3.0 - 5.0
|
Other (SIDC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-28T10:00Z
|
----
|
70.0
|
2022-03-26T15:15Z |
42.75
|
Max Kp Range: 3.0 - 5.0
|
Cone+HAF (SEPC, NSSC, CAS)
|
Jingjing Wang (NSSC SEPC) |
Detail
|
| 2022-03-27T16:52Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-03-26T17:44Z |
23.13
|
Max Kp Range: 4.0 - 6.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-03-28T04:28Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-03-27T07:00Z |
21.47
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-03-28T04:02Z
(-9.0h, +9.0h)
|
----
|
----
|
2022-03-27T07:00Z |
21.03
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-03-28T01:38Z
|
----
|
72.5
|
--- |
--- |
Max Kp Range: 3.25 - 5.625
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-03-20T11:24:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Visible in the NE in SOHO LASCO C2 and in the NW in STEREO A COR2. Associated with an eruption from AR 12971 (N17E11), visible in SDO AIA 131/171/193/304 and STEREO A EUVI 195 beginning 2022-03-20T07:30Z.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-03-24T01:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-03-20T13:54Z |
83.10
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-23T15:30Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-03-20T16:35Z |
70.92
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-23T08:36Z
(-1.4h, +2.1h)
|
----
|
8.0
|
2022-03-20T23:36Z |
57.00
|
Max Kp Range: 3.0 - 5.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-24T12:00Z
(-12.0h, +12.0h)
|
----
|
20.0
|
2022-03-21T11:03Z |
72.95
|
Max Kp Range: 3.0 - 4.0
|
Other (SIDC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-24T23:00Z
|
----
|
50.0
|
2022-03-22T06:15Z |
64.75
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-03-24T13:46Z
|
----
|
----
|
2022-03-22T12:28Z |
49.30
|
----
|
SPM
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-03-24T01:40Z
|
----
|
26.0
|
--- |
--- |
Max Kp Range: 2.4 - 4.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
| 2022-03-23T09:48Z
|
----
|
----
|
2022-03-22T12:30Z |
21.30
|
----
|
SPM2
|
Xinhua Zhao (NSSC CAS) |
Detail
|
|
|
CME: 2022-03-16T13:36:00-CME-001
|
| Actual Shock Arrival Time: 2022-03-19T20:57Z |
Observed Geomagnetic Storm Parameters:
----
CME Note: Filament eruption begins around 2022-03-16T12:35Z and is seen well in SDO AIA 131, 171, 193, 304 and STEREO A EUVI 195 in the NE quadrant. Following this, brightening and an associated EUV wave is visible in STEREO A EUVI 195 and SDO AIA 193. Post eruptive arcades are then visible in SDO AIA 171 and 193 at 13:24Z. Arrival Note: Gradual field amplification accompanied by flux rope and pileup. Field amplitude only exceeds 10 nT for one data point at 2022-03-20T07:00Z, and there is no clear sudden shock. Associated with Kp reaching 3 during synoptic periods 2022-03-20T00:00Z-06:00Z and slight magnetospheric compression to about 8.5 Re at 2022-03-20T03:38Z.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-03-20T00:14Z
(-7.0h, +7.0h)
|
3.28
|
----
|
2022-03-16T20:35Z |
72.37
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-03-19T05:00Z
(-7.0h, +7.0h)
|
-15.95
|
----
|
2022-03-16T21:27Z |
71.50
|
----
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Mattie Anastopulos (M2M Office) |
Detail
|
| 2022-03-19T12:21Z
|
-8.60
|
----
|
2022-03-17T04:00Z |
64.95
|
Max Kp Range: 3.0 - 4.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-03-20T20:00Z
(-12.0h, +12.0h)
|
23.05
|
30.0
|
2022-03-17T09:38Z |
59.32
|
Max Kp Range: 3.0 - 4.0
|
Other (SIDC)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-03-19T22:20Z
(-12.0h, +20.0h)
|
1.38
|
100.0
|
2022-03-17T18:58Z |
49.98
|
Max Kp Range: 3.0 - 4.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-03-20T15:00Z
|
18.05
|
----
|
2022-03-17T19:08Z |
49.82
|
----
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-03-20T07:13Z
|
10.27
|
----
|
2022-03-18T02:50Z |
42.12
|
----
|
SPM
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-03-19T11:59Z
|
-8.97
|
----
|
2022-03-18T02:54Z |
42.05
|
----
|
SPM2
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-03-19T23:45Z
|
2.80
|
65.0
|
--- |
--- |
Max Kp Range: 3.0 - 4.25
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-03-10T19:23:00-CME-001
|
| Actual Shock Arrival Time: 2022-03-13T10:11Z |
Observed Geomagnetic Storm Parameters:
Max Kp: 6.0
