Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 3 - 9.04.2017, Forecast on 10 - 17.04.2017, Carrington Rotation 2189 (2,37.04.2017) Earth above the ecliptic (-6.4, -6,0) deg. (S30-N25 is geoeffectiveness zone) SUNSPOT-FORMING ACTIVITY WAS ON A HIGH (3.04), THE MIDDLE (4 -6.04), THE LOW - 7, THE VERY LOW - 9.04 LEVELS AND 8.04 WAS SPOTLESS DAY (27 ON THIS YEAR). THE ESTIMATED, MOST LIKELY WEEKLY AVERAGE VALUE OF THE RELATIVE SUNSPOT NUMBER IN THE INTERNATIONAL SYSTEM (old) FOR THE THE PERIOD IS W=25+33/-25 (Wn= 39+54/-39). ON THE VISIBLE DISC OF THE SUN 4 -0 SUNSPOT GROUP, ONE WAS A BIG SIZE AND QUITE AR12645 (S08L012, Sp max=600 msh) HAVE BEEN OBSERVED. THE AR HAD MOSTLY TRANSITED AROUND THE W-limb AT 7.04 WITH ONLY THE TRAILING SPOTS VISIBLE FROM THIS LAR- GE ELONGATED AR. NEXT WEEK SUNSPOT-FORMING ACTIVITY IS EXPECTED AT THE LOW LEVEL. THE ESTIMATED, MOST LIKELY WEEKLY AVERAGE VALUE OF THE RELATIVE SUN- SPOT NUMBER IN THE INTERNATIONAL SYSTEM (old) FOR THE NEXT WEEK IS W= 30+10/-30. FLARE ACTIVITY WAS AT THE LARGE LEVEL 03.04 AND THE LOW IN OTHER DAYS. ONE SOLAR FILAMENT EJECTION OCCURRENCES THROUGH THE PERIOD. ACCORDING TO THE SOHO AND STEREO CORONOGRAPHS DATA > 10 CMEs HAVE BEEN OBSERVED. ---------------------------------------------------------------------- FLARES to tm te local. Class E(1-8A) AR RII/IV CME X-ray/Ïp J/m-2 03.04 0056 0105 >0112 N15W75L054 M1.2/SF 8.2E-03 12644 03.04 1415 1429 1454 N19W80L054 2N/M5.8 3.1E-02 12644 II/2 IV/1 CME DSF to te ËÏÏÒÄÉÎÁÔÙ l × ÇÒÁÄ. Fl Aï CME/to 03.04 >0101 >1315 N29W32L023 4 ---------------------------------------------------------------------- NEXT WEEK FLARE ACTIVITY IS EXPECTED AT A LOW AND 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 + N38L298 N25L293 N08L303 N30L308 10.04 >9 SDO, SOHO.. CH + N05L317 N03L312 S02L320 N02L323 03.04 1 SDO, SOHO.. Both CH, perhaps, parts of one CH. 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. ------------------------------------------------------------------------ FROM 26.03/2130 UT THE EARTH IS IN "-" SECTOR OF THE INTERPLANETARY MAG- NETIC FIELD. 3-4 AND 8-9.04 THE SIGN OF SECTOR HAVE BEEN CHANGED. THE FOLLOWING SECTOR BOUNDARY -/+ THE EARTH HAS EXPECTED TO PASS 10.04. APRIL 03 04 05 06 07 08 09 APRIL Wus 097 075 037 038 027 000 013 F10.7 108 094 085 076 074 073 074 èbcg ó1.2 ÷5.5 ÷2.7 ÷1.6 á9.4 ÷1.0 á7.2 GOES Sp 1270 890 550 400 070 000 020 msh N 1 1 IMF ~ ~ - - - ~ ~ DSCOVR Å>2 1.9å+9 8.6å+7 5.7E+6 6.0E+6 7.8E+6 1.2å+7 8.3å+7 GOES Ie>2 53552 18021 210 241 224 491 3029 pfu Ap 3 19 10 7 10 16 18 nô BOULDER Dst nô KIOTO Amsc 8 15 11 12 9 11 11 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 WAS BE- GINING AT 22.03/1530 UT AND OBSERVED 22.03-04.04. NEXT INCREASE WAS BEGINING AT 09.04/1330 UT. THE GREATER THAN 2 MeV ELECTRON FLUX AT GEOSTATIONARY ORBIT OF VERY HIGH LEVEL IS EXPECTED 10 - 12.04. MINOR STORM CONDITION (G1, Ams=31, dur.=12 h.) OBSERVED ONLY IN BOUL- DER CENTER 8 - 9.04 AND 4.04 IN BOULDER CENTER OBSERVED SUBSTORM (G1, dur.= 9 h.). IN OTHER DAYS THE GEOMAGNETIC CONDITION WAS UNSETTLED. NEXT WEEK GEOMAGNETIC CONDITION WILL BE QUIET 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