--------------------------------------------------------------------  
THE RELATIVE MONTHLY MEAN SUNSPOT NUMBER ON JUNE 2014 HAS MADE 
                           Wjune= 71.0, 
THAT GIVES FOR 65 MONTH (2013, DECEMBER) DEVELOPMENT CURRENT 24 
CYCLES OF SOLAR ACTIVITY THE SMOOTHED MONTHLY MEAN SUNSPOT NUMBER 
                           W*dec. = 76.0 
THE BEGINNING 24 CYCLES OF SOLAR ACTIVITY - I 2009 with W*=1.8
THE MOST PROBABLE TIME OF THE MAXIMUM OF THE CURRENT CYCLE-
                           I 2014 
THE MOST PROBABLE HEIGHT OF THE MAXIMUM - Wmax = 78

THE INTERNATIONAL DAILY VALUE OF RELATIVE SUNSPOT NUMBER FOR 2014, 
JUNE ACCORDING DATA OF 69 SOLAR OBSERVATORIES HAS MADE 
      
      1.. 44    6.. 82   11..120   16.. 58   21.. 64   26.. 46
      2.. 43    7.. 92   12..136í  17.. 66   22.. 62   27.. 46
      3.. 51    8.. 98   13..126   18.. 83   23.. 53   28.. 49
      4.. 44    9..108   14.. 95   19.. 66   24.. 28Í  29.. 64
      5.. 60   10..112   15.. 51   20.. 55   25.. 38   30.. 91

THE MONTHLY MEAN OF OBSERVED RADIO FLUX OF THE 10 cm (2800 MHz ON 
2014, JUNE                 Fjune = 122.0

THE MONTHLY MEAN OF GEOMAGNETIC Ap-index ON 2014, JUNE
                          Ap june = 6.7
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     Weekly Bulletin on Solar and Geomagnetic Activity
               Highlights on 30.06 - 06.07.2014,
                Forecast on 07 - 14.07.2014,
          Carrington Rotation 2252 ( 28,03.06.2014)

 SUNSPOT-FORMING ACTIVITY AFTER JUNE, 1 REMAINED AT THE HIGH LEVEL. 
ESTIMATED, WEEKLY AVERAGE VALUE OF THE RELATIVE SUNSPOT NUMBER IN 
THE INTERNATIONAL SYSTEM WAS MADE W = 112+42/-38.  ON THE VISIBLE 
DISK OF THE SUN WERE CONSTANTLY OBSERVED 8-11 SUNSPOTS GROUPS FROM
WHICH TWO WERE THE MIDDLE SIZE AND ONE - THE LARGE SIZE:
AR12109 (S08L220, Sp=830 mvh) left on a visible disk of the Sun on 
June 1, by June 4 the area reached level of big group and continues 
to increase the area, but remains quiet, while..

NEXT WEEK THE HIGH AND THE MIDDLE LEVEL OF SUNSPOT-FORMING ACTIVITY 
IS EXPECTED. ESTIMATED, MOST LIKELY WEEKLY AVERAGE VALUE OF RELATIVE 
SUNSPOT NUMBER IN THE INTERNATIONAL SYSTEM  FOR THE NEXT WEEK IS EX-
PECTED W = 070+20/-20.

 FLARE ACTIVITY  WAS ON A THE MIDDLE LEVEL AT JUNE 1  AND THE LOW IN
OTHER DAYS. FOR THE PERIOD 3 EJECTIONS OF SOLAR FILAMENTS WERE OBSER-
VED.  BY DATA OF CORONOGRAPHS SOHO AND STEREO  WERE OBSERVED 34 CME, 
ONE OF WHICH WERE THE TYPE OF "PARTIAL HALO II".

-------------------------------------------------------------------
FLARES  to   tm  te   c/p local. Class  E(1-8A)   AR   RII/IV   CME
                                X-ray/Ïp J/m-2
01.07 1105 1123 >1159 N12E60L261 V1.4/   3.5E-2 12106

 DSF     to      te   c/p local.     l in deg.  Fl    AR     CME
05.07 >0040   <1308  N36E24L230       16
05.07  0724   <1243  N38E33L198       11      
05.07 >1715   <0505  S43E59L221       19             
--------------------------------------------------------------------

NEXT WEEK FLARE ACTIVITY IS EXPECTED ON LOW AND, IN SEPARATE DAYS, 
AT THE AVERAGE LEVEL.

ON THE VISIBLE SOLAR DISK THE FOLLOWING CORONAL HOLES WERE OBSERVED:
--------------------------------------------------------------------
  sign N end   Å end   S end   W end      EE   R  G   Observatories
CH  -  N08L003 S05L000 S12L001 S02L005  30.06  2      SDO, SOHO, ...
CH  +  N01L325 S05L317 S08L325 S05L334  03.07  1      SDO, SOHO, ...
CH  +  N06L254 S05L252 S10L254 S02L259  09.07  2      SDO, SOHO, ..
R - solar rotations; KP - KIT PEAK solar observatory;
EE-date of possible geomag. disturbance in the Earth's environment.
G - geoeffectivity in last solar rotation; 
A-active geomagnetic condition.
---------------------------------------------------------------------

AFTER 03.07/05 UT THE EARTH IS IN "-" SECTOR OF THE INTERPLANETARY MAG-
NETIC FIELD. THE FOLLOWING SECTOR BOUNDER -/+ THE EARTH HAS TO PASS ON 
JULY, 08.

JUNE      30     01     02     03     04     05     06       JUNE
Wus      124    154    180    179    199    213    256
F10.7    141    152    169    178    188    193    201      
èbcg    B7.7   B9.6   B8.9   B8.8   C1.0   B9.6    ó1.2       GOES
Sp       750    850   1260   1430   1830   2090   2230  mvh   
N                1      1      1      1      1      1     
IMF       +      +      +     +/-     -      -      +        áóå
Å>2   1.3E+5 1.9å+5 3.2å+5 2.4å+5 1.8å+5 2.6E+5 2.7E+5       GOES
Ie>2                                                    pfu  GOES 
Ap        7      4      4      7      5      3      4    nT   áÒ
Dst                                                      nT  KIOTO
Amsc      9      12      11     11     9     8      9    nT  IZMIRAN
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Å>2 - Daily Electron Fluency e/(cm2-ster-day) with E>2 MeV.
Ie>2 - the maximum intensity of electron flux in geostationary orbits 
in days according to GOES 15 in (electrons/cm2-s-sr) for events
> 1000 pfu.

THE GREATER THAN 2 MeV ELECTRON FLUX AT GEOSTATIONARY ORBIT VERY HIGH 
LEVEL WAS NOT OBSERVED.

THE GREATER THAN 2 MeV ELECTRON FLUX AT GEOSTATIONARY ORBIT VERY HIGH 
LEVEL BE NOT EXPECTED.

ALL DAYS THE GEOMAGNETIC CONDITIONS REMAINED QUIET AND UNSETTLED.

NEXT WEEK THE GEOMAGNETIC CONDITIONS ARE EXPECTED UNSETTLED AND QUIET.

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