CME Note: Visible in the NW of STEREO A COR2 and as a halo in SOHO LASCO C2/C3. Associated with an eruption, dimming, and EUV wave SE of AR2962 (N12W12), best seen in SDO AIA 171/193 starting around 2022-03-10T18:42Z. Associated with below-threshold increase in greater than 10 MeV proton flux at GOES-P beginning 2022-03-10T23:15Z and below-threshold increase in 13-100 MeV proton flux at STEREO A IMPACT beginning 2022-03-11T01:00Z. | ARRIVAL NOTE UPDATE - from DONKI IPS entry (2022-03-13T06:35:00-IPS-001): Sudden jump in magnetic field amplitude reaching 20 nT as well as a jump in speed, density, and temperature. A subsequent rotation can be seen in the B-field components with a decrease in temperature indicating a flux rope passage. Bz mostly north during the flux rope passage starting around 2022-03-13T22:00Z.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-03-13T21:00Z
(-7.0h, +7.0h)
|
10.82
|
----
|
2022-03-11T04:00Z |
54.18
|
----
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-14T00:00Z
(-12.0h, +12.0h)
|
13.82
|
----
|
2022-03-11T06:00Z |
52.18
|
Max Kp Range: 4.0 - 6.0
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-03-13T23:00Z
(-6.0h, +6.0h)
|
12.82
|
80.0
|
2022-03-11T06:30Z |
51.68
|
Max Kp Range: 4.0 - 6.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-03-13T15:59Z
(-7.0h, +7.0h)
|
5.80
|
----
|
2022-03-11T07:00Z |
51.18
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-03-13T16:38Z
(-9.0h, +9.0h)
|
6.45
|
----
|
2022-03-11T07:00Z |
51.18
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-03-13T11:35Z
(-7.0h, +7.0h)
|
1.40
|
----
|
2022-03-11T13:48Z |
44.38
|
Max Kp Range: 5.0 - 8.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-14T01:00Z
|
14.82
|
70.0
|
2022-03-11T14:20Z |
43.85
|
Max Kp Range: 5.0 - 7.0
|
Cone+HAF (SEPC, NSSC, CAS)
|
Jingjing Wang (NSSC SEPC) |
Detail
|
| 2022-03-13T11:51Z
|
1.67
|
----
|
2022-03-11T14:30Z |
43.68
|
Max Kp Range: 4.0 - 5.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-03-13T18:00Z
(-12.0h, +12.0h)
|
7.82
|
80.0
|
2022-03-11T15:29Z |
42.70
|
Max Kp Range: 4.0 - 7.0
|
Other (SIDC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-13T09:11Z
(-7.5h, +9.2h)
|
-1.00
|
97.0
|
2022-03-11T18:23Z |
39.80
|
Max Kp Range: 5.0 - 7.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-13T12:36Z
|
2.42
|
----
|
2022-03-13T01:55Z |
8.27
|
----
|
SPM
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-03-13T08:01Z
|
-2.17
|
----
|
2022-03-13T01:56Z |
8.25
|
----
|
SPM2
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-03-13T16:24Z
|
6.22
|
81.75
|
--- |
--- |
Max Kp Range: 4.42857 - 6.57143
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-03-10T02:00:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Visible in the SE in SOHO LASCO C2/C3 and as a southward halo in STEREO A COR2. Associated with a filament eruption centered near S40E50, visible in SDO AIA 131/171/193/304 and STEREO A EUVI 195/304 beginning 2022-03-09T21:30Z. Second of a 2-CME eruption from this filament.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-03-13T21:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-03-10T16:09Z |
76.85
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-13T13:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-03-10T21:29Z |
63.52
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Michelangelo Romano (M2M Office) |
Detail
|
| 2022-03-13T11:43Z
(-0.5h, +0.5h)
|
----
|
8.0
|
2022-03-11T00:05Z |
59.63
|
Max Kp Range: 3.0 - 5.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-13T18:00Z
(-12.0h, +12.0h)
|
----
|
80.0
|
2022-03-11T14:30Z |
51.50
|
Max Kp Range: 4.0 - 6.0
|
Other (SIDC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-13T15:00Z
|
----
|
----
|
2022-03-12T02:26Z |
36.57
|
Max Kp Range: 3.0 - 4.0
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-03-13T18:58Z
|
----
|
----
|
2022-03-13T02:17Z |
16.68
|
----
|
SPM
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-03-12T23:32Z
|
----
|
0.0
|
2022-03-13T02:21Z |
-2.82
|
----
|
SPM2
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-03-13T13:53Z
|
----
|
29.3333
|
--- |
--- |
Max Kp Range: 2.8 - 4.6
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-03-10T00:12:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Visible in the SE in SOHO LASCO C2/C3 and as a southward halo in STEREO A COR2. Associated with a filament eruption centered near S40E50, visible in SDO AIA 131/171/193/304 and STEREO A EUVI 195/304 beginning 2022-03-09T21:30Z. First of a 2-CME eruption from this filament.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-03-13T23:00Z
|
----
|
20.0
|
2022-03-10T13:22Z |
81.63
|
Max Kp Range: 2.0 - 5.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-03-13T21:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-03-10T16:09Z |
76.85
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-13T13:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-03-10T21:29Z |
63.52
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Michelangelo Romano (M2M Office) |
Detail
|
| 2022-03-13T11:43Z
(-0.5h, +0.5h)
|
----
|
8.0
|
2022-03-11T00:05Z |
59.63
|
Max Kp Range: 3.0 - 5.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-13T18:00Z
