--------------------------------------------------------------------  
THE RELATIVE MONTHLY MEAN SUNSPOT NUMBER ON NOVEMBER 2013 HAS MADE 
                           Wnov.= 77.6, 
THAT GIVES FOR 59 MONTH (2013, MAY) DEVELOPMENT CURRENT 24 CYC-
LES OF SOLAR ACTIVITY THE SMOOTHED MONTHLY MEAN SUNSPOT NUMBER 
                           W*may = 57.9 
THE BEGINNING 24 CYCLES OF SOLAR ACTIVITY - I 2009 with W*=1.8
THE MOST PROBABLE TIME OF THE MAXIMUM OF THE CURRENT CYCLE-
                           XII.2013 - IV 2014
THE MOST PROBABLE HEIGHT OF THE MAXIMUM - Wmax = 66 - 75.

THE INTERNATIONAL DAILY VALUE OF RELATIVE SUNSPOT NUMBER FOR 2013, 
NOVEMBER ACCORDING DATA OF 62 SOLAR OBSERVATORIES HAS MADE 
      
      1.. 72    6.. 99   11.. 77   16..125   21.. 49   26.. 25m
      2.. 69    7..113   12.. 92   17..131M  22.. 46   27.. 50
      3.. 84    8.. 97   13..104   18.. 99   23.. 45   28.. 68
      4.. 87    9.. 71   14..118   19.. 77   24.. 49   29.. 67
      5.. 83   10.. 69   15..113   20.. 57   25.. 27   30.. 65
 
THE MONTHLY MEAN OF OBSERVED RADIO FLUX OF THE 10 cm (2800 MHz)ON 
2013, NOVEMBER              Fnov.= 132.1

THE MONTHLY MEAN OF GEOMAGNETIC Ap-index ON 2013, NOVEMBER
                          Ap nov.= 7.65
---------------------------------------------------------------------------


      Weekly Bulletin on Solar and Geomagnetic Activity
                Highlights on 25.11 - 01.12.2013,
               Forecast on 02 - 09.12.2013,
          Carrington Rotation 2144 (21,73.11.2013)

 SUNSPOT-FORMING ACTIVITY OF THE SUN REMAINED  AT AN AVERAGE LEVEL
SINCE NOVEMBER 2, GRADUALLY INCREASING. WEEKLY, THE AVERAGE OF SUN-
SPOT NUMBER IN THE INTERNATIONAL SYSTEM  WAS  MADE W = 049+13/-21. 
ON THE VISIBLE SOLAR DISK CONSTANTLY OBSERVED 4-6 SUNSPOT GROUPS  
ONE OF WHICH - THE  AN AVERAGE AREA.

NEXT WEEK IS EXPECTED THE AVERAGE LEVEL OF SUNSPOT ACTIVITY. ESTI-
MATED MOST LIKELY WEEKLY AVERAGE VALUE OF RELATIVE SUNSPOT NUMBER 
IN THE INTERNATIONAL SYSTEM FOR THE NEXT WEEK IS EXPECTED W = 060
+30/-20.

 FLARE ACTIVITY WAS FOR AT THE THE LOW ALL DAYS. DURING THE CONSI-
DERED PERIOD 3 DSF WERE OBSERVED.  BY SOHO  AND STEREO CORONOGRAPHS 
DATA THERE WERE OBSERVED 51 CME FROM WHICH ONE WAS THE "PARTIAL HALO 
III" TYPE AND 6 - "PARTIAL HALO II" TYPE.
--------------------------------------------------------------------
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
26.11 >1010    2237   S27E44L250       14
28.11  0104    0228   S08W47L315       17
01.12  0423    0541   S28E03L225       6  
c/p local. - central part localization 
--------------------------------------------------------------------

NEXT WEEK THE LEVEL OF THE FLARE ACTIVITY IS EXPECTED AT THE LOW LE-
VELS. 

ON THE VISIBLE SOLAR DISK THE FOLLOWING CORONAL HOLES WERE OBSERVED:
--------------------------------------------------------------------
  sign N end   Å end   S end   W end     EE  R  G   Observatories
óH  -  N10L180 N07L185 S05L200 S03L202 07.12 4  G1  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/
---------------------------------------------------------------------

AFTER 26.11/17 UT THE EARTH IS IN "+" SECTOR OF INTERPLANETARY MAGNE-
TIC FIELDS. THE FOLLOWING SECTORAL BOUNDARY +/- THE EARTH MUST PASS
1.12.

NOVEMBER  25     26     27     28     29     30     01     NOVEMBER
Wus      052    047    076    100    095    102    104
F10.7    119    116    129    133    129    131    131      
èbcg    B4.6   ÷4.5   B4.6   B5.0   ÷3.5   ÷3.5   ÷3.7       GOES
Sp       200    140    370    800    770    630    650  mvh   
N         1      1      2      1             1           
IMF       -     -/+     +      +      +      +      +        áóå
Å>2   9.0å+5 9.5å+5 9.4å+5 1.0å+6 1.1å+6 8.4E+6 9.8E+5       GOES
Ie>2                                                    pfu  GOES 
Ap        1      1      2      2      5      9      10   nT  áÒ
Dst                                                      nT  KIOTO
Amsc      4      4      5      6      12     12     9    nT  IZMIRAN
--------------------------------------------------------------------
Å>2 - the fluxes in (electrons/cm2-day-sr) with E>2 MeV.
Ie>2 - the maximum intensity of a flux of electrons in geostationary 
orbits in days according to GOES 15 in (electrons/cm2-s-sr) for events
> 1000 p.f.u.

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

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

GEOMAGNETIC CONDITION IS CHANGING FROM UNSETTLED TO THE LOW.  

 NEXT WEEK THE GEOMAGNETIC CONDITION  IS EXPECTED UNSETTLED AND QUIET 
ALL DAYS, EXCEPT 7.12 WHEN THE EARTH WILL PASS HIGH-SPEED STREAM FROM 
SOLAR NEAR EQUATORIAL CORONAL HOLE. PROBABILITY OF THE MAGNETIC STORM 
NOT LESS THAN 30%.

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