CME Scoreboard |
|
Prediction for CME (2014-09-02T16:00:00-CME-001)CME Observed Time: 2014-09-02T16:00ZCME Shock Arrival Time: 2014-09-06T04:33Z Observed Geomagnetic Storm Parameters due to CME: Max Kp: 3.0 Dst min. in nT: -26 Dst min. time: 2014-09-07T03:00Z Predicted Arrival Time: 2014-09-06T12:00Z Predicted geomagnetic storm max Kp range due to CME: 4.0 - 4.0 Prediction Method: WSA-ENLIL + Cone (NOAA/SWPC) Prediction Method Note: (Arrival Prediction by NOAA/SWPC submitted to this system by M. Leila Mays) (Submitted CME shock arrival time taken from the excerpted Forecast Discussion below). (Submitted Kp estimate is from the excerpted Forecast Discussion and 3-Day Forecast below). -- Product: Forecast Discussion Issued: 2014 Sep 03 1230 UTC Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center Solar Activity .24 hr Summary... Solar activity remained at low levels. The largest flare of the period, a C4 flare at 03/0253 UTC, appeared to originate from a region just beyond the southeastern limb. Region 2152 (S15W19, Eac/beta-gamma) also produced a few low level C-class flares during the period. This region continued to grow, primarily in its intermediate spot area, and show signs of separation between the leader and trailer spots. Region 2153 (S10W45, Dao/beta) exhibited signs of decay during the period. Region 2154 (S19E29, Cao/beta) continued to show signs of growth, though that growth rate slowed near the end of the period. SDO AIA/304 imagery captured a 44 degree long filament, centered near N32W14, erupting between 02/1300-1600 UTC. The eruption was also evident in ground-based H-alpha imagery from the GONG facilities. Initial analysis indicated there is an Earth-directed component of the coronal mass ejection (CME), set to arrive early to midday on 6 Sep, just outside this forecast period. Further analysis will be conducted on this CME and adjustments to the forecast will be made accordingly. .Forecast... Solar activity is expected to be low with an increasing chance for M-class (R1-R2 (Minor-Moderate)) flare activity over the next three days (03-05 Sep). Regions in the north and south, just beyond the east limb, have been very active as they approach the visible disk. These regions, as well as Region 2152, will be monitored closely as they represent the greatest threat for the next few days. Energetic Particle .24 hr Summary... The greater than 2 MeV electron flux was at normal to high levels, reaching a peak flux value of 6110 pfu at 02/1620 UTC. The greater than 10 MeV and 100 MeV proton flux values were elevated in response to yesterday's back-side event, but remained below alert thresholds. Protons greater than 10 MeV at geosynchronous orbit reached a peak level of 3 pfu at 03/0845Z, while 100 MeV protons reached a max of .7 pfu at 02/2210 UTC. .Forecast... The greater than 2 MeV electron flux is expected to be at normal to high levels for the next three days (03-05 Sep). The greater than 10 MeV proton flux is expected to remain enhanced, but below alert threshold levels (S1-Minor) for the next three days (03-05 Sep) in the absence of another significant flare. Solar Wind .24 hr Summary... The solar wind environment at the ACE spacecraft remained fairly consistent throughout the period. Wind speed averaged near 420 km/s range, Phi remained positive, and Bt held steady near 6 nT. Bz ranged between +/-5 nT, but was predominantly negative during the period. .Forecast... Solar wind parameters are expected to remain enhanced over the next three days (03-05 Sep). Solar wind speeds are likely to see steadily decreasing values as the high speed stream influence continues to wane. Geospace .24 hr Summary... The geomagnetic field was at quiet to unsettled levels, with isolated minor storm levels observed at high latitudes. .Forecast... The geomagnetic field is expected to be at quiet to active levels (Below G1-Minor) through midday on day one (03 Sep). Quiet to unsettled conditions are expected, with a chance for Active levels for days two and three (04-05 Sep), as high speed solar wind stream influences persist. Product: 3-Day Forecast Issued: 2014 Sep 05 0030 UTC Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center A. NOAA Geomagnetic Activity Observation and Forecast The greatest observed 3 hr Kp over the past 24 hours was 3 (below NOAA Scale levels). The greatest expected 3 hr Kp for Sep 05-Sep 07 2014 is 4 (below NOAA Scale levels). NOAA Kp index breakdown Sep 05-Sep 07 2014 Sep 05 Sep 06 Sep 07 00-03UT 3 3 4 03-06UT 2 3 3 06-09UT 2 3 3 09-12UT 2 3 2 12-15UT 3 3 2 15-18UT 3 3 3 18-21UT 3 4 3 21-00UT 3 4 3 Rationale: No G1 (Minor) or greater geomagnetic storms are expected. No significant transient or recurrent solar wind features are forecast. B. NOAA Solar Radiation Activity Observation and Forecast Solar radiation, as observed by NOAA GOES-13 over the past 24 hours, was below S-scale storm level thresholds. Solar Radiation Storm Forecast for Sep 05-Sep 07 2014 Sep 05 Sep 06 Sep 07 S1 or greater 5% 5% 5% Rationale: No S1 (Minor) or greater solar radiation storms are expected. No significant active region activity favorable for radiation storm production is forecast. C. NOAA Radio Blackout Activity and Forecast No radio blackouts were observed over the past 24 hours. Radio Blackout Forecast for Sep 05-Sep 07 2014 Sep 05 Sep 06 Sep 07 R1-R2 55% 55% 55% R3 or greater 10% 10% 10% Rationale: R1-R2 (Minor-Moderate) radio blackouts are likely with a slight chance for R3 (Major) for the next three days due to potential flare activity from Regions 2152 (S15W38), 2157 (S13E68) and 2158 (N16E83). Thank you for using the Product Subscription Service. If you would like to remove a product subscription or update the personal information in your account, go to the Product Subscription Site. Please do not use the from address for correspondence, as it is not monitored. For comments or help, please contact SWPC Help.Lead Time: 64.05 hour(s) Difference: -7.45 hour(s) Prediction submitted by Leila Mays (GSFC) on 2014-09-03T12:30Z |
|
CCMC
Rules of the Road: CCMC requests that users notify the CCMC, CME
model/technique developers and submitting forecasters/researchers before
performing event and validation studies with data from the CME Arrival
Time Scoreboard. It is recommended that such studies be performed with
the knowledge and collaboration of developers and submitting
forecasters/researchers. Curator: Chiu Wiegand | NASA Official: Dr. Masha Kuznetsova | Privacy and Security Notices | Accessibility | CCMC Data Policy |