Weekly Bulletin on Solar and Geomagnetic Activity
               Highlights on 23 - 29.06.2014,
                Forecast on 30.06 - 06.07.2014,
 Carrington Rotation 2151, 2252 (31,83.05; 28,03.06.2014)

 SUNSPOT-FORMING ACTIVITY  REMAINED AT THE MIDDLE LEVEL. ESTIMATED, 
WEEKLY AVERAGE VALUE OF THE RELATIVE SUNSPOT NUMBER IN THE INTERNA-
TIONAL SYSTEM WAS MADE W=043+24/-21.  ON THE VISIBLE DISK OF THE 
SUN WERE CONSTANTLY OBSERVED 4 - 8 SMALL SUNSPOTS GROUPS.

NEXT WEEK THE MIDDLE LEVEL OF SUNSPOT-FORMING ACTIVITY IS EXPECTED. 
ESTIMATED, MOST LIKELY WEEKLY AVERAGE VALUE OF RELATIVE SUNSPOT NUM-
BER IN THE INTERNATIONAL SYSTEM  FOR THE NEXT WEEK  IS  EXPECTED W=
050+20/-20.

FLARE ACTIVITY  WAS ON A THE LOW LEVEL ALL DAYS, BUT 25 AND 27 JUNE
THE LEVEL OF FLARE ACTIVITY  WAS VERY LOW. FOR THE PERIOD 3 EJECTI-
ONS OF SOLAR FILAMENTS  WERE OBSERVED. BY DATA OF CORONOGRAPHS SOHO 
AND STEREO  WERE OBSERVED 35 CME, FOUR OF WHICH  WERE  THE TYPE  OF 
"PARTIAL HALO II".

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FLARES  to   tm  te   c/p local. Class  E(1-8A)   AR   RII/IV   CME
                                X-ray/Ïp J/m-2
 DSF     to      te   c/p local.     l in deg.  Fl    AR     CME
24.06 >0044   <1252  S15W08L051    6
25.06 >0138   <1245  N15E20L010    9
25.06 >0138   <1245  N01E16L014    4 
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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:
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  sign N end   Å end   S end   W end      EE   R  G   Observatories
CH  -  N08L026 N08L025 S13L043 S11L048  27.06  2      SDO, SOHO, ...
CH  -  N08L003 S05L000 S12L001 S02L005  30.06  2      SDO, SOHO, ...
CH  -  S40L344 S55L284 S70L324 S60L044  27.06  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.
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AFTER 26.06/03 UT THE EARTH IS IN "+" SECTOR OF THE INTERPLANETARY MAG-
NETIC FIELD. THE FOLLOWING SECTOR BOUNDER +/- THE EARTH HAS TO PASS ON 
JULY, 01.

JUNE      23     24     25     26     27     28     29       JUNE
Wus      064    037    052    072    078    089    112
F10.7    093    094    097    100    104    115    126      
èbcg    B1.6   B1.7   B1.8   B2.3   B4.6   B6.2    B6.8       GOES
Sp       170    130    240    240    150    230    660  mvh   
N                1      1             3      3      3     
IMF       -      -      -     -/+     +      +      +        áóå
Å>2   7.8E+6 1.6å+6 1.2å+6 9.4å+5 1.2å+6 1.0E+6 1.1E+6       GOES
Ie>2                                                    pfu  GOES 
Ap        4      7      6      4      3      6      8   nT   áÒ
Dst                                                     nT   KIOTO
Amsc      8      9      10     8      10     12     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