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OK0NAG > SOLAR    11.03.12 15:05l 121 Lines 4759 Bytes #999 (0) @ EU
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Subj: GEOALERT SIDC
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Date: Sun, 11 Mar 2012 13:02:43 GMT
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Subject: GEOALERT SIDC
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:Issued: 2012 Mar 11 1301 UTC
:Product: documentation at http://www.sidc.be/products/xut
#--------------------------------------------------------------------#

# GEOALERT message from the SIDC (RWC-Belgium)                       #

#--------------------------------------------------------------------#


GEOALERT BRU071
UGEOA 30512 20311 1237/ 9930/
12112 24112 37112
99999
PLAIN
NOTE: the above forecasts are valid from 1230UT, 11 Mar 2012 until 13 Mar 
2012
PREDICTIONS FOR 11 Mar 2012  10CM FLUX: 152 / AP: 051
PREDICTIONS FOR 12 Mar 2012  10CM FLUX: 150 / AP: 032
PREDICTIONS FOR 13 Mar 2012  10CM FLUX: 152 / AP: 058
COMMENT: Catania sunspot group 65 (NOAA AR 1429) maintains
beta-gamma-delta configuration of its photospheric magnetic field, and

two more groups (still unnumbered) appeared from behind the east limb.

We expect continuous flaring activity on the C-level, and another
M-class flare is probable, especially in Catania sunspot group 65 (NOAA

AR 1429). An X-class flare is possible, but unlikely. Catania sunspot
group 65 (NOAA AR 1429) produced an M8.4 flare peaking at 17:44 UT
yesterday. The flare was accompanied by coronal dimmings, an EIT wave
and a post-eruption arcade observed by SDO/AIA, and a full halo CME
first detected in the SOHO/LASCO C2 field of view at 18:00 UT.
STEREO/SECCHI COR2 data indicate that the bulk of the CME material is
directed northward of the ecliptic plane. A preliminary estimate of the

CME plane-of-the-sky speeds in the LASCO and COR2 A data gives values
around 900 and 800 km/s respectively. We expect the corresponding ICME

to arrive at the Earth early on March 13, resulting in a moderate to
strong (K = 6-7) geomagnetic storm. The Earth is currently inside a slow

(around 440 km/s) solar wind flow with weak to average (2-4 nT)
interplanetary magnetic field magnitude. We expect quiet geomagnetic
conditions in the next several hours. Later this evening (or tomorrow
morning) we expect a strong (K = 7 or higher) geomagnetic storm due to

the arrival of the magnetic cloud corresponding to the full halo CME on

March 9. The proton event is still going on, and we expect it to last
for at least another 12 hours.

TODAY'S ESTIMATED ISN  : 081, BASED ON 10 STATIONS.
99999
UGEOI 30512 20311 1237/ 10///
1//// 21491 3024/ 4//// 8//// 9////
99999

NOTICEABLE EVENTS SUMMARY
DAY BEGIN MAX  END  LOC    XRAY OP  10CM RADIO BURST TYPES     Catania 
NOAA NOTE
10  1715  1744 1830 N17W24 M8.4      460 IV/2                          
 65 1429 Location taken from SolarSoft Events
END

UGEOR 30512 20311 1237/ 08/10 11104
10062 2//// 3//// 4201/ 50010 60003 36527 00000
10063 2//// 3//// 4422/ 50200 60015 30915 01000
10064 2//// 3//// 4432/ 50160 60015 40619 04100
10065 2//// 3//// 4552/ 50830 60039 10917 29522
99999
UMAGF 30503 20311 1004/ 10060 1/021 23223 34221 
UMAGF 31523 20311 ///// 1000/ 1/024 25533 32442 
 
#--------------------------------------------------------------------#

# Solar Influences Data analysis Center - RWC Belgium                #

# Royal Observatory of Belgium                                       #

# Fax : 32 (0) 2 373 0 224                                           #

# Tel.: 32 (0) 2 373 0 491                                           #

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