(-12.0h, +12.0h)
|
----
|
80.0
|
2022-03-11T14:30Z |
51.50
|
Max Kp Range: 4.0 - 6.0
|
Other (SIDC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-13T17:52Z
|
----
|
----
|
2022-03-13T03:18Z |
14.57
|
----
|
SPM
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-03-13T17:25Z
|
----
|
36.0
|
--- |
--- |
Max Kp Range: 2.6 - 4.8
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-03-08T04:24:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: The likely source is an eruption from the vicinity of Active Region 2958. Dimming and opening magnetic field lines as well as an EUV wave are observed in SDO AIA 193 A starting around 2022-03-08T03:24Z, while in SDO 304 A, longitudinal brightening occurs along the active region with ejecta and bright post eruptive loops. UPDATE (2022-03-11T19:55Z): There is a weak magnetic shock at 2022-03-11T10:59Z that may possibly be associated with this CME, but the solar wind density data are inconclusive and the solar wind speed and temperature data do not support a CME arrival, and this may be part of the previous CME arrival signature which began 2022-03-10T18:37Z.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-03-11T20:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-03-08T18:15Z |
73.75
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Mary Aronne (M2M) |
Detail
|
| 2022-03-10T23:02Z
|
----
|
----
|
2022-03-08T20:00Z |
51.03
|
Max Kp Range: 4.0 - 5.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-03-12T03:00Z
(-8.0h, +4.0h)
|
----
|
30.0
|
2022-03-08T22:50Z |
76.17
|
Max Kp Range: 4.0 - 2.0
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-03-11T22:00Z
(-7.0h, +7.0h)
|
----
|
1.0
|
2022-03-09T01:43Z |
68.28
|
Max Kp Range: 2.0 - 3.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-03-11T17:00Z
|
----
|
15.5
|
--- |
--- |
Max Kp Range: 3.0 - 3.25
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-03-07T00:12:00-CME-001
|
| Actual Shock Arrival Time: 2022-03-10T18:37Z |
Observed Geomagnetic Storm Parameters:
Max Kp: 4.0
CME Note: This CME is first seen as a faint partial halo to the NW in SOHO LASCO C2 (later in C3) and followed by a more bright and slightly more narrow shape to the W/NW in STEREO A COR2. The source of this CME is an eruption to the E/SE of AR12958 (N17W28) stretching across multiple longitudes from ~W20 to ~W45 based off of the dimming signature seen in SDO/AIA 193. The eruption is best seen in the SDO/AIA 193, 211, 94, 335, and STEREO A EUVI 195 wavelengths. From STEREO A's point of view, the eruption appears as opening field lines along the Eastern limb, while in SDO/AIA's point of view, the eruption is more clear with dimming, a post-eruptive arcade, and a brief EUV wave (seen best in SDO/AIA 211). UPDATE (2022-03-11T14:50Z): Arrival Field indicated by enhancement exceeding 10 nT, accompanied by field component rotation. Preceded by pileup, followed by slight speed increase. Temperature data inconclusive.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-03-10T13:38Z
(-7.0h, +7.0h)
|
-4.98
|
----
|
2022-03-07T20:25Z |
70.20
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-03-10T15:00Z
(-6.0h, +6.0h)
|
-3.62
|
60.0
|
2022-03-08T00:26Z |
66.18
|
Max Kp Range: 4.0 - 5.0
Dst min. in nT: -30
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-03-10T00:17Z
|
-18.33
|
----
|
2022-03-08T01:00Z |
65.62
|
Max Kp Range: 3.0 - 4.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-03-10T11:26Z
(-2.8h, +2.317h)
|
-7.18
|
6.0
|
2022-03-08T02:22Z |
64.25
|
Max Kp Range: 2.0 - 4.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-03-10T10:48Z
|
-7.82
|
----
|
2022-03-08T02:59Z |
63.63
|
----
|
SPM
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-03-09T11:39Z
|
-30.97
|
----
|
2022-03-08T03:01Z |
63.60
|
----
|
SPM2
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-03-10T21:00Z
|
2.38
|
----
|
2022-03-08T06:40Z |
59.95
|
----
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-03-11T07:00Z
(-12.0h, +12.0h)
|
12.38
|
60.0
|
2022-03-08T13:04Z |
53.55
|
Max Kp Range: 3.0 - 5.0
|
Other (SIDC)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-03-10T12:11Z
(-7.0h, +7.0h)
|
-6.43
|
----
|
2022-03-09T07:00Z |
35.62
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-03-10T01:48Z
(-9.0h, +9.0h)
|
-16.82
|
----
|
2022-03-09T07:00Z |
35.62
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-03-10T10:28Z
|
-8.15
|
42.0
|
--- |
--- |
Max Kp Range: 2.8 - 4.4
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-03-05T00:01:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-03-09T18:00Z
|
----
|
20.0
|
2022-03-06T03:30Z |
86.50
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-03-10T08:32Z
|
----
|
----
|
2022-03-06T06:19Z |
98.22
|
----
|
SPM
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-03-07T15:46Z
