SIDC ursigram
3-day-forecast of solar and geomagnetic activity.Source | SIDC (RWC-Belgium) |
Frequency | Daily |
Format | Encoded data (ISES) |
Mail header | SIDC ursigram |
SIDC code | uge |
Latest issue
:Issued: 2022 Aug 13 1230 UTC :Product: documentation at http://www.sidc.be/products/uge #--------------------------------------------------------------------# # DAILY BULLETIN ON SOLAR AND GEOMAGNETIC ACTIVITY from the SIDC # #--------------------------------------------------------------------# SIDC URSIGRAM 20813 GEOALERT BRU225 UGEOA 30512 20813 1230/ 9930/ 11132 20132 30132 99999 PLAIN NOTE: the above forecasts are valid from 1230UT, 13 Aug 2022 until 15 Aug 2022 COMMENT: Several C flares occurred in the past 24 hours. Most of them from the newly emerged NOAA active region 3079 in the South as reported yesterday. The strongest flare was a C6.8 flare peaking at 7:31UTC. This bipolar region developed a dominant trailing spot and exhibits mixed polarity field in the intermediate area. The unipolar active regions NOAA 3071 and 3074 were stable while unipolar region NOAA 3078 showed some growth and became bipolar. The bipolar NOAA active region 3077 has decayed just as the newly numbered NOAA active region 3080 which was shortlived. The now bipolar region NOAA 3076 in the north has grown following the new flux emergence reported yesterday. Another bipolar region has recently emerged rapidly in the north east (NOAA active region 3081). All in all, C class flaring is very likely with now also chances for M class flaring. No Earth-directed coronal mass ejections (CMEs) were detected in the available coronagraph imagery. The greater than 10 MeV proton flux was at nominal levels in the past 24 hours and is expected to remain so in the next days. The greater than 2 MeV electron flux remained above the 1000 pfu threshold and is expected to remain above or around the threshold in the next 24 hours. The 24h electron fluence was at moderate levels and is expected to be at moderate levels with a slow decreasing trend. Declining high speed Solar wind conditions were recorded. Solar wind speed decreased from around 575 to just over 500 km/s while the interplanetary magnetic field strength varied around 5nT. The magnetic field orientation showed mostly a connection to a positive sector (field away from the Sun). Over the next 24 hours Solar wind speed is expected to continue the decreasing trend and slowly return towards slow Solar wind conditions. Geomagnetic conditions were quiet to unsettled (both local K Dourbes and NOAA Kp 1-3). Geomagnetic conditions are expected to be quiet to unsettled over the next days. TODAY'S ESTIMATED ISN : 126, BASED ON 19 STATIONS. UGEOI 30512 20813 1230/ 12/// 1//// 21200 3//// 4//// 8//// 9//// 99999 UGEOR 30512 20813 1230/ 11/09 13105 10003 2//// 3//// 472// 50100 60001 34217 00000 10006 2//// 3//// 472// 50150 60001 30615 00000 10008 2//// 3//// 4442/ 50180 60014 12318 03000 10009 2//// 3//// 4311/ 50050 60013 32817 01000 10010 2//// 3//// 472// 50040 60002 25324 01000 99999 UMAGF 30503 20813 1004/ 12065 1/012 22321 31112 BT #--------------------------------------------------------------------# # Solar Influences Data analysis Center - RWC Belgium # # Royal Observatory of Belgium # # # # Website http://www.sidc.be. # # E-mail sidc-support@oma.be # # To unsubscribe http://www.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 # #--------------------------------------------------------------------#
Details
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