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Prediction for CME (2024-07-28T02:24:00-CME-001)CME Observed Time: 2024-07-28T02:24ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/32269/-1 CME Note: Full halo CME visible in SOHO LASCO C2/C3 and towards the east in STEREO A COR2. The source is likely the M9.9 flare peaking at 2024-07-28T01:57Z from AR 3766 and/or the M7.8 flare directly preceding it from the same region. Dimming and EUV wave visible in SDO AIA 193 and 335 and GOES SUVI 284, post-eruptive arcades visible in SDO AIA 131/171/193. The eruption is also visible in STEREO A EUV imagery. Arrival signature is characterized by an increase in magnetic field components from 9nT to approx. 16nT, preceded by a smaller increase from 6nT to 9nT starting at 2024-07-31T10:40Z and accompanied by a sharp increase in solar wind speed from approx. 400 km/s to over 470 km/s, as well as sharp increase in solar wind density to over 10p/cc. This is possibly a combined arrival of this CME and multiple other Earth-directed CMEs. CME Shock Arrival Time: 2024-07-31T13:46Z Observed Geomagnetic Storm Parameters due to CME: ---- Predicted Arrival Time: 2024-07-31T20:00Z (-12.0h, +12.0h) Confidence that the CME will arrive: 70.0% Predicted geomagnetic storm max Kp range due to CME: 4.0 - 7.0 Prediction Method: Other (SIDC) Prediction Method Note: #--------------------------------------------------------------------# # DAILY BULLETIN ON SOLAR AND GEOMAGNETIC ACTIVITY from the SIDC # # (RWC Belgium) # #--------------------------------------------------------------------# SIDC URSIGRAM 40728 SIDC SOLAR BULLETIN 28 Jul 2024, 1245UT SIDC FORECAST SOLAR FLARES : M-class flares expected (probability >=50%) GEOMAGNETISM : Quiet (A<20 and K<4) SOLAR PROTONS : Quiet PREDICTIONS FOR 28 Jul 2024 10CM FLUX: 205 / AP: 008 PREDICTIONS FOR 29 Jul 2024 10CM FLUX: 206 / AP: 008 PREDICTIONS FOR 30 Jul 2024 10CM FLUX: 205 / AP: 009 Solar Active Regions and flaring: The solar flaring activity was at high level during the last 24 hours, with few C-class flares and seven M-class flares. The strongest flare was GOES M9.9 flare from NOAA active region (AR) 3766 which peaked at 01:57 UTC on Jul 28. During the flare, the source region (AR 3766) of the flare had beta configuration of its photospheric magnetic field. NOAA AR 3766 produced three M-class flares and NOAA AR 3762, which is the most complex region on the disk (beta-gamma-delta magnetic field configuration), produced four M-class flares. The solar flaring activity is expected to be at moderate to high levels over the next 24 hours, possibly with few M-class flares and a chance for isolated X-class flares from NOAA AR 3766 or NOAA AR 3762. Coronal mass ejections: ...Another halo CME was first observed in the C2 images around 02:24 UTC on Jul 28. It was associated to the two subsequent M-class flares from the NOAA AR 3766 (S07 E10) and the EUV wave. The first M7.8 flare peaked at 01:51 UTC and the second M9.9 flare peaked at 01:57 UTC on Jul 28. Associated type II radio emissions were detected at 01:51 UTC on Jul 28, during the flaring activities. With a projected speed of about 470 km/s and its source region located closer to the central meridian, it is expected to impact the Earth later on the evening of July 31. ------- #--------------------------------------------------------------------# # FAST WARNING 'PRESTO' MESSAGE from the SIDC (RWC-Belgium) # #--------------------------------------------------------------------# A halo coronal mass ejection (CME) was first observed in the SOHO/LASCO-C2 images around 02:24 UTC on Jul 28. This CME was associated to two subsequent M-class flares from the NOAA AR 3766 (S07 E10) and the EUV wave. The first M7.8 flare peaked at 01:51 UTC and the second M9.9 flare peaked at 01:57 UTC on Jul 28. Associated type II radio emissions were detected at 01:51 UTC on Jul 28, during the flaring activities. With a projected speed of about 470 km/s and its source region located closer to the central meridian, it is expected to impact the Earth later on the evening of July 31. #--------------------------------------------------------------------# # Solar Influences Data analysis Center - RWC Belgium # # Royal Observatory of Belgium # # #Lead Time: 51.20 hour(s) Difference: -6.23 hour(s) Prediction submitted by Tony Iampietro (M2M) on 2024-07-29T10:34Z |
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