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Prediction for CME (2015-07-19T09:48:00-CME-001)CME Observed Time: 2015-07-19T09:48ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/8951/-1 CME Note: The arrival time for the CME is a little uncertain since it was possible embedded with a CIR preceding a CH HSS CME Shock Arrival Time: 2015-07-22T15:30Z Observed Geomagnetic Storm Parameters due to CME: ---- Predicted Arrival Time: 2015-07-22T15:00Z (-12.0h, +12.0h) Predicted geomagnetic storm max Kp range due to CME: 2.0 - 4.0 Prediction Method: Other (SIDC) Prediction Method Note: :Issued: 2015 Jul 20 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 50720 SIDC SOLAR BULLETIN 20 Jul 2015, 1230UT SIDC FORECAST (valid from 1230UT, 20 Jul 2015 until 22 Jul 2015) SOLAR FLARES : Quiet conditions (<50% probability of C-class flares) GEOMAGNETISM : Active conditions expected (A>=20 or K=4) SOLAR PROTONS : Quiet PREDICTIONS FOR 20 Jul 2015 10CM FLUX: 100 / AP: 011 PREDICTIONS FOR 21 Jul 2015 10CM FLUX: 099 / AP: 013 PREDICTIONS FOR 22 Jul 2015 10CM FLUX: 098 / AP: 011 COMMENT: The long-duration C2.1 flare related to the complex filament eruption in the southwest quadrant peaked on 19 July at 10:40UT and ended at 13:02UT. The bulk of the related coronal mass ejection (CME), first seen in LASCO/C2 imagery by CACTus on 09:48UT, is directed away from Earth. However, a glancing blow from this CME cannot be ruled out and may impact Earth on 22 or early 23 July. At most active geomagnetic conditions are expected. The two currently visible sunspot regions were quiet. No C-class flares or other earth-directed CMEs were observed. Quiet flaring conditions are expected, with a small chance on a C-class flare. Solar wind speed further declined from 300 km/s to 270 km/s around 03:00UT, then increased to its current values between 290-300 km/s. Bz was initially very low, but has been persistently negative from about 03:00UT till 11:00UT, with maximum values near -6 nT. Bz then quickly returned to very low values. The interplanetary magnetic field (IMF) was mostly directed away from the Sun. Quiet to unsettled geomagnetic conditions have been observed. Mostly quiet to unsettled geomagnetic conditions are expected, but with a chance on an active geomagnetic episode in response to the anticipated arrival of the high speed stream of the positive transequatorial coronal hole. TODAY'S ESTIMATED ISN : 044, BASED ON 16 STATIONS. SOLAR INDICES FOR 19 Jul 2015 WOLF NUMBER CATANIA : /// 10CM SOLAR FLUX : 099 AK CHAMBON LA FORET : 005 AK WINGST : 002 ESTIMATED AP : 002 ESTIMATED ISN : 047, BASED ON 26 STATIONS. NOTICEABLE EVENTS SUMMARY DAY BEGIN MAX END LOC XRAY OP 10CM Catania/NOAA RADIO_BURST_TYPES NONE 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 # # # # Legal notices: # # - Intellectual Property Rights: # # http://www.astro.oma.be/common/internet/en/data-policy-en.pdf # # - Liability Disclaimer: # # http://www.astro.oma.be/common/internet/en/disclaimer-en.pdf # # - Use and processing of your personal information: # # http://www.astro.oma.be/common/internet/en/privacy-policy-en.pdf # #--------------------------------------------------------------------#Lead Time: 51.00 hour(s) Difference: 0.50 hour(s) Prediction submitted by Leila Mays (GSFC) on 2015-07-20T12:30Z |
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