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Prediction for CME (2023-08-23T02:17:00-CME-001)CME Observed Time: 2023-08-23T02:17ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/26602/-1 CME Note: Filament eruption CME with asymmetric front seen to the southwest comprised of a brighter bulk along the right leading edge and fainter loop with cavity on the left leading edge. Notable deflection westward as seen in SDO 304 imagery. CME was not detected at Earth. Observed Geomagnetic Storm Parameters due to CME: ---- Predicted Arrival Time: 2023-08-27T12:00Z (-7.0h, +7.0h) Predicted geomagnetic storm max Kp range due to CME: 2.0 - 4.0 Prediction Method: WSA-ENLIL + Cone (NOAA/SWPC) Prediction Method Note: Please enter the following information for your prediction: SWPC ENLIL settings: ENLIL version: 2.9e Resolution: medium Ambient settings: a8b1 Ejecta settings: d4t1x1 WSA version: 2.2 GONG: mrbqs CME input parameters Time at 21.5Rs boundary: Radial velocity (km/s): 729 Longitude (deg): W37 Latitude (deg): S22 Half-angular width (deg): 16 Product: Forecast Discussion Issued: 2023 Aug 24 0030 UTC Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center Solar Activity .24 hr Summary... Solar activity was low, with only low level C-class flares observed this period. Region 3405 (N10W48, Hsx/alpha) was the main flare producer, including the largest flare of the period; a C3.9/Sf flare at 23/1407 UTC. This region continued to decay throughout the period and became less active by the end of the day. Region 3413 (N10E46, Fho/beta) was the only spot group that exhibited any sort of growth, though it was still too foreshortened to get an accurate magnetic analysis. It did, however, produce a C1.7 flare at 23/1516 UTC and a C2.5 flare at 23/1616 UTC. There is also a chance that this could actually be two spot groups, but that determination will be made when it rotates farther onto the visible disk and a more accurate analysis can be made. The remaining numbered sunspot regions were either in decay or stable. The filament eruption observed off the SW sector of the limb, first visible in coronagraph imagery near 23/0259 UTC, was analyzed and indicates a possible weak impact at Earth around midday on 27 Aug. .Forecast... Solar activity is expected to remain low, with a slight chance for M-class flares, for the next three days (24-26 Aug) . Energetic Particles .24 hr Summary... The greater than 2 MeV electron flux reached moderate levels. The greater than 10 MeV proton flux was at background levels. .Forecast... The greater than 2 MeV electron flux is expected to be at normal to moderate levels on 24 Aug, eventually reaching high levels by 25-26 Aug. The greater than 10 MeV proton flux is expected to remain at background readings through 26 Aug. Solar Wind .24 hr Summary... The solar wind environment reflected a mostly background regime. Total field strength averaged near 5 nT, Bz was generally north to near-neutral with no significant deviations, and wind speeds decreased from over 460 km/s to around 425 km/s. The phi angle was mostly negative. .Forecast... The solar wind environment is expected to isolated, weak enhancements through 26 Aug with persistent, yet intermittent, CH HSS influences. Geospace .24 hr Summary... The geomagnetic field was at quiet levels. .Forecast... Mostly quiet to unsettled levels are expected through 26 Aug with intermittent, weak HSS influence.Lead Time: 92.00 hour(s) Difference: ----- Prediction submitted by Chris Stubenrauch (M2M Office) on 2023-08-23T16:00Z |
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