SOLAR SUNSPOT ACTIVITY OF THE SUN OF THE LAST PERIOD AGAIN HAS RISEN 
TO THE AVERAGE LEVEL. SETTLEMENT, RATING, WEEKLY AVERAGE OF SUNSPOT 
NUMBER IN THE INTERNATIONAL SYSTEM FOR THE PERIOD HAS MADE W=036+4/-26. 
ON THE VISIBLE DISK OF THE SUN IT WAS OBSERVED FROM ONE (13.06) TO 3 
SUNSPOT GROUPS.

NEXT WEEK A LEVEL OF SUNSPOT ACTIVITY IS EXPECTED LOW AND BY THE END OF 
THE PERIOD THE AVERAGE. THE MOST LIKELY THE CALCULATED WEEKLY AVERAGE 
VALUE OF SUNSPOT NUMBER IN THE INTERNATIONAL SYSTEM FOR THE NEXT PERIOD 
W=040+10/-10.

FLARE ACTIVITY WAS AT THE AVERAGE LEVEL ON JUNE, 14th WHEN IN SUNSPOT 
GROUP OF THE AVERAGE SIZE NEAR EAST LIMB THERE WAS FLARE OF X-RAY CLASS
 í1.3/SF, AND ON A LOW LEVEL IN OTHER DAYS. SOHO CORONOGRAPH FOR THE 
PERIOD ARE REGISTRED 32 CORONAL MASS EJECTIONS FROM THEM 2 TYPES "PARTIAL 
HALO II" (TO 180 deg.) 13.06 And III (TO 270 deg.) 14.06.

------------------------------------------------------------------------
      to   tm   te   location   Class   å(1-8A)  áR  Radio II/IV  CME Pr
                                X-ray Ïp J/m-2   
14.06 2136 2147 >2210 N15E47L174 M12.3/SF 1.8E-2 
        to    te   location      l × ÇÒÁÄ.   Fl  Aï        CME
DSF 14/0609  1500     SE                             CME/pH/750km/s
DSF 16/   1426    S23W335L250      10                CME/1612 UT
DSF 17/>0841 2157 S15W17L286               
---------------------------------------------------------------------

NEXT WEEK FLARE ACTIVITY IS EXPECTED ON LOW AND AVERAGE LEVELS.
 
ON THE VISIBLE SOLAR DISK FOR LAST WEEK WERE OBSERVED NEXT CORONAL HOLES:
--------------------------------------------------------------------------
  sign N end   å end   S end   W end       EE     R   Observatories
óî -  S05L154 S27L145 S31L149 S15L170  23.06   2   KP, SDO, SOHO.....
R - solar rotations; KP - KITT PEAK solar observatory;
EE - date of possible geomagnetic disturbation in the Earth's environment.
--------------------------------------------------------------------------
 
WITH 11.06/14 UT THE EARTH WAS IN + SECTOR OF THE INTERPLANETARY MAGNETIC 
FIELD. THE FOLLOWING SECTOR BOOUNDERY + /- THE EARTH SHOULD PASS ON 22.06.

JUNE    13     14     15     16     17     18     19     JUNE
Wus    016    048    048    062    065    067    047     
F10.7  087    099    102    103    104    099    099     
èbcg  B2.6   B2.4   B2.2   B3.0   B2.9   B2.3   ÷2.0     GOES
Sp     020    230    450    450    360    350    270
Nnew    1      1                    1             1
IMF     -      -      -      -      -      -    - /+     ACE
Å>2 1.0å+7 1.5å+7 2.8å+7 3.1E+7 1.5å+7 6.9å+6 5.5å+6     GOES
Nm%                                                      THULE
Ap      9      7      8      4      12     4      3      áÒ
Dst                                                      KIOTO
Amsc    11     9      10     8      11     8      9      IZMIRAN
-----------------------------------------------------------------

THE GREATER THAN 2 MeV ELECTRON FLUX AT GEOSYNCHRONOUS ORBIT WAS NOT 
OBSERVED.

NEXT WEEK THE GREATER THAN 2 MeV ELECTRON FLUX AT HIGH LEVEL IS 
NOT EXPECTED.

GEOMAGNETIC CONDITIONS WERE UNSETTLED ALL PERIOD. FROM EJECTION OF SOLAR 
FILAMENT 14.06 IN THE ENVIRONEMENT SPACE SUDDEN IMPULSE SI-17/0244 UT WAS 
OBSERVED, HOWEVER ON THE CONDITION OF THE GEOMAGNETIC FIELD IT PRACTICALLY 
WASN'T REFLECTED.

NEXT WEEK ON JUNE, 23RD THE EARTH WILL PASS THE HIGH-SPEED STREAM OF THE 
SOLAR WIND FROM CORONAL HOLE OF THE SOLAR SOUTHERN HEMISPHERE WHICH IN THE 
PREVIOUS TURN HAS CAUSED THE SMALL MAGNETIC STORM. PROBABILITY OF THE 
MAGNETIC STORM 23-24.06 ORDER OF 40 %. IN OTHER DAYS IT IS MOST PROBABLE 
QUIET AND UNSETTLED GEOMAGNETIC CONDITIONS.