CME Scoreboard |
|
Prediction for CME (2014-08-01T18:36:00-CME-001)CME Observed Time: 2014-08-01T18:36ZCME was not detected at Earth. Observed Geomagnetic Storm Parameters due to CME: ---- Predicted Arrival Time: 2014-08-04T15:00Z Prediction Method: Other (SIDC) Prediction Method Note: :Issued: 2014 Aug 02 1235 UTC :Product: documentation at http://www.sidc.be/products/meu #--------------------------------------------------------------------# # DAILY BULLETIN ON SOLAR AND GEOMAGNETIC ACTIVITY from the SIDC # # (RWC Belgium) # #--------------------------------------------------------------------# SIDC URSIGRAM 40802 SIDC SOLAR BULLETIN 02 Aug 2014, 1208UT SIDC FORECAST (valid from 1230UT, 02 Aug 2014 until 04 Aug 2014) SOLAR FLARES : Eruptive (C-class flares expected, probability >=50%) GEOMAGNETISM : Quiet (A<20 and K<4) SOLAR PROTONS : Quiet PREDICTIONS FOR 02 Aug 2014 10CM FLUX: 176 / AP: 011 PREDICTIONS FOR 03 Aug 2014 10CM FLUX: 182 / AP: 007 PREDICTIONS FOR 04 Aug 2014 10CM FLUX: 186 / AP: 010 COMMENT: There are currently 9 sunspot regions on the solar disk. NOAA 2130 produced an M2 flare peaking at 14:48UT, and NOAA 2127 was the source of an M1.5 flare peaking at 18:13UT. The CME associated to this flaring activity was first observed by SOHO/LASCO at 18:36UT. This CME had a true speed of about 800 km/s, but the bulk was directed to the SE. Nonetheless, difference imagery detected the outline of a faint halo to the WSW, and was a near full halo as seen from the STEREO-A vantage point. Hence, a glancing blow of this CME can not be excluded and could impact Earth in the afternoon of 4 August. NOAA 2127, 2130 and 2132 still have areas with some mixed magnetic polarity. The CME associated to the 1 August (10:15UT) filament eruption, which took place in the same location as the 30 July filament eruption, was directed mainly to the north. It does not seem to have an Earth-directed component despite its proximity to the disk's center. Two 25-degrees long filaments in the NE and SW quadrant remained stable. C-class flaring is expected, with a chance for an M-class flare. Solar wind speed increased from about 350 km/s to values between 400-450 km/s. Bz oscillated between -10 and +10 nT. Local geomagnetic conditions were quiet to unsettled, with Kp briefly reaching active levels just before midnight. No obvious signature from the CME associated to the 30 July filament eruption has been observed so far in the solar wind parameters. Geomagnetic conditions are expected to be quiet to unsettled, with locally a chance on active conditions as the solar wind may still be modulated by the 30 July CME (2 August) and the influence of a coronal hole stream (4 August). TODAY'S ESTIMATED ISN : 123, BASED ON 12 STATIONS. SOLAR INDICES FOR 01 Aug 2014 WOLF NUMBER CATANIA : /// 10CM SOLAR FLUX : 168 AK CHAMBON LA FORET : 021 AK WINGST : 012 ESTIMATED AP : 013 ESTIMATED ISN : 119, BASED ON 20 STATIONS. NOTICEABLE EVENTS SUMMARY DAY BEGIN MAX END LOC XRAY OP 10CM Catania/NOAA RADIO_BURST_TYPES 01 1443 1448 1457 ////// M2.0 340 35/2130 III/1 01 1755 1813 1848 ////// M1.5 97 32/2127 III/2CTM/1II/2IV/1 END BT #--------------------------------------------------------------------# # Solar Influences Data analysis Center - RWC Belgium # # Royal Observatory of Belgium # # Fax : 32 (0) 2 373 0 224 # # Tel.: 32 (0) 2 373 0 491 # # # # For more information, see http://www.sidc.be. Please do not reply # # directly to this message, but send comments and suggestions to # # 'sidctech@oma.be'. If you are unable to use that address, use # # 'rvdlinden@spd.aas.org' instead. # # To unsubscribe, visit http://sidc.be/registration/unsub.php # #--------------------------------------------------------------------#Lead Time: 50.42 hour(s) Difference: ----- Prediction submitted by Leila Mays (GSFC) on 2014-08-02T12:35Z |
|
CCMC
Rules of the Road: CCMC requests that users notify the CCMC, CME
model/technique developers and submitting forecasters/researchers before
performing event and validation studies with data from the CME Arrival
Time Scoreboard. It is recommended that such studies be performed with
the knowledge and collaboration of developers and submitting
forecasters/researchers. Curator: Chiu Wiegand | NASA Official: Dr. Masha Kuznetsova | Privacy and Security Notices | Accessibility | CCMC Data Policy |