--------------------------------------------------------------------  
THE RELATIVE MONTHLY MEAN SUNSPOT NUMBER ON MAY 2014 HAS MADE 
                           Wmay= 75.2, 
THAT GIVES FOR 64 MONTH (2013, NOVEMBER) DEVELOPMENT CURRENT 24 
CYCLES OF SOLAR ACTIVITY THE SMOOTHED MONTHLY MEAN SUNSPOT NUMBER 
                           W*nov. = 75.4 
THE BEGINNING 24 CYCLES OF SOLAR ACTIVITY - I 2009 with W*=1.8
THE MOST PROBABLE TIME OF THE MAXIMUM OF THE CURRENT CYCLE-
                           XI 2013 
THE MOST PROBABLE HEIGHT OF THE MAXIMUM - Wmax = 75.4

THE INTERNATIONAL DAILY VALUE OF RELATIVE SUNSPOT NUMBER FOR 2014, 
MAY ACCORDING DATA OF 66 SOLAR OBSERVATORIES HAS MADE 
      
 1.. 59    6.. 99   11..100   16.. 89   21.. 57   26.. 61   31.. 38
 2.. 77    7.. 80   12..103   17..101   22.. 44   27.. 52
 3.. 82    8.. 88   13.. 89   18.. 92   23.. 61   28.. 47
 4.. 85    9.. 93   14..111M  19.. 68   24.. 73   29.. 32m
 5.. 95   10.. 82   15..104   20.. 58   25.. 73   30.. 37

THE MONTHLY MEAN OF OBSERVED RADIO FLUX OF THE 10 cm (2800 MHz ON 
2014, MAY                 Fmay= 129.7

THE MONTHLY MEAN OF GEOMAGNETIC Ap-index ON 2014, MAY
                          Ap may= 5.7
---------------------------------------------------------------------------
 

     Weekly Bulletin on Solar and Geomagnetic Activity
               Highlights on 26.05 - 01.06.2014,
              Forecast on 02 - 09.06.2014,
  Carrington Rotation 2150, 2151 (04,62.05; 31,83.05.2014)

 SUNSPOT-FORMING ACTIVITY OF THE SUN REMAINED AT THE AVERAGE LEVEL,
GRADUALLY DECREASING BY THE PERIOD END. ESTIMATED,  WEEKLY AVERAGE 
VALUE OF THE RELATIVE SUNSPOT NUMBER IN THE INTERNATIONAL SYSTEM 
WAS MADE W=47+19/-14. ON THE VISIBLE SOLAR DISK CONSTANTLY OBSERVED 
6-4 SMALL SUNSPOT GROUPS.

NEXT WEEK IS EXPECTED THE AVERAGE LEVEL OF SUNSPOT-FORMING ACTIVITY. 
ESTIMATED, MOST LIKELY WEEKLY AVERAGE VALUE OF RELATIVE SUNSPOT NUM-
BER IN THE INTERNATIONAL SYSTEM FOR THE NEXT WEEK IS EXPECTED W=050
+10/-20.

FLARE ACTIVITY WAS AT A LOW LEVEL AND ONLY 30.04 ON VERY LOW. WITHIN 
THE PERIOD WERE OBSERVED 5 SOLAR FILAMENT EJECTIONS. BY SOHO AND STE-
REO CORONOGRAPHS DATA THERE WERE OBSERVED 43 CME, 4 OF WHICH WERE OF 
"PARTIAL HALO II" TYPE.

-------------------------------------------------------------------
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
27.05  >0105  <1228  N00E23L033        6                     
29.05  >0029  <1238  S03E15L015        5            
29.05  >0921  <1237  N25W48L078       12 
01.06  >0125  <1125  N05E26L321        4
01.06  >0918  >2331  N23W46L036       10 
--------------------------------------------------------------------

NEXT WEEK FLARE ACTIVITY IS EXPECTED AT THE AVERAGE LEVELS.

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  -  S02L012 S04L007 S19L008 S10L014   3.06  2  G0  SDO, SOHO, ...
CH  -  S40L344 S60L327 S70L344 S38L357   3.06  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.
---------------------------------------------------------------------

AFTER 27.05/21 UT THE EARTH IS IN "+" SECTOR OF THE INTERPLANETARY MAG-
NETIC FIELD THOUGH 29 AND 30.05 SIGN OF THE FIELD REPEATEDLY CHANGED.  
THE FOLLOWING SECTOR BOUNDER +/-THE EARTH HAS TO PASS ON JUNE, 4.

MAY       26     27     28     29     30     31     01       MAY
Wus      110    096    072    055    056    056    108
F10.7    108    106    099    103    102    104    103      
èbcg    B3.8   B3.2   ÷2.5   ÷2.4   ÷2.4   ÷2.5   B2.5       GOES
Sp       510    210    500    100    110    130    260  mvh   
N                       1             1             2      
IMF       -     -/+     +     +/-    -/+     +      +        áóå
Å>2   7.7E+6 1.4å+7 2.3å+6 6.1å+5 1.2å+5 2.1E+5  1.8E+5      GOES
Ie>2                                                    pfu  GOES 
Ap        3      4      4      6      9      4      4    nT   áÒ
Dst                                                      nT  KIOTO
Amsc      8      11     9      12     15     9      8    nT  IZMIRAN
--------------------------------------------------------------------
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.

GEOMAGNETIC CONDITIONS REMAIN QUITE ABD 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