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Prediction for CME (2018-02-12T01:25:00-CME-001)CME Observed Time: 2018-02-12T01:25ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/13660/-1 CME Note: This partial halo CME is associated with a long duration C1.5 flare peaking at 1:35Z from AR2699. CME Shock Arrival Time: 2018-02-15T07:38Z Observed Geomagnetic Storm Parameters due to CME: ---- Predicted Arrival Time: 2018-02-14T09:00Z Predicted geomagnetic storm max Kp range due to CME: 5.0 - 5.0 Prediction Method: WSA-ENLIL + Cone (NOAA/SWPC) Prediction Method Note: Product: Forecast Discussion Issued: 2018 Feb 13 0030 UTC Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center Solar Activity .24 hr Summary... Solar activity was at low levels during the period due to a long duration C1 flare at 12/0135 UTC from Region 2699 (S07W29, Dai/beta). Associated with the flare activity was an asymmetric halo CME first observed in SOHO/LASCO C2 imagery at 12/0125 UTC. WSA/ENLIL model analysis of the event indicated a glancing blow late on 14 Feb to early on 15 Feb. New flux emergence and consolidation was observed in the intermediate area of Region 2699 while the larger leading and trailing spots were stable. .Forecast... There is a chance for C-class flares with a slight chance for an isolated M-class flare on days one through three (13-15 Feb) due to the flare potential of Region 2699. Energetic Particle .24 hr Summary... The greater than 2 MeV electron flux was at normal levels and the greater than 10 MeV proton flux were at or near background levels. .Forecast... The greater than 2 MeV electron flux is expected to continue at normal levels for the next three days (13-15 Feb). There is a slight chance for a greater than 10 MeV proton event on day one (13 Feb) due to recent flare activity from Region 2699. The greater than 10 MeV proton flux is expected to be at background levels on days two and three (14-15 Feb). Solar Wind .24 hr Summary... Solar wind parameters were at nominal levels. Solar wind speed ranged from approximately 300-345 km/s. Total field ranged from 1-7 nT while the Bz component was between +5/-4 nT. Phi angle was oriented in a mostly positive (away) solar sector with brief rotations into a negative (towards) sector. .Forecast... Solar wind parameters are expected to be at nominal levels on day one and through the majority of day two (13-14 Feb). By late on day two to early on day three (15 Feb), parameters are expected to become enhanced with the arrival of the 12 Feb CME likely in combination with the arrival of a CIR in advance of a negative polarity CH HSS. Solar wind speed reaching 600 km/s is likely with the CH HSS based on STEREO A Mag & Plastic data. Geospace .24 hr Summary... The geomagnetic field was quiet. .Forecast... The geomagnetic field is expected to be mostly quiet on days one and through the majority of day two (13-14 Feb). A glancing blow from the 12 Feb CME combined with CIR effects is expected to arrive late on day two through early on day three (14-15 Feb). Active levels are expected late on 14 Feb with unsettled to G1 (Minor) storm levels likely on 15 Feb. -- Product: 3-Day Forecast Issued: 2018 Feb 13 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 2 (below NOAA Scale levels). The greatest expected 3 hr Kp for Feb 13-Feb 15 2018 is 5 (NOAA Scale G1). NOAA Kp index breakdown Feb 13-Feb 15 2018 Feb 13 Feb 14 Feb 15 00-03UT 2 1 3 03-06UT 1 2 4 06-09UT 1 1 5 (G1) 09-12UT 1 1 5 (G1) 12-15UT 1 1 4 15-18UT 1 1 3 18-21UT 2 2 3 21-00UT 2 4 4 Rationale: A glancing blow from the 12 Feb CME combined with CIR effects is expected to arrive late on day two through early on day three (14-15 Feb). G1 (Minor) storm levels are likely on 15 Feb as a result.Lead Time: 60.28 hour(s) Difference: 22.63 hour(s) Prediction submitted by Leila Mays (GSFC) on 2018-02-12T19:21Z |
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