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Prediction for CME (2016-07-23T05:24:00-CME-001)CME Observed Time: 2016-07-23T05:24ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/11056/-1 CME Note: large spray of cooler material ejected from the active region with this CME, associated with double peaked flare. CME was not detected at Earth. Observed Geomagnetic Storm Parameters due to CME: ---- Predicted Arrival Time: 2016-07-25T21:00Z (-12.0h, +12.0h) Confidence that the CME will arrive: 15.0% Predicted geomagnetic storm max Kp range due to CME: 2.0 - 5.0 Prediction Method: Other (SIDC) Prediction Method Note: :Issued: 2016 Jul 23 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 60723 SIDC SOLAR BULLETIN 23 Jul 2016, 1230UT SIDC FORECAST (valid from 1230UT, 23 Jul 2016 until 25 Jul 2016) SOLAR FLARES : M-class flares expected (probability >=50%) GEOMAGNETISM : Quiet (A<20 and K<4) SOLAR PROTONS : Warning condition (activity levels expected to increase, but no numeric forecast given) PREDICTIONS FOR 23 Jul 2016 10CM FLUX: 093 / AP: 008 PREDICTIONS FOR 24 Jul 2016 10CM FLUX: 090 / AP: 006 PREDICTIONS FOR 25 Jul 2016 10CM FLUX: 087 / AP: 016 COMMENT: NOAA 2567 started another active flaring episode shortly after midnight producing 3 M-class flares. The intensities and peak timings of the events were resp. M5.0 (02:11UT), M7.6 (05:16UT), and M5.5 (05:31UT). In particular the last event was accompanied by an impressive ejection of material. San Vito reported a type II radio burst with related shock speed of the disturbance of 729 km/s. The greater than 10 MeV proton flux is somewhat enhanced (0.77 pfu at 07:25UT), but has remained so far well below the event threshold (10 pfu). The currently available coronagraphic images show that the bulk of the associated coronal mass ejections (CMEs) is directed away from the Earth. However, a glancing blow from the CME of the double-peaked M-class event cannot be excluded. No other earth-directed CMEs were observed. An accurate assessment of the magnetic configuration of the NOAA 2565 / 2567 sunspot cluster is difficult due to its close proximity near the west limb. Nonetheless, further M-class flaring is possible, with a small chance on an X-class flare. A warning for a potential proton event has been put into effect. The interplanetary magnetic field was directed towards the Sun (negative), except during the 17:00-02:00UT interval when it was steadily positive (away from the Sun). This interval corresponded to somewhat elevated solar wind speeds between about 440 and 500 km/s and Bz near 0 nT. At the end of the reporting period, solar wind parameters were back at nominal values with wind speed near 390 km/s, and Bz varying between -8 and +7 nT. A small positive coronal hole (CH; latitude +20 degrees) is near the central meridian. Quiet to unsettled geomagnetic conditions were observed. Mostly quiet to unsettled geomagnetic conditions are expected. An active episode is not excluded, in particular on 25 July when a glancing blow from the 23 July CME is possible. TODAY'S ESTIMATED ISN : 030, BASED ON 22 STATIONS. SOLAR INDICES FOR 22 Jul 2016 WOLF NUMBER CATANIA : 057 10CM SOLAR FLUX : 090 AK CHAMBON LA FORET : 018 AK WINGST : 012 ESTIMATED AP : 011 ESTIMATED ISN : 044, BASED ON 30 STATIONS. NOTICEABLE EVENTS SUMMARY DAY BEGIN MAX END LOC XRAY OP 10CM Catania/NOAA RADIO_BURST_TYPES 23 0146 0211 0223 ////// M5.0 09/2567 VI/2III/2 23 0500 0516 0524 N02W74 M7.6 3B 310 09/2567 III/2 23 0527 0531 0533 ////// M5.5 900 09/2567 V/3IV/2II/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 # # # # 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: 38.03 hour(s) Difference: ----- Prediction submitted by Leila Mays (GSFC) on 2016-07-24T06:58Z |
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