Weekly Bulletin on Solar and Geomagnetic Activity
               Highlights on 13 - 17.10.2014,
                Forecast on 18 - 27.10.2014,
   Carrington Rotations 2155, 2156 (17,72.09; 15,00.10.2014)
 
 SUNSPOT-FORMING ACTIVITY OF THE SUN  WAS AT THE AVERAGE LEVEL. 
ESTIMATED, WEEKLY AVERAGE VALUE OF THE RELATIVE SUNSPOT NUMBER 
IN THE INTERNATIONAL SYSTEM WAS MADE W = 34+20/-11. ON THE VI-
SIBLE DISK OF THE SUN CONSTANTLY OBSERVED 3 - 7 SMALL SUNSPOTS 
GROUPS. 
15.10 ON EAST LIMB THERE WAS AR12192 - CAR 12172+73 IN WHICH ON 
LAST ROTATION TWO LARGE FLARES WERE OCCURRED. FROM 7.10 ON THE 
BACK SIDE OF THE SUN (å"-40") IN CAR THE FAST INCREASE IN ITEN
SITY ON OBSERVATION OF THE GONG SIGNAL, AND 14, 16.10 WAS OBSER-
VED LARGE FLARES WHICH WERE REFLECTED IN THE VISIBLE DISK OF THE 
SUN AS FLARES OF THE CLASS M WERE OBSERVED.

NEXT WEEK THE AVERAGE AND LOW LEVELS OF SUNSPOT-FORMING ACTIVITY 
IS EXPECTED. ESTIMATED, MOST LIKELY WEEKLY AVERAGE VALUE OF RELA-
TIVE SUNSPOT NUMBER IN THE INTERNATIONAL SYSTEM FOR THE NEXT WEEK 
IS EXPECTED W = 040+10/-20.

 FLARE ACTIVITY WAS AT THE MIDDLE LEVEL ON 14 AND 16 OCTOBER, THE 
LOW LEVEL - IN OTHER DAYS.  THERE IS 6 EJECTIONS OF THE SOLAR FI-
LAMENTS. BY DATA OF CORONOGRAPHS SOHO AND STEREO WERE OBSERVED 20 
CME, ONE OF WHICH WAS THE "HALO" TYPE AND TWO - "PARTIAL GALO 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
14.10* 1821 1837 >1846 s13E90L252 M1.1/   9.7E-03  12192         CME
14.10* 1907 1921 >0019 s13E90L252 M2.2    3.1E-01  12192         CME
16.10  1258 1303 >1305 S13W88L120 M4.3    8.2E-03  12192         CME
* AR - 2 days for å-limb

DSF     to      te    c/p local.     l in deg.  Fl    AR     CME
14.10  >0018   >1331  S26W35L039       12
14.10   0844    0934  S19W44L048       10
15.10   2251    0234  N03E30L317       15                    
16.10  >1034   >0555  N02W67L051        7
17.10  >0003   >1332  N30E36L284        6
17.10  >0940   >2244  N25E29L291       23  
--------------------------------------------------------------------

NEXT WEEK FLARE ACTIVITY IS EXPECTED ON THE LOW AND THE AVERAGE LE-
VELS.LARGE AND POWERFUL FLARES ARE POSSIBLE IN AR12192 ONLY IN CASE 
OF EMERGENCE OF THE NEW SIGNIFICANT MAGNETIC FLUX. TODAY ENERGY OF 
LAST MAGNETIC FLUX IS SPENT.

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  +   N18L302 N17L304 S07L312 N05L325  20.10  1      SDO,SOHO....
CH  +   N45L302 N30L300 N20L308 N30L312  21.10  1      SDO,SOHO....
Possibly it is one very extended CH
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 11.10/10 UT  THE EARTH IS IN "-" SECTOR OF THE INTERPLANETARY 
MAGNETIC FIELD. THE FOLLOWING SECTOR BOUNDERY - / + THE EARTH HAS TO 
PASS 19.10.

OCTOBER   13      14    15     16     17     OCTOBER
Wus      041     070   090    060    039      
F10.7    113     120   126    139    146           
èbcg    ÷3.5    ÷3.7  Ó1.3   Ó1.1   Ó1.0     GOES
Sp       400     420   400    420    620 mvh   
N         1       1     2             1                  
IMF       -       -     -      -      -      áóå
Å>2   3.0E+5 1.5å+6 3.7å+5 4.0å+5 9.5å+5     GOES
Ie>2                                     pfu GOES 
Ap        8     19      12     7      8   nT  áÒ
Dst      -6    -50     -50    -26    -33  nT  KIOTO
Amsc      9     24      9      7      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 NOT OBSERVED.

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

MODERATE MAGNETIC STORM (G2, Ams=45, dur.=12 h.) ACCORDING IZMIRAN DA-
TA AND (G1, Ams= 45, dur.= 12 h.) ACCORDING BOULDER CENTRE DATA IT IS 
NOTED 14-15.10 AS A RESULT OF DISTURBANCE ARRIVAL FROM FILAMENT EJEC-
TION ON 10.10. IN OTHER DAYS THE GEOMAGNETIC CONDITION WAS UNSETTLED.

NEXT WEEK THE GEOMAGNETIC CONDITIONS IS EXPECTED ACTIVE ON OCTOBER 20
-21 WHEN THE EARTH  PASSES THE HIGH-SPEED STREAM  FROM NEAREQUATORIAL  
CORONAL HOLE. THE PROBABILITY OF THE MAGNETIC STORM  ISN'T LOWER THAN 
40%. BESIDES,  AFTER OCTOBER, 21 MAGNETIC STORMS  FROM POSSIBLE FLARE 
ACTIVITY OF AR12192 ARE POSSIBLE.

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