Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 14 - 20.08.2017, Forecast on 21 - 28.08.2017, Carrington Rotation 2193, 2194 (20.07; 16,48.08.2017) Earth above the ecliptic (3,3; 4,0) deg. (S30 - N38 is geoeffectiveness zone) SUNSPOT-FORMING ACTIVITY CHANGED FROM THE VERY LOW TO MIDDLE LEVELS. THE ESTIMATED, MOST LIKELY WEEKLY AVERAGE VALUE OF THE RELATIVE SUN- SPOT NUMBER IN THE INTERNATIONAL SYSTEM (old) FOR THE PERIOD W=018+8 /-11 (Wn=029+13/-18). ON THE VISIBLE SOLAR DISK 2 SMALL SUNSPOT GROUP. NEXT WEEK THE LEVEL OF SUNSPOT-FORMING ACTIVITY WILL REMAIN AT A MID- DLE LEVEL. THERE IS A PROBABILITY THAT SPOTLESS DAYS WILL BE OBSERVED UNTIL THE END OF THE PERIOD. MOST LIKELY WEEKLY AVERAGE VALUE OF THE RELATIVE SUNSPOT NUMBER IN THE INTERNATIONAL SYSTEM (old) FOR THE NEXT WEEK IS W= 030+20/-10. FLARE ACTIVITY WAS AT A VERY LOW ALL DAYS. ONE SOLAR FILAMENT EJEC- TIONS OCCURRENCES THROUGH THE PERIOD. ACCORDING TO THE DATA FROM SOHO AND STEREO CORONOGRAPHS NO CMEs HAVE BEEN OBSERVED. ---------------------------------------------------------------------- FLARES to tm te local. Class E(1-8A) AR RII/IV CME X-ray/Ïp J/m-2 20.08 0136 0152 0203 N06E89L M1.1/ 1.1E-02 12672 DSF to te ËÏÏÒÄÉÎÁÔÙ l × ÇÒÁÄ. Fl Aï CME/to 19.08 >0922 >0105 N29E17L 6 0001 --------------------------------------------------------------------- NEXT WEEK THE FLARE ACTIVITY WILL CHANGE BITWEEN A MIDDLE END A VERY LOW LEVELS. ON THE VISIBLE SOLAR DISK THE FOLLOWING CORONAL HOLES WERE OBSERVED: --------------------------------------------------------------------- sign N end E end S end W end Sch EE R G Space Obser. CH + N50L008 N30L318 N17L023 N22L040 16.08 4 SDO, SOHO... Sch - CH Square in Mm**2 (in square megameters) near the central meri- dian on http://sdowww.lmsal.com/suntoday/; n/d - no data; R - solar rotations; EE-date of possible geomag. disturbance in the Earth's environment. G(0-5)-geoeffectivity in last solar rotation on the middle latitudes. A-active geomagnetic condition. ------------------------------------------------------------------------ 16.08/02 UT THE EARTH IS IN "+" SECTOR OF THE INTERPLANETARY MAGNE- TIC FIELD. NEXT SECTOR BOUNDARY +/- EARTH SHOULD BE PASSED 0N 28.08. AUGUST 07 08 09 10 11 12 13 AUGUST Wus 011 011 011 011 011 011 011 F10.7 073 071 072 071 070 070 068 èbcg á5.2 á3.9 á3.5 á3.3 á3.0 á2.7 á2.9 GOES Sp 140 120 130 110 110 110 110 msh N IMF + + + + +/- - - DSCOVR Å>2 4.4å+8 5.3å+8 3.9E+8 3.2å+8 1.4å+8 2.6å+7 3.8å+7 GOES Ie>2 4301 10425 7825 6774 4952 920 978 pfu Ap 5 4 4 5 7 11 7 nô Dst nô KIOTO Amsc 4 4 5 6 7 10 8 nô IZMIRAN ------------------------------------------------------------------ Å>2 - Daily Electron Fluency e/(cm2-ster-day) with E>2 MeV. Ie>2 - the maximum intensity of electron flux in geostationary or- bits in days according to GOES15 in (electrons/cm2.s.sr) for events > 1000 pfu. THE GREATER THAN 2 MeV ELECTRON FLUX AT GEOSYNCHRONOUS ORBIT HAS BE- GIN 5.08/1405 UT UT AND 05 - 12.08 WAS OBSERVED. THE SECOND INCREASE HAS BEGUN 15.08/1245 UT AND 15-16.08 WERE OBSERVED. THE FOLLOWING IN- CREASE HAS BEGUN 18.08/1650 UT AND WAS OBSERVED 18 - 20.08, THE REA- SONS OF THE LAST ARE VERY MYSTERIOUS. THE GREATER THAN 2 MeV ELECTRON FLUX AT GEOSTATIONARY ORBIT OF VERY HIGH LEVEL IS EXPECTED 18 - 23?.08. MINOR MAGNETIC STORM (G1, Ams=34, dur. = 21 h.). HAS REGISTERED BOUL- DER CENTER DATA 17-18.08 WHEREAS ACCORDING IZMIRAN DATA THE SUBSTORM OF G1-INTENSITY AND 9 h. DURATION IS NOTED AT THIS TIME. SECOND MINOR MAGNETIC STORM (G1, Ams=34, dur.=42 h.) OCCURENCES 18-20.08 ACCORDING TO THE CENTER IN BOULDER AND (G1, Ams= 27, dur.= 39 h.) ACCORDING TO THE IZMIRAN DATA. THE 1st GEOMAGNETIC DISTURBANCE WAS CONNECTED WITH EARTH's PASSING OF THE HIGH-SPEED STREAM FROM THE CORONAL HOLE OF NOR- THERN SUBPOLAR CORONAL HOLE, ON WHICH THEN DISTURBANCE FROM SOLAR FI- LAMENT EJECTION 16.08 WITH CORONAL MASS EJECTON WAS IMPOSED. IN OTHER DAYS GEOMAGNETIC CONDITION WAS QUIET. NEXT WEEK THE GEOMAGNETIC CONDITION WILL BE UNSETTLED AND QUIET. HIGHLIGHT AND FORECAST COMPOSED FROM DATA: NOAA SWPC, BOULDER, USA http://www.swpc.noaa.gov, THE SOLAR INFLUENCES DATA ANALYSIS CENTRE, SIDC, BRUSSELS, BELGIUM http://sidc.oma.be/index.php3, THE IZMIRAN, MOSCOW, TROITSK, RUSSIA http://www.izmiran.ru V. Ishkov