|
----
|
----
|
2022-03-06T06:23Z |
33.38
|
----
|
SPM2
|
Xinhua Zhao (NSSC CAS) |
Detail
|
| 2022-03-10T15:44Z
(-2.5h, +2.5h)
|
----
|
----
|
2022-03-09T20:30Z |
19.23
|
----
|
ELEvoHI
|
Tanja Amerstorfer (SRI) |
Detail
|
| 2022-03-09T14:30Z
|
----
|
20.0
|
--- |
--- |
Max Kp Range: 3.0 - 5.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-03-02T18:24:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: The CME is associated with the M2.0 class from Active Region 12958 (N18E27) peaking at 2022-03-02T17:39Z and the eruption marked by an EUV wave and seen in EUVI A 195 and AIA 193 after 2022-03-02T17:45Z. UPDATE (2022-03-09T17:45Z): There is no conclusive arrival signature for this ICME. The L1 solar wind signature is dominated by the 2022-03-05 high speed stream.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-03-06T09:00Z
|
----
|
----
|
2022-03-02T23:36Z |
81.40
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-03-06T12:00Z
|
----
|
30.0
|
2022-03-03T13:20Z |
70.67
|
Max Kp Range: 2.0 - 5.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-03-06T05:00Z
|
----
|
30.0
|
2022-03-03T15:12Z |
61.80
|
Max Kp Range: 3.0 - 6.0
|
Other (SIDC)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-03-06T17:00Z
|
----
|
----
|
2022-03-04T03:20Z |
61.67
|
Max Kp Range: 4.0 - 5.0
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-03-06T04:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-03-04T22:07Z |
29.88
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Chris Stubenrauch (M2M Office) |
Detail
|
| 2022-03-06T09:24Z
|
----
|
30.0
|
--- |
--- |
Max Kp Range: 2.6 - 4.8
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-03-02T15:04:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Faint CME is likely associated with an eruption marked by the relatively small area dimming in the vicinity of AR2956 visible in SDO AIA 193 imagery starting around 2022-03-02T14:45Z. UPDATE (2022-03-09T17:41Z): There is a short-duration field component rotation beginning 2022-03-05T10:30Z that may possibly be an arrival signature for this ICME, but the L1 solar wind signature is dominated by the 2022-03-05 high speed stream and an ICME signature is inconclusive.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-03-05T22:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-03-02T19:47Z |
74.22
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-03-06T22:00Z
|
----
|
10.0
|
2022-03-04T03:20Z |
66.67
|
Max Kp Range: 3.0 - 4.0
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-03-06T10:00Z
|
----
|
10.0
|
--- |
--- |
Max Kp Range: 2.5 - 4.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-02-19T10:23:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Visible as a partial halo N in STEREO A COR2, visible in NE of SOHO LASCO C2/C3. Source inconclusive, but possibly associated with some dimming/brightening in STEREO A EUVI 195 between 2022-02-19T05:45Z and 2022-02-19T08:55Z (data gap) and in SDO AIA 193 beginning around 2022-02-19T06:15Z.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-02-22T12:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-02-22T14:10Z |
-2.17
|
Max Kp Range: 3.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Michelangelo Romano (M2M Office) |
Detail
|
| 2022-02-22T12:00Z
|
----
|
----
|
--- |
--- |
Max Kp Range: 3.0 - 4.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-02-06T15:38:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
Max Kp: 5.0
CME Note: This CME is visible in the far north of SOHO LASCO C2 and in the northwest of STEREO A COR2. The source is unclear. It overlaps in STEREO A COR2 with the CME first seen in STEREO A COR2 at 2022-02-06T14:09Z, which was caused by a filament eruption near the Earth facing center disk. The L1 shock arrival of the combined front of this CME and 2022-02-06T14:09Z CME is around 2022-02-09T20:09Z and the flux rope part possibly starts around mid-day on 2022-02-10.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-02-09T23:08Z
(-7.0h, +7.0h)
|
|
----
|
2022-02-06T22:17Z |
69.87
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Mary Aronne (M2M) |
Detail
|
| 2022-02-09T14:09Z
(-7.1h, +7.0h)
|
|
100.0
|
2022-02-06T23:11Z |
68.97
|
Max Kp Range: 4.0 - 6.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-02-09T18:38Z
|
|
100.0
|
--- |
--- |
Max Kp Range: 3.5 - 5.5
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-02-06T14:09:00-CME-001
|
| Actual Shock Arrival Time: 2022-02-09T20:09Z |
Observed Geomagnetic Storm Parameters:
Max Kp: 5.0
