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Prediction for CME (2018-08-20T21:24:00-CME-001)CME Observed Time: 2018-08-20T21:24ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/14113/-1 CME Note: The CME is associated with a filament eruption occurring around 2018-08-20T18:00Z at N40W05 in SDO 193. CME Shock Arrival Time: 2018-08-25T06:00Z Observed Geomagnetic Storm Parameters due to CME: Max Kp: 7.0 Dst min. in nT: -169 Dst min. time: 2018-08-26T07:00Z Predicted Arrival Time: 2018-08-24T14:00Z Predicted geomagnetic storm max Kp range due to CME: 4.0 - 4.0 Prediction Method: WSA-ENLIL + Cone (NOAA/SWPC) Prediction Method Note: Product: 3-Day Forecast Issued: 2018 Aug 24 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 Aug 24-Aug 26 2018 is 4 (below NOAA Scale levels). NOAA Kp index breakdown Aug 24-Aug 26 2018 Aug 24 Aug 25 Aug 26 00-03UT 2 4 3 03-06UT 2 4 2 06-09UT 2 3 2 09-12UT 1 2 2 12-15UT 1 3 2 15-18UT 1 2 2 18-21UT 2 1 2 21-00UT 4 2 2 Rationale: No G1 (Minor) or greater geomagnetic storms are expected. Active levels are expected late on day one through early on day two (24-25 Aug) due to the anticipated arrival of the 20 Aug CME with possible combined effects from a weak CH HSS. Product: Forecast Discussion Issued: 2018 Aug 22 0030 UTC Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center Solar Activity .24 hr Summary... Solar activity was very low. Region 2719 (S12E09) decayed into a plage region and was inactive. At approximately 20/22 UTC a faint and slow-moving CME was seen in LASCO coronagraph imagery. The source region for this CME is unclear, and the bulk of the ejecta appears to be directed southwest of the Sun-Earth line. Further analysis of this event determined that a glancing blow from the CME is possible. However, due to it's lack of density and slow nature, impact is expected to be negligible. .Forecast... Solar activity is expected to be very low for the next three days (22-24 Aug). Energetic Particle .24 hr Summary... The greater than 2 MeV electron flux reached high levels this period with a peak flux of 9,290 pfu observed at 21/2025 UTC. The greater than 10 MeV proton flux was steady at background levels. .Forecast... The greater than 2 MeV electron flux is expected to reach high levels for the next three days (22-24 Aug) due to enhanced solar wind conditions. The greater than 10 MeV proton flux is expected to continue at background levels throughout the forecast period. Solar Wind .24 hr Summary... Solar wind parameters reflected a negative polarity CH HSS. Solar wind speeds steadily declined from around 600 km/s to around 450 km/s. Total field strength was steady near 5 nT. There were no significant deviations in the Bz component. The phi angle remained negative. .Forecast... Solar wind parameters are expected to remain enhanced for the next three days (22-24 Aug) due to the continued, but waning, influence of a negative polarity CH HSS. Geospace .24 hr Summary... The geomagnetic field was at quiet to unsettled levels due to the continued influence of the negative polarity CH HSS. .Forecast... Mostly unsettled levels are expected over the next three days (22-24 Aug) due to the continued influence of a negative polarity CH HSS. 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: 78.58 hour(s) Difference: 16.00 hour(s) Prediction submitted by Leila Mays (GSFC) on 2018-08-21T23:25Z |
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