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Prediction for CME (2020-12-07T16:24:00-CME-001)CME Observed Time: 2020-12-07T16:24ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/16214/-1 CME Note: This CME is associated with a C7.4 flare from AR 2790 (S23W11) that peaked at 2020-12-07T16:32Z. The eruption signature of this event can be seen in SDO AIA 193/304 starting as early 2020-12-07T15:30Z. The chosen start time for this CME event is the initial time it was observed in STEREO A COR2 imagery since SOHO LASCO data was unaavailable during real-time analysis. ARRIVAL SIGNATURE: Beginning at 2020-12-10T01:29Z, DSCOVR detects magnetic field strength increases to 10 nT, solar wind speed jumps from 450 to 600 km/s, density jumps to over 20/cc, and temperatures jump to over 300,000 K. Similar signatures are seen by ACE at the same time. CME Shock Arrival Time: 2020-12-10T01:29Z Observed Geomagnetic Storm Parameters due to CME: ---- Predicted Arrival Time: 2020-12-09T19:00Z Predicted geomagnetic storm max Kp range due to CME: 5.0 - 7.0 Prediction Method: WSA-ENLIL + Cone (NOAA/SWPC) Prediction Method Note: Product: Forecast Discussion Issued: 2020 Dec 08 1230 UTC Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center Solar Activity .24 hr Summary... Solar activity reached low levels. Region 2791 (S15, L=221) was inactive and decayed to plage. Region 2790 (S22W23, Hsx/alpha) produced a long duration C7 flare which resulted in a full halo CME as observed in coronagraph imagery. A consensus of model runs suggest speeds between 830-880 km/s, and arrival in the latter half of 09 Dec. .Forecast... Solar activity is expected to be at mostly low levels with a slight chance for C-class flares 08-10 Dec. Energetic Particle .24 hr Summary... The greater than 2 MeV electron flux was normal to moderate and the greater than 10 MeV proton flux remained at background values. .Forecast... The greater than 2 MeV electron flux is expected to be normal to moderate 08-10 Dec, while the greater than 10 MeV proton flux is expected to continue at background. Solar Wind .24 hr Summary... Solar wind parameters, as measured by the ACE satellite, reflected ambient conditions. Total IMF strength ranged primarily from 2 to 5 nT and the Bz component underwent mainly weak deviations. Solar wind speed averaged 350-400 km/s. The phi angle was predominantly positive with brief excursions into a negative solar sector. .Forecast... The solar wind is anticipated to continue as primarily a slow regime on 08 Dec. Elevated conditions are likely 09-10 Dec with the combined influence of a weak, negative polarity CH and arrival of a CME from the 07 Dec event. Geospace .24 hr Summary... The geomagnetic field was quiet. .Forecast... The geomagnetic field is expected to be primarily quiet 08 Dec. G1 (Minor) storm conditions are likely 09-10 Dec due to the combined effects of a weak, negative polarity CH and the arrival of a CME from the 07 Dec event. Actual time was taken from simulation at: https://www.swpc.noaa.gov/products/wsa-enlil-solar-wind-prediction Space Weather Message Code: WATA50 Serial Number: 64 Issue Time: 2020 Dec 08 1506 UTC WATCH: Geomagnetic Storm Category G3 Predicted Highest Storm Level Predicted by Day: Dec 09: G1 (Minor) Dec 10: G3 (Strong) Dec 11: G2 (Moderate) THIS SUPERSEDES ANY/ALL PRIOR WATCHES IN EFFECT NOAA Space Weather Scale descriptions can be found at www.swpc.noaa.gov/noaa-scales-explanation Potential Impacts: Area of impact primarily poleward of 50 degrees Geomagnetic Latitude. Induced Currents - Power system voltage irregularities possible, false alarms may be triggered on some protection devices. Spacecraft - Systems may experience surface charging; increased drag on low Earth-orbit satellites and orientation problems may occur. Navigation - Intermittent satellite navigation (GPS) problems, including loss-of-lock and increased range error may occur. Radio - HF (high frequency) radio may be intermittent. Aurora - Aurora may be seen as low as Pennsylvania to Iowa to Oregon.Lead Time: 36.98 hour(s) Difference: 6.48 hour(s) Prediction submitted by Yaireska Collado (M2M Office) on 2020-12-08T12:30Z |
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