CME Note: This is a partial halo CME as seen in the west of STEREO A COR2 and is seen in the far south of SOHO LASCO C2/C3. The source is an eruption beginning around 2022-02-06T12:04Z near AR 12939 characterized by a filament eruption best seen seen in SDO AIA 304, dimming and an EUV wave in SDO AIA 193, and opening field lines in SDO AIA 171. The L1 shock arrival of the combined front of this CME and 2022-02-06T15:38 CME is around 2022-02-09T20:09Z and the flux rope part possibly starts around mid-day on 2022-02-10.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-02-09T22:30Z
(-7.0h, +7.0h)
|
2.35
|
----
|
2022-02-06T19:10Z |
72.98
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Mary Aronne (M2M) |
Detail
|
| 2022-02-09T11:07Z
|
-9.03
|
----
|
2022-02-06T20:30Z |
71.65
|
Max Kp Range: 3.0 - 5.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-02-09T23:08Z
(-7.0h, +7.0h)
|
2.98
|
----
|
2022-02-06T22:17Z |
69.87
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Mary Aronne (M2M) |
Detail
|
| 2022-02-09T14:09Z
(-7.1h, +7.0h)
|
-6.00
|
100.0
|
2022-02-06T23:11Z |
68.97
|
Max Kp Range: 4.0 - 6.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-02-09T10:00Z
|
-10.15
|
----
|
2022-02-07T01:15Z |
66.90
|
Max Kp Range: 4.0 - 6.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-02-10T01:00Z
(-7.0h, +7.0h)
|
4.85
|
----
|
2022-02-07T04:00Z |
64.15
|
----
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-02-09T19:26Z
(-9.0h, +9.0h)
|
-0.72
|
----
|
2022-02-07T07:00Z |
61.15
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-02-09T13:42Z
(-9.0h, +9.0h)
|
-6.45
|
----
|
2022-02-07T07:00Z |
61.15
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-02-09T12:00Z
(-12.0h, +12.0h)
|
-8.15
|
75.0
|
2022-02-07T10:29Z |
57.67
|
Max Kp Range: 3.0 - 6.0
|
Other (SIDC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-02-09T19:00Z
|
-1.15
|
----
|
2022-02-08T02:55Z |
41.23
|
----
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-02-09T17:00Z
|
-3.15
|
87.5
|
--- |
--- |
Max Kp Range: 3.33333 - 5.5
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-01-29T23:36:00-CME-001
|
| Actual Shock Arrival Time: 2022-02-01T21:37Z |
Observed Geomagnetic Storm Parameters:
Max Kp: 4.0
CME Note: Visible as a halo in SOHO LASCO C2/C3 and as a partial halo to the W in STEREO A COR2. Associated with an eruption from AR 12936 (N17E10), visible in SDO AIA 171/193 (eruption/EUV wave) and SDO AIA 304 (post-eruptive arcades) beginning 2022-01-29T21:57Z. Also visible in STEREO A EUVI 195 beginning 2022-01-29T22:05Z. Associated with elevated 0.035-0.065 MeV electron flux at STEREO A beginning 2022-01-30T00:15Z and elevated 2.2-12 MeV proton flux at STEREO A beginning 2022-01-30T00:59Z. 13-100 MeV proton flux at STEREO A remained at background level. UPDATE (2022-02-02T12:35Z): Arrival indicated by sudden jumps in density (exceeding 15 per cc), speed (exceeding 470 km/s), temperature, and field amplitude (exceeding 13 nT). This IPS arrival time is the arrival of the sheath, and the flux rope arrived around 2022-02-02T19:43Z.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-02-01T23:07Z
(-9.0h, +9.0h)
|
1.50
|
----
|
2022-01-30T12:00Z |
57.62
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-02-01T21:29Z
(-9.0h, +9.0h)
|
-0.13
|
----
|
2022-01-30T12:00Z |
57.62
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-02-02T12:00Z
(-12.0h, +12.0h)
|
14.38
|
80.0
|
2022-01-30T12:47Z |
56.83
|
Max Kp Range: 3.0 - 6.0
|
Other (SIDC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-02-01T19:36Z
(-7.0h, +7.0h)
|
-2.02
|
----
|
2022-01-30T13:50Z |
55.78
|
Max Kp Range: 4.0 - 6.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-02-01T17:48Z
|
-3.82
|
----
|
2022-01-30T16:00Z |
53.62
|
Max Kp Range: 3.0 - 4.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-02-02T04:00Z
|
6.38
|
----
|
2022-01-30T16:43Z |
52.90
|
----
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-02-01T09:07Z
(-12.2h, +17.1h)
|
-12.50
|
100.0
|
2022-01-30T21:24Z |
48.22
|
Max Kp Range: 4.0 - 6.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-02-02T10:00Z
(-12.0h, +12.0h)
|
12.38
|
100.0
|
2022-01-31T00:11Z |
45.43
|
Max Kp Range: 5.0 - 6.0
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-02-02T00:00Z
(-7.0h, +7.0h)
|
2.38
|
----
|
2022-01-31T01:31Z |
44.10
|
----
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-02-02T01:00Z
|
3.38
|
70.0
|
2022-01-31T01:37Z |
44.00
|
Max Kp Range: 4.0 - 6.0
|
Cone+HAF (SEPC, NSSC, CAS)
|
Jingjing Wang (NSSC SEPC) |
Detail
|
| 2022-02-01T23:48Z
|
2.18
|
87.5
|
--- |
--- |
Max Kp Range: 3.83333 - 5.66667
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-01-25T13:25:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: This CME is faintly visible to the S/SE in SOHO LASCO C2/C3 and to the S/SW in STEREO A COR2. The potential source of this CME is an eruption associated with dimming seen around S40E15 in STEREO A EUVI 195 starting around 2022-01-25T10:35Z. This source could not be confirmed with SDO/AIA data due to an outage.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-01-29T00:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-01-26T17:49Z |
