Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 23 - 29.04.2018, Forecast on 30.04 - 06.05.2018, Carrington Rotation 2003 (19,22.04.2018) Earth out of ecliptic (-2.5 - -2.1) deg. (S28 - N25 is zone o geoeffectiveness) THE SUNSPOT-FORMING ACTIVITY OF THE SUN WAS ON VERY LOW LEVEL, THE VISIBLE DISK WAS SPOTLESS 28 -29.04 (69d ON 2018). THE ES- TIMATED, MOST LIKELY WEEKLY AVERAGE VALUE OF THE RELATIVE SUN- SPOT NUMBER IN THE INTERNATIONAL SYSTEM (old) FOR THE PERIOD W = 007+5/-7 (Wn = 011+10/-11). ON THE VISIBLE DISK ONE SMALL, QUITE SUNSPOT GROUP HAS BEEN OBSERVED. NEXT WEEK THE LEVEL OF SUNSPOT ACTIVITY WILL BE ON THE VERY LOW LEVEL AND WITH HIGH PROBABILITY THE SUN WILL BE SPOTLESS. LIKELY WEEKLY AVERAGE VALUE OF THE RELATIVE SUNSPOT NUMBER IN THE INTERNATIONAL SYSTEM (old) FOR THE NEXT WEEK IS W=010+10/ -10. FLARE ACTIVITY WAS ON THE VERY LOW LEVELS ON PERIOD. NO EJEC- TA OF SOLAR FILAMENTS AND TWO CORONAL MASS EJECTIONS (26 AND 29.04) HAVE BEEN OBSERVED. ---------------------------------------------------------------------- FLARES FROM M1 CLASSES to tm te local. Class E(1-8A) AR RII/IV CME X-ray/Ïp J/m-2 DSF to te localization l × ÇÒÁÄ. Fl AR CME/to --------------------------------------------------------------------- NEXT WEEK THE FLARE ACTIVITY IS EXPECTED AT 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. 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. ------------------------------------------------------------------------ AFTER 27.04/0100 UT EARTH IS IN "+" SECTOR OF INTERPLANETARY MAG- NETIC FIELD. NEXT SECTOR BOUNDARY +/- THE EARTH MUST PASS 9.05. APRIL 23 24 25 26 27 28 29 APRIL Wus 022 019 017 014 011 000 000 F10.7 074 073 071 069 069 070 071 èbcg á4.7 á4.3 á3.4 á3.1 á2.5 á2.6 á2.6 GOES Sp 080 050 050 020 010 000 000 msh N IMF - - - - -/+ + + DSCOVR Å>2 7.3E+8 4.9E+8 1.6E+8 17å+8 1.2å+8 5.4å+7 5.5å+7 GOES Ie>2 21958 15976 11840 4623 4841 2359 1250 pfu Ap 6 5 4 4 5 4 4 nô Dst nô KIOTO Amsc 8 5 4 5 6 4 5 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 BEGAN AT 10.04/0430 UT AND OBSERVED 10.03 - 29.04. NEXT WEEK THE GREATER THAN 2 MeV ELECTRON FLUX AT GEOSYNCHRONOUS ORBIT IS NOT EXPECTED4. GEOMAGNETIC CONDITION WAS UNSETTLED AND QUITE. NEXT WEEK THE GEOMAGNETIC CONDITION SHOULD BE QUITE AND UNSETTLED. 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