|
|
Prediction for CME (2015-08-21T10:24:00-CME-001)CME Observed Time: 2015-08-21T10:24ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/9152/-1 CME Note: associated with M1.4 flare CME was not detected at Earth. Observed Geomagnetic Storm Parameters due to CME: ---- Predicted Arrival Time: 2015-08-26T07:10Z (-12.0h, +12.0h) Confidence that the CME will arrive: 20.0% Predicted geomagnetic storm max Kp range due to CME: 2.0 - 4.0 Prediction Method: Other (SIDC) Prediction Method Note: :Issued: 2015 Aug 22 1230 UTC :Product: documentation at http://www.sidc.be/products/meu #--------------------------------------------------------------------# # DAILY BULLETIN ON SOLAR AND GEOMAGNETIC ACTIVITY from the SIDC # # (RWC Belgium) # #--------------------------------------------------------------------# SIDC URSIGRAM 50822 SIDC SOLAR BULLETIN 22 Aug 2015, 1230UT SIDC FORECAST (valid from 1230UT, 22 Aug 2015 until 24 Aug 2015) SOLAR FLARES : M-class flares expected (probability >=50%) GEOMAGNETISM : Quiet (A<20 and K<4) SOLAR PROTONS : Quiet PREDICTIONS FOR 22 Aug 2015 10CM FLUX: 115 / AP: 008 PREDICTIONS FOR 23 Aug 2015 10CM FLUX: 118 / AP: 010 PREDICTIONS FOR 24 Aug 2015 10CM FLUX: 122 / AP: 008 COMMENT: Solar activity remained enhanced over the past 24 hours, with Active Region (AR) 2403 (Macintosh:Dkc/Type:Beta-Gamma) showing continued flux emergence, and producing several C-class flares and two M-class flares; an M1.1 class flare on 2015-Aug-21 peaking at 20:34 UT, and an M1.2 flare on 2015-Aug-22 peaking at 06:49 UT. An earlier M1.4 class flare produced by AR 2403, peaking at 09:48 UT, had an associated Coronal Mass Ejection (CME). Although there was evidence of a dimming on the Sun, the extent of the CME became apparent as LASCO observations became available. At the time the AR was located at S17E26, and the CME was largely directed to the south east, and is not expected to significantly interact with the Earth, the CME had a speed of 297 km/s, and if a small component was to reach the Earth it would be expected to arrive on 2015-Aug-26 at 07:00 UT. AR 2404 (Macintosh:Cro/Type:Beta) emerged yesterday and has shown some evidence of growth, but still remains small. No other evident Earth directed CMEs were produced in the past 24 hours. Solar activity is expected to remain active over the next 24 hours, with AR 2403 producing C-class flares with the possibility of M and X-class flares. The solar wind speed, as recorded by the ACE satellite, has been slowly decreasing over the past 24 hours, from roughly 460 km/s to 400 km/s. The total interplanetary magnetic field (IMF) strength, as recorded by the ACE satellite, has been around 5 nT, and the Bz component was largely fluctuating between -5 nT and +5 nT yesterday (2015-Aug-21) but has been largely negative over the past 10 hours, around -4 nT. Geomagnetic conditions varied between quiet and moderate over the past 24 hours, with the local (Dourbes) K-index reaching 3 and the NOAA K-index reaching 2. There is currently a small coronal hole located at S15W45 which may increase solar wind speeds. The low solar wind speed, combined with the low magnitude Southward Bz indicates that geomagnetic activity should be small with possible low level enhancements over the next 24 hours. TODAY'S ESTIMATED ISN : 069, BASED ON 21 STATIONS. SOLAR INDICES FOR 21 Aug 2015 WOLF NUMBER CATANIA : /// 10CM SOLAR FLUX : 110 AK CHAMBON LA FORET : 013 AK WINGST : 008 ESTIMATED AP : 007 ESTIMATED ISN : 077, BASED ON 29 STATIONS. NOTICEABLE EVENTS SUMMARY DAY BEGIN MAX END LOC XRAY OP 10CM Catania/NOAA RADIO_BURST_TYPES 21 0934 0948 1007 S17E26 M1.4 2B 73 ///2403 II/1 21 1910 2034 2050 S12E26 M1.1 1N ///2403 III/1 22 0639 0649 0659 S15E20 M1.2 1B 62 ///2403 II/2 END BTLead Time: 91.27 hour(s) Difference: ----- Prediction submitted by Leila Mays (GSFC) on 2015-08-22T11:54Z |
|
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 |