54.18
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-01-29T03:30Z
|
----
|
----
|
--- |
--- |
Max Kp Range: 2.5 - 3.5
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
| 2022-01-29T07:00Z
|
----
|
----
|
2022-01-26T23:50Z |
55.17
|
Max Kp Range: 3.0 - 4.0
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
|
|
CME: 2022-01-25T02:38:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: This CME is first visible to the NW in in STEREO A COR2 and to the N in SOHO LASCO C2/C3. The source of this CME is unclear due to a SDO/AIA data outage during the event and a data gap in STEREO A EUVI. The speculative source is AR12935 (N26E04) based off of an apparent eruption signature seen after the data gap in STEREO A EUVI 195.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-01-28T16:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-01-25T20:01Z |
67.98
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Mary Aronne (M2M) |
Detail
|
| 2022-01-28T16:00Z
|
----
|
----
|
--- |
--- |
Max Kp Range: 2.0 - 4.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-01-23T10:53:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Initially visible in the NW of STEREO A COR2, later (2022-01-23T14:30Z) visible in NE of SOHO LASCO C2/C3. Associated with a narrow filament eruption centered near N25E35, visible in SDO AIA 171/304 and STEREO A EUVI 304 beginning around 2022-01-23T08:00Z.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-01-26T18:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-01-23T16:12Z |
73.80
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-01-26T18:30Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-01-23T17:59Z |
72.52
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-01-26T13:27Z
(-1.1h, +1.3h)
|
----
|
6.0
|
2022-01-23T19:57Z |
65.50
|
Max Kp Range: 3.0 - 4.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-01-26T16:39Z
|
----
|
6.0
|
--- |
--- |
Max Kp Range: 2.33333 - 3.33333
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-01-22T12:38:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Visible in the NW in STEREO A COR2, NE in SOHO LASCO C2. Associated with a filament eruption near N40E20, visible in SDO AIA 171/193/304 and STEREO A EUVI 195 beginning 2022-01-22T06:35Z. There is a fainter envelope surrounding the clear leading edge in both coronagraphs.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-01-27T18:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-01-22T15:56Z |
122.07
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-01-26T00:00Z
|
----
|
----
|
2022-01-23T00:41Z |
71.32
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-01-26T21:00Z
|
----
|
----
|
--- |
--- |
Max Kp Range: 2.5 - 4.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-01-21T09:53:00-CME-001
|
| Actual Shock Arrival Time: 2022-01-24T17:09Z |
Observed Geomagnetic Storm Parameters:
----
CME Note: This CME is associated with a filament/prominence eruption visible toward the SE limb of the Earth-facing disk in SDO AIA 193/304 near S20E60 (near AR 2934) starting around 2022-01-21T07:45Z. A corresponding dimming/ejection of material is visible to the SE in STEREO A EUVI 195 starting around the same time. The CME appears as a partial halo in STEREO A COR2. This is a possible combined arrival with the 2022-01-20T09:09Z CME.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-01-24T12:00Z
(-7.0h, +7.0h)
|
-5.15
|
----
|
2022-01-21T16:23Z |
72.77
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Michelangelo Romano (M2M Office) |
Detail
|
| 2022-01-24T10:00Z
(-7.0h, +7.0h)
|
-7.15
|
----
|
2022-01-21T20:03Z |
69.10
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Michelangelo Romano (M2M Office) |
Detail
|
| 2022-01-24T00:58Z
(-7.0h, +8.1h)
|
-16.18
|
68.0
|
2022-01-21T23:42Z |
65.45
|
Max Kp Range: 3.0 - 5.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-01-24T01:23Z
(-7.0h, +7.0h)
|
-15.77
|
----
|
2022-01-22T07:00Z |
58.15
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-01-24T05:22Z
(-9.0h, +9.0h)
|
-11.78
|
----
|
2022-01-22T07:00Z |
58.15
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-01-24T05:56Z
|
-11.22
|
68.0
|
--- |
--- |
Max Kp Range: 2.33333 - 4.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-01-20T09:09:00-CME-001
|
| Actual Shock Arrival Time: 2022-01-24T17:09Z |
Observed Geomagnetic Storm Parameters:
----
CME Note: The source of this CME is a filament eruption visible in SDO/AIA 304 starting around 2022-01-20T08:00Z followed by notable dimming best seen in SDO/AIA 193 and some rising loops after the filament erupts (visible in both SDO/AIA 193 and 171). The source location is just NW of AR 12933. This is a possible combined arrival with the 2022-01-21T09:53Z CME.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-01-23T08:00Z
