Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 22 - 28.07.2013, Forecast on 29.07 - 04.08.2013, Carrington Rotations 2139 (08,42.07.2013) SUNSPOT-FORMING ACTIVITY OF THE SUN REMAINED AT THE AVERAGE LEVEL, GRADUALLY INCREASING. WEEKLY, THE AVERAGE OF SUNSPOT NUMBER IN THE INTERNATIONAL SYSTEM WAS MADE W = 040+10/-8. ON THE VISIBLE SOLAR DISK CONSTANTLY THERE WERE 3 - 5 QUITE SUNSPOTS GROUPS. NEXT WEEK THE LEVEL OF SUNSPOT ACTIVITY IS EXPECTED TO BE THE AVE- RAGE LEVEL. THE CALCULATED MOST LIKELY WEEKLY AVERAGE VALUE OF SUNSPOT NUMBER IN THE INTERNATIONAL SYSTEM FOR THE NEXT WEEK IS EXPECTED W = 050+10/-10. FLARE ACTIVITY WAS AT THE LOW LEVEL. BY SOHO AND STEREO CORONO- GRAPHS DATA THERE WERE OBSERVED 24 CME FROM WHICH ONE WAS THE TYPE " HALO" AND ONE - "PARTIAL HALO II" TYPE. -------------------------------------------------------------------- FLARES to tm te c/p local. Class E(1-8A) AR RII/IV CME X / opt. J/m-2 DSF to te c/p local. l in deg. Fl AR CME 26.07 >0333 <0001 N16W11L120 12 28.07 >0924 <2332 S02W40L123 5 c/p local. - central part localization -------------------------------------------------------------------- NEXT WEEK THE FLARE ACTIVITY IS EXPECTED AT THE LOW AND SOMETIME AVE- RAGE LEVEL. ON THE VISIBLE SOLAR DISK THE FOLLOWING CORONAL HOLES WERE OBSERVED: --------------------------------------------------------------------- sign N end Å end S end W end EE R Observatories CH ? N05L106 S30L074 S35L076 N02L107 23.07 1 SDO, SOHO.. CH ? N20L164 N15L137 S12L147 N17L159 25.07 2 SDO, SOHO.. CH ? N52L005 N50L002 N22L027 N38L062 02.08 4 SDO, SOHO.. R - solar rotations; KP - KITT PEAK solar observatory; EE-date of possible geomag. disturbation in the Earth's environment. ---------------------------------------------------------------------- AFTER 25.07/14 UT EARTH IS IN "+" SECTOR OF THE INTERPLANETARY MAGNE- TIC FIELD. THE FOLLOWING SECTOR BOUNDARY -/ + THE EARTH SHOULD PASS AUGUST 07 - 08. JULY 22 23 24 25 26 27 28 JULY Wus 053 084 065 071 058 064 068 F10.7 110 107 108 107 110 108 109 èbcg ÷2.8 B2.5 B2.8 ÷2.2 B3.3 B3.2 B3.8 GOES Sp 240 250 320 340 330 340 470 m.v.h. N 3 1 1 1 IMF - - - -/+ + + + áóå Å>2 1.7å+8 6.6E+7 8.7E+7 7.3å+7 8.8å+6 2.8E+7 1.3E+7 GOES Ie>2 4016 1555 1905 2586 289 1430 365 GOES Ap 5 5 5 11 14 7 6 nT áÒ Dst nT KIOTO Amsc 9 7 6 14 14 14 10 nT IZMIRAN -------------------------------------------------------------------- Å>2 - a fluence in (electrons/cm2-day-sr) with E>2 MeV. Ie>2 - the maximum intensity of a flux of electrons in geostationary orbits in days according to GOES 15 in (electrons/cm2-s-sr) for events > 1000 p.f.u. THE GREATER THAN 2 MeV ELECTRON FLUX AT GEOSTATIONARY ORBIT VERY HIGH LEVEL BEGAN AT 11/01 UT AND OBSERVED TO 25 AND 27. THE GREATER THAN 2 MeV ELECTRON FLUX AT GEOSTATIONARY ORBIT VERY HIGH LEVEL IS NOT EXPECTED. MINOR GEOMAGNETIC STORM (G0, Ams = 27, dur.= 12 h.) WAS REGISTERED 25 -27 JULY ACCORDING BY DATA OF THE CENTER IN BOULDER. ACCORDING IZMIRAN DATA IN THIS DAY WAS REGISTERED SUBSTORM (9 h.) INTENSITE G0. IN OTHER DAYS GEOMAGNETIC CONDITION WAS UNSETTLED AND QUITE. NEXT WEEK THE GEOMAGNETIC SITUATION IS EXPECTED UNSETTLED AND QUITE. OF NOAA SWPC http://www.sec.noaa.gov, OF THE SOLAR INFLUENCES DATA ANALYSIS CENTER - SIDC, BELGIUM http://sidc.oma.be/index.php3, OF THE IZMIRAN, RUSSIA http://www.izmiran.ru