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Prediction for CME (2013-10-22T04:36:00-CME-001)CME Observed Time: 2013-10-22T04:36ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/3423/-1 CME was not detected at Earth. Observed Geomagnetic Storm Parameters due to CME: ---- Predicted Arrival Time: 2013-10-24T18:00Z Predicted geomagnetic storm max Kp range due to CME: 5.0 - 5.0 Prediction Method: Other (SIDC) Prediction Method Note: :Issued: 2013 Oct 23 1329 UTC :Product: documentation at http://www.sidc.be/products/meu #--------------------------------------------------------------------# # DAILY BULLETIN ON SOLAR AND GEOMAGNETIC ACTIVITY from the SIDC # # (RWC Belgium) # #--------------------------------------------------------------------# SIDC URSIGRAM 31023 SIDC SOLAR BULLETIN 23 Oct 2013, 1310UT SIDC FORECAST (valid from 1230UT, 23 Oct 2013 until 25 Oct 2013) SOLAR FLARES : Active (M-class flares expected, probability >=50%) GEOMAGNETISM : Quiet (A<20 and K<4) SOLAR PROTONS : Quiet PREDICTIONS FOR 23 Oct 2013 10CM FLUX: 146 / AP: 008 PREDICTIONS FOR 24 Oct 2013 10CM FLUX: 146 / AP: 013 PREDICTIONS FOR 25 Oct 2013 10CM FLUX: 141 / AP: 013 COMMENT: There were two M flares and seven C flares on the Sun during the past 24 hours. The brightest one was an M4.2 flare released by beta-gamma-delta region NOAA AR 11875 with peak time at 21:20 UT on October 22, and caused a Type II radio burst with estimated shock speed of 1955 km/s. All flares except a low C flare (from NOAA AR 11877) were produced by AR 11875. More M flares are likely from AR 11875 within the next 48 hours, with a slight chance for an X flare. In the past 24 hours, solar wind speed further increased from about 300 km/s to a maximum of about 400 km/s around 19h UT on October 22. It has since fluctuated between 340 and 400 km/s. In the same period, the Interplanetary Magnetic Field has varied between 4 and 9 nT, with current values around 5 nT. These variations are consistent with the influence of a weak coronal hole high speed stream. Solar wind speed is expected to return to nominal values on October 24. LASCO C2 observed a CME associated with a filament eruption at 4:36 UT on October 22, which has a slight chance of producing a glancing blow in the second half of October 24. Geomagnetic activity was at quiet levels (K Dourbes between 0 and 3; NOAA Kp between 1 and 2) during the past 24 hours. Quiet conditions (K DourbesLead Time: 28.52 hour(s) Difference: ----- Prediction submitted by Leila Mays (GSFC) on 2013-10-23T13:29Z |
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