(-7.0h, +7.0h)
|
-33.15
|
----
|
2022-01-19T02:00Z |
135.15
|
----
|
WSA-ENLIL + Cone (NOAA/SWPC)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-01-24T06:00Z
(-7.0h, +7.0h)
|
-11.15
|
----
|
2022-01-20T17:35Z |
95.57
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Michelangelo Romano (M2M Office) |
Detail
|
| 2022-01-23T20:19Z
(-7.0h, +7.0h)
|
-20.83
|
----
|
2022-01-20T20:09Z |
93.00
|
Max Kp Range: 3.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Michelangelo Romano (M2M Office) |
Detail
|
| 2022-01-23T21:00Z
(-4.0h, +8.0h)
|
-20.15
|
50.0
|
2022-01-21T04:30Z |
84.65
|
Max Kp Range: 2.0 - 4.0
Dst min. in nT: -20
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-01-23T16:15Z
(-9.0h, +9.0h)
|
-24.90
|
----
|
2022-01-21T07:00Z |
82.15
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-01-23T09:10Z
(-9.0h, +9.0h)
|
-31.98
|
----
|
2022-01-21T07:00Z |
82.15
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-01-23T17:00Z
|
-24.15
|
50.0
|
2022-01-21T07:37Z |
81.53
|
Max Kp Range: 3.0 - 4.0
|
Cone+HAF (SEPC, NSSC, CAS)
|
Jingjing Wang (NSSC SEPC) |
Detail
|
| 2022-01-24T02:31Z
(-5.4h, +4.3h)
|
-14.63
|
62.0
|
2022-01-22T04:52Z |
60.28
|
Max Kp Range: 2.0 - 4.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-01-24T03:00Z
(-6.0h, +6.0h)
|
-14.15
|
30.0
|
2022-01-22T15:25Z |
49.73
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-01-23T19:28Z
|
-21.68
|
48.0
|
--- |
--- |
Max Kp Range: 2.5 - 4.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-01-19T06:23:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: This CME visible to the SW in STEREO A COR2 imagery is associated with a filament eruption centered near S50W20 visible in SDO AIA 304 starting as early as 2022-01-19T02:46Z. The event is very faintly seen as a partial halo to the SW in SOHO LASCO C2/C3 white light coronagraph imagery. There is some rotation-like behavior in the field components, but theres no magnetic shock and no arrival is supported by the density/speed/temperature data.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-01-23T03:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-01-19T20:05Z |
78.92
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Michelangelo Romano (M2M Office) |
Detail
|
| 2022-01-23T15:00Z
(-9.0h, +9.0h)
|
----
|
60.0
|
2022-01-20T08:00Z |
79.00
|
Max Kp Range: 2.0 - 5.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-01-23T09:00Z
|
----
|
60.0
|
--- |
--- |
Max Kp Range: 2.0 - 4.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-01-18T18:23:00-CME-001
|
| Actual Shock Arrival Time: 2022-01-21T12:55Z |
Observed Geomagnetic Storm Parameters:
----
CME Note: This CME is visible to the NW in SOHO LASCO C2/C3 and STEREO A COR2 imagery. It is associated with an M1.5 flare from AR 12929 (N07W53) and brightening/EUV wave visible in SDO AIA 193 starting aorund 2022-01-18T17:20Z. The source signature is also visible in STEREO A EUVI 195 toward the NW limb around the same time. The CME arrival includes weak magnetic shock and jumps in solar wind density/speed/temp, preceded by a weak pileup.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-01-21T11:00Z
(-7.0h, +7.0h)
|
-1.92
|
----
|
2022-01-18T23:54Z |
61.02
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-01-21T02:23Z
|
-10.53
|
----
|
2022-01-19T00:05Z |
60.83
|
Max Kp Range: 3.0 - 4.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-01-22T01:00Z
(-6.0h, +8.0h)
|
12.08
|
65.0
|
2022-01-19T02:48Z |
58.12
|
Max Kp Range: 3.0 - 4.0
Dst min. in nT: -25
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-01-20T20:53Z
(-9.0h, +9.0h)
|
-16.03
|
----
|
2022-01-19T07:00Z |
53.92
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-01-21T09:29Z
(-7.0h, +7.0h)
|
-3.43
|
----
|
2022-01-19T07:00Z |
53.92
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-01-21T18:00Z
(-12.0h, +12.0h)
|
5.08
|
30.0
|
2022-01-19T10:39Z |
50.27
|
Max Kp Range: 3.0 - 5.0
|
Other (SIDC)
|
Michelangelo Romano (M2M Office) |
Detail
|
| 2022-01-22T00:01Z
(-9.0h, +9.0h)
|
11.10
|
60.0
|
2022-01-19T12:30Z |
48.42
|
Max Kp Range: 3.0 - 5.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-01-21T14:01Z
(-4.983h, +3.55h)
|
1.10
|
12.0
|
2022-01-20T01:00Z |
35.92
|
Max Kp Range: 2.0 - 4.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-01-21T23:00Z
|
10.08
|
60.0
|
2022-01-20T09:53Z |
27.03
|
Max Kp Range: 3.0 - 5.0
|
Cone+HAF (SEPC, NSSC, CAS)
|
Jingjing Wang (NSSC SEPC) |
Detail
|
| 2022-01-21T13:45Z
|
0.83
|
45.4
|
--- |
--- |
Max Kp Range: 2.71429 - 4.28571
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-01-17T14:48:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-01-22T11:00Z
|
----
