Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 02 - 08.01.2012, Forecast on 09 - 16.01.2012, Carrington Rotations 2118, 2119 (13,61.12.2011; 09,94.01.2012) SOLAR SUNSPOT ACTIVITY OF THE LAST PERIOD WAS ON AVERAGE LEVEL. ESTIMATED, RATING, WEEKLY AVERAGE OF SUNSPOT NUMBER IN THE INTE- RNATIONAL SYSTEM FOR THE PERIOD WAS MADE W=060+11/-10. ON THE VISIBLE DISK OF THE SUN CONSTANTLY ARE PRESENT FROM 5 TO 7 SUN- SPOT GROUPS, AMONG WHICH ONE AVERAGE SIZE. NEXT WEEK THE LEVEL OF SUNSPOT ACTIVITY IS EXPECTED TO BE THE AVERAGE. THE CALCULATED MOST LIKELY WEEKLY AVERAGE VALUE OF SUN- SPOT NUMBER IN THE INTERNATIONAL SYSTEM FOR THE NEXT PERIOD W = 060+10/-10. FLARE ACTIVITY WAS ON LOW LEVEL IN ALL DAYS. BY DATA OF SOHO CO- RONOGRAPHS FOR THE PERIOD IT WAS OBSERVED 45 CORONAL MASS EJECTION AMONG WHICH WERE ONE TYPE "HALO" (2.01) AND 4 - TYPE "PARTIAL HALO II" (angular width 90-180 deg.). --------------------------------------------------------------------- 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 04.01/>2330 <1505 N30E03L067 14 05.01/ 1238 N30W11L067 16 C2 11392 CME c/p local. - central part localization --------------------------------------------------------------------- NEXT WEEK FLARE ACTIVITY IS EXPECTED ON LOW AND VERY LOW LEVELS. ON THE VISIBLE SOLAR DISK DURING THE LAST WEEK THE FOLLOWING CORONAL HOLES WERE OBSERVED : --------------------------------------------------------------------- sign N end Å end S end W end EE R Observatories CH - N18L051 S10L036 S13L039 N10L056 07.01 3 SDO, SOHO... CH + S19L004 S23L353 S30L359 S23L006 12.12 2 KP, SDO, SOHO... R - solar rotations; KP - KITT PEAK solar observatory; EE-date of possible geomag. disturbation in the Earth's environment. --------------------------------------------------------------------- WITH 05.01/23 UT THE EARTH WAS IN "-" SECTOR INTERPLANETARY MAGNETIC FIELDS. THE FOLLOWING SECTOR BOUNDERY - /+ THE EARTH SHOULD PASS ON 13.01. JANUARY 02 03 04 05 06 07 08 JANUARY Wus 083 095 101 099 118 110 090 F10.7 135 135 136 141 136 141 136 èbcg ÷4.1 ÷4.1 ÷3.9 ÷4.3 ÷4.8 ÷6.1 ÷6.1 GOES Sp 570 650 960 890 1000 1000 900 Nnew 1 1 1 1 1 IMF + + + +/- - - - ACE Å>2 9.9å+5 1.0å+6 1.2E+6 7.4å+5 7.2å+5 1.6å+6 5.8å+6 GOES Nm% THULE Ap 2 8 2 5 4 4 4 áÒ Dst ëIOTO Amsc 4 5 4 6 8 8 6 IZMIRAN --------------------------------------------------------------- THE GREATER THAN 2 MeV ELECTRON FLUX AT GEOSYNCHRONOUS ORBIT VERY HIGH LEVEL OF FLUX WAS NOT OBSERVED. THE GREATER THAN 2 MeV ELECTRON FLUX AT HIGH LEVEL IS NOT EXPECTED. ALL PERIOD GEOMAGNETIC CONDITIONS WERE UNSETTLED AND QUIET. NEXT WEEK GEOMAGNETIC CONDITIONS ARE EXPECTED QUIET AND UNSETTLED. HIGHLIGHT AND FORECAST COMPOSED FROM DATA 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