CME Scoreboard |
|
Prediction for CME (2014-04-02T13:55:00-CME-001)CME Observed Time: 2014-04-02T13:55ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/5080/-1 CME Shock Arrival Time: 2014-04-05T09:40Z Observed Geomagnetic Storm Parameters due to CME: Max Kp: 4.0 Predicted Arrival Time: 2014-04-05T00:00Z (-9.0h) Predicted geomagnetic storm max Kp range due to CME: 5.0 - 5.0 Prediction Method: Other (SIDC) Prediction Method Note: :Issued: 2014 Apr 03 1223 UTC :Product: documentation at http://www.sidc.be/products/meu #--------------------------------------------------------------------# # DAILY BULLETIN ON SOLAR AND GEOMAGNETIC ACTIVITY from the SIDC # # (RWC Belgium) # #--------------------------------------------------------------------# SIDC URSIGRAM 40403 SIDC SOLAR BULLETIN 03 Apr 2014, 1204UT SIDC FORECAST (valid from 1230UT, 03 Apr 2014 until 05 Apr 2014) SOLAR FLARES : Eruptive (C-class flares expected, probability >=50%) GEOMAGNETISM : Quiet (A<20 and K<4) SOLAR PROTONS : Quiet PREDICTIONS FOR 03 Apr 2014 10CM FLUX: 154 / AP: 005 PREDICTIONS FOR 04 Apr 2014 10CM FLUX: 154 / AP: 007 PREDICTIONS FOR 05 Apr 2014 10CM FLUX: 154 / AP: 023 COMMENT: Solar activity was dominated by an M6.5 flare from NOAA AR 2027 peaking at 14:05 UT, April 2. It was associated with a filament eruption and type II radio bursts. The corresponding full halo CME was first visible in LASCO C2 at 13:36 UT. Measured projected speeds by CACTus vary between 500 km/s and over 1500 km/s. The bulk of the mass was expelled in north east direction. Given the location of the source region and the direction of the ejecta the impact on earth will probably be limited. We can expect at least the impact of the CME driven shock but also a weak impact of the CME itself is probable. Arrival is likely to be around midnight April 4 to 5. Solar wind speed decreased rather steadily from just above 400 km/s to now just above 360 km/s. The total magnetic field was stable in the 4 to 6 nT range. No signatures of the anticipated arrival of the CMEs of March 28, 29, and 30 have been observed. Geomagnetic conditions were at quiet levels (both local K and planetary Kp <=2) over the last 24 hours. Geomagnetic conditions are expected to remain quiet in the next 36 hours. Afterwards, the arrival of the April 1 and April 2 CMEs may cause unsettled to active conditions and possibly minor storms. Also the low latitude coronal hole that passed the central meridian late April 1, early April 2 may become geoeffective by midnight April 4 to 5. TODAY'S ESTIMATED ISN : 097, BASED ON 14 STATIONS. SOLAR INDICES FOR 02 Apr 2014 WOLF NUMBER CATANIA : 125 10CM SOLAR FLUX : 155 AK CHAMBON LA FORET : 010 AK WINGST : 005 ESTIMATED AP : 005 ESTIMATED ISN : 084, BASED ON 21 STATIONS. NOTICEABLE EVENTS SUMMARY DAY BEGIN MAX END LOC XRAY OP 10CM Catania/NOAA RADIO_BURST_TYPES 02 1318 1405 1428 N14E53 M6.5 2B 3700 09/2027 II/1IV/2 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 # #--------------------------------------------------------------------# :Issued: 2014 Apr 02 1801 UTC :Product: documentation at http://www.sidc.be/products/presto #--------------------------------------------------------------------# # FAST WARNING 'PRESTO' MESSAGE from the SIDC (RWC-Belgium) # #--------------------------------------------------------------------# The M6.5 flare peaking at 14:05 UT originated from NOAA AR 2017, and was associated with type II radio bursts observed by the Humain station. The corresponding CME appears as a full halo CME from the viewpoint of STEREO A spacecraft. It becomes visible in STEREO B COR2 at 13:55 UT, and in STEREO A COR2 at 13:54 UT. Unfortunately the STEREO B COR2 data suffer a data gap right after the onset. In the latest LASCO C2 data it appears at 13:36 UT and also appears to develop as a full halo CME from the Sun-Earth line viewpoint. Arrival of the CME can be expected as early as April 3 after 15:00 UT. #--------------------------------------------------------------------# # 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: 45.28 hour(s) Difference: 9.67 hour(s) Prediction submitted by Leila Mays (GSFC) on 2014-04-03T12:23Z |
|
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 |