|
----
|
2022-01-18T04:15Z |
102.75
|
Max Kp Range: 4.0 - 5.0
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-01-21T11:00Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-01-18T18:01Z |
64.98
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-01-21T23:00Z
|
----
|
----
|
--- |
--- |
Max Kp Range: 3.0 - 4.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-01-16T20:48:00-CME-001
|
| Actual Shock Arrival Time: 2022-01-18T23:04Z |
Observed Geomagnetic Storm Parameters:
Max Kp: 6.0
CME Note: This CME is associated with a C2.6 flare from active region 12929 (N08W30). The eruption is characterized by opening field lines and dimming best seen in SDO AIA 193 starting around 2022-01-16T19:20Z. The eruption is also visible in the northwest in STEREO A EUVI 195 with the same source signatures. UPDATE: This arrival signature exhibits an increase B-tot from 5 to 9nT with a coinciding increase in density. A subsequent rotation can be seen in the B-field components corresponding with a decrease in temperature that is indicative of a flux rope passage.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-01-20T00:00Z
|
24.93
|
20.0
|
2022-01-18T03:18Z |
19.77
|
Max Kp Range: -- - 5.0
|
WSA-ENLIL + Cone (Met Office)
|
Met Office (Met Office) |
Detail
|
| 2022-01-20T09:00Z
|
33.93
|
----
|
2022-01-18T03:54Z |
19.17
|
Max Kp Range: 4.0 - 5.0
|
WSA-ENLIL + Cone (BoM)
|
Duty Forecaster (ASFC) |
Detail
|
| 2022-01-20T00:00Z
(-7.0h, +7.0h)
|
24.93
|
----
|
2022-01-18T18:01Z |
5.05
|
Max Kp Range: 2.0 - 3.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Anna Chulaki (M2M Office) |
Detail
|
| 2022-01-20T03:00Z
|
27.93
|
20.0
|
--- |
--- |
Max Kp Range: 3.0 - 4.33333
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-01-15T16:12:00-CME-001
|
| Actual Shock Arrival Time: 2022-01-18T23:04Z |
Observed Geomagnetic Storm Parameters:
Max Kp: 6.0
CME Note: The potential source is activity centered around N15W15, which includes an eruption with rising loops around 2022-01-15T12:00Z and eruption just south of the rising loops characterized by dimming around 2022-01-15T13:00Z. One of these eruptions is also potentially associated with the 2022-01-15T14:00Z CME, which overlaps with this CME in the coronagraphs.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-01-19T06:00Z
(-7.0h, +7.0h)
|
6.93
|
----
|
2022-01-16T15:31Z |
55.55
|
Max Kp Range: 2.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Mary Aronne (M2M) |
Detail
|
| 2022-01-19T12:00Z
(-12.0h, +12.0h)
|
12.93
|
20.0
|
2022-01-17T12:31Z |
34.55
|
Max Kp Range: 3.0 - 4.0
|
Other (SIDC)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-01-19T09:00Z
|
9.93
|
20.0
|
--- |
--- |
Max Kp Range: 2.5 - 4.0
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME: 2022-01-14T13:38:00-CME-001
|
| This CME was not detected at Earth! |
Observed Geomagnetic Storm Parameters:
----
CME Note: Visible in SW of STEREO A COR2 and SOHO LASCO C2/C3, moving quickly through the FOV. Associated with a large eruption from AR 12925 (S33W40), visible in SDO AIA 171/193/304 and STEREO A EUVI 195 beginning 2022-01-14T12:54Z. UPDATE: There appears to be a weak component rotation of two components of magnetic field at around 2022-01-17T14:00Z, preceded by drop in density/temperature. However, according to Lan, there is no sign of a shock and there appears to be no ICME arrival on 2022-01-17.
|
| Predicted Shock Arrival Time |
Difference (hrs) |
Confidence (%) |
Submitted On |
Lead Time (hrs) |
Predicted Geomagnetic Storm Parameter(s) |
Method |
Submitted By |
| 2022-01-16T14:39Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-01-14T17:22Z |
45.28
|
Max Kp Range: 3.0 - 4.0
|
WSA-ENLIL + Cone (NASA M2M)
|
Robert Loper (M2M Office) |
Detail
|
| 2022-01-16T15:03Z
|
----
|
----
|
2022-01-14T17:50Z |
45.22
|
Max Kp Range: 6.0 - 7.0
|
SARM
|
Marlon Nunez (UMA) |
Detail
|
| 2022-01-16T04:33Z
(-7.0h, +7.0h)
|
----
|
----
|
2022-01-15T07:00Z |
21.55
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-01-16T23:39Z
(-9.0h, +9.0h)
|
----
|
----
|
2022-01-15T07:00Z |
40.65
|
----
|
EAM (Effective Acceleration Model)
|
Evangelos Paouris (UoA) |
Detail
|
| 2022-01-17T17:00Z
(-12.0h, +12.0h)
|
----
|
50.0
|
2022-01-15T12:52Z |
52.13
|
Max Kp Range: 3.0 - 7.0
|
Other (SIDC)
|
Carina Alden (M2M Office) |
Detail
|
| 2022-01-16T12:03Z
(-7.5h, +11.0h)
|
----
|
62.0
|
2022-01-15T16:05Z |
19.97
|
Max Kp Range: 3.0 - 5.0
|
Ensemble WSA-ENLIL + Cone (NASA M2M)
|
Mary Aronne (M2M) |
Detail
|
| 2022-01-16T20:00Z
|
----
|
60.0
|
2022-01-16T08:44Z |
11.27
|
Max Kp Range: 3.0 - 5.0
|
Cone+HAF (SEPC, NSSC, CAS)
|
Jingjing Wang (NSSC SEPC) |
Detail
|
| 2022-01-16T18:42Z
|
----
|
57.3333
|
--- |
--- |
Max Kp Range: 3.6 - 5.6
|
Average of all Methods
|
Auto Generated (CCMC) |
Detail
|
|
|
CME Scoreboard