Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2014-01-07T18:24Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C3
STEREO B: SECCHI/COR2
Activity ID: 2014-01-07T18:24:00-CME-001 (version 3)
Source Location: S30W20
Active Region Number: 11943
Note Keyword:
Source Signature Keyword:
Morphology Keyword:
Note: From active regions 1943/1944. Dimming region (S30W20) and CME longitude far from flare source location (11943 S12W08). See Moestl et al. (2015) doi:10.1038/ncomms8135 and Mays et al. (in prep).
Submitted on 2015-06-01T22:02Z by Leila
Mays
A Notification with ID
20140107-AL-003 was sent on 2014-01-07T20:01Z
A Notification with ID
20140107-AL-005 was sent on 2014-01-07T20:53Z
A Notification with ID
20140108-AL-001 was sent on 2014-01-08T00:22Z
A Notification with ID
20140108-AL-003 was sent on 2014-01-08T04:11Z
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The List of CME Analysis already entered: |
Event Type |
Catalog |
Measurement TypeCME measurement type: Leading Edge (LE), Shock Front (SH), Right Hand Boundary (RHB), Left Hand Boundary (LHB), Black/White Boundary (BW), Prominence Core (COR), Disconnection Front (DIS), Trailing Edge (TE). |
Prime?"primary flag" which is either True or False. If there are multiple CME analysis entries for a single CME, this flag would indicate which analysis is considered most accurate per measurement type. This is a helpful flag if you would like to download only one most accurate CME analysis per CME per Measurement Type |
Technique |
Long |
Lat |
Speed |
Type |
Half Width |
Time 21.5 |
Note |
WSA-ENLIL+Cone Result(s) |
Submitted By |
CME Analysis
|
M2M_CATALOG |
|
true |
|
30.0 |
-24.0 |
2061.0 |
R |
49.0 |
2014-01-07T19:48Z |
remeasured. GCS major half width=49, minor half width=21, tilt=-141. See Moestl et al. (2015) doi:10.1038/ncomms8135 and Mays et al. (2015) doi:10.1088/0004-637X/812/2/145 for more measurements. |
Not modeled
|
Leila Mays on 2016-03-02T02:47Z |
CME Analysis
|
M2M_CATALOG |
|
false |
|
10.0 |
-28.0 |
2750.0 |
R |
60.0 |
2014-01-07T19:33Z |
Very preliminary, based only on STEREO-A COR2 and deprojection estimate from Hundhausen. |
Not modeled
|
Barbara Thompson on 2014-01-07T19:57Z |
CME Analysis
|
M2M_CATALOG |
|
false |
|
10.0 |
-25.0 |
2750.0 |
R |
68.0 |
2014-01-07T19:33Z |
|
1: Result 1 (2.0 AU)
Earth = 2014-01-08T19:00Z
(PE: -24.5 h)
Mars = 2014-01-09T17:08Z
|
Barbara Thompson on 2014-01-07T20:53Z |
CME Analysis
|
M2M_CATALOG |
|
false |
|
40.0 |
-30.0 |
2400.0 |
R |
68.0 |
2014-01-07T19:50Z |
using data from SOHO, STEREO A and B (however triangulation was still not possible) |
1: Result 1 (2.0 AU)
Earth = 2014-01-09T00:38Z
(PE: -18.9 h)
Mars = 2014-01-09T17:55Z
|
Leila Mays on 2014-01-08T00:19Z |
CME Analysis
|
M2M_CATALOG |
|
false |
|
28.0 |
-26.0 |
1950.0 |
O |
48.0 |
2014-01-07T19:48Z |
Updated parameters from a GCS fit. Tilt = 38 deg ellipse aspect ratio = 1.59 . major half width = 50 minor half width = 32. |
Not modeled
|
Leila Mays on 2015-04-24T15:08Z |
CME Analysis
|
SWPC_ANNEX_CME_CATALOG |
|
false |
SWPC_CAT |
21.0 |
-21.0 |
2048.0 |
R |
50.0 |
2014-01-07T20:01Z |
SWPC info:
CME Start = 2014-01-07T01:32Z
Shock at ACE = 2014-01-09T19:31Z
WSA/ENLIL prediction = 204-01-09T08:00Z
CME ID = 389
Reference Time = 2014-01-08T00:00Z |
Not modeled
|
chiu wiegand on 2017-11-15T19:01Z |
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All directly linked activities: |
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Comments by users: |
"http://iswax.ccmc.gsfc.nasa.gov/ENSEMBLE/2014-01-07_ncmes1_sims48_LIHUE046/Detailed_results_20140107_182400_ncmes1_sims48_LIHUE046.txt" --Commented by Leila
Mays on 2014-01-09T18:03:27 (version
2)
|
"2014-01-07 CME
http://go.nasa.gov/1bSpRwd
ensemble results
http://go.nasa.gov/1bSoEVQ
scoreboard predictions
http://kauai.ccmc.gsfc.nasa.gov/SWScoreBoard/
nice running difference movie
http://www.lmsal.com/nitta/nrt/nrt_aia_0193_rdiff_512_640_20140107_18.mov" --Commented by Leila
Mays on 2014-01-08T21:43:17 (version
1)
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"tag-up comments: CH in NE and CH near equator could have helped deflect CME to larger longitudes. X1.2 flare looks like a classic two ribbon flare, no saturation in AIA." --Commented by Leila
Mays on 2014-01-08T16:46:16 (version
1)
|
"CME is a slightly asymmetric halo in STB. Asymmetric halo in LASCO.
Barbara: X1.2 flare, CME and SEP event from AR1943/1944 complex, starting at 18:02UT. Strong dimmings observed in SDO/AIA, X1.2 flare starting at 18:02UT, peaking at 18:31UT from near AR1943 but connections to AR1944." --Commented by Leila
Mays on 2014-01-08T00:21:56 (version
1)
|
"Kevin Schenk measurements: http://umbra.nascom.nasa.gov/lasco/observations/halo/2014/140107/" --Commented by Leila
Mays on 2014-01-08T00:20:16 (version
1)
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