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OK0NAG > SOLAR    13.09.17 14:32l 144 Lines 5040 Bytes #999 (0) @ EU
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Subj: GEOALERT SIDC
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Date: Wed, 13 Sep 2017 12:30:12 GMT
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Subject: GEOALERT SIDC

:Issued: 2017 Sep 13 1230 UTC
:Product: documentation at http://www.sidc.be/products/xut
#--------------------------------------------------------------------#

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

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

GEOALERT BRU256
UGEOA 30512 70913 1230/ 9930/ 
10132 21132 37132 
99999
PLAIN
NOTE: the above forecasts are valid from 1230UT, 13 Sep 2017 until 15 Sep 
2017
PREDICTIONS FOR 13 Sep 2017  10CM FLUX: 077 / AP: 023
PREDICTIONS FOR 14 Sep 2017  10CM FLUX: 076 / AP: 015
PREDICTIONS FOR 15 Sep 2017  10CM FLUX: 075 / AP: 008
COMMENT: Strongest flare observed in the last 24 hours was the C1.6 flare

(peaked at 19:20 UT on September 12), which originated from the Catania

sunspot group 55 (NOAA AR 2680). The flare was, similarly to the C-class

flare from this active region reported yesterday, associated with the EIT

wave, coronal dimming, and rather slow and narrow CME (with projected speed

of 350 km/s and angular width of about 100 degree). This CME will not
arrive at the Earth.
We might expect more isolated C-class flares in the coming hours
(probability is about 25%), in particular from the Catania sunspot group 
55
(NOAA AR 2680).
The particle event, associated with the X8.2 flare is still on going, but

the level of the proton fluxes is decreasing, and presently only fluxes

with >10 MeV are slightly above the event threshold.

The sudden jump of the solar wind speed (up to maximum value of 650 km/s)

and simultaneous increase of the density and interplanetary magnetic field

magnitude (up to 16 nT) observed at about 19:26 UT on September 12
indicated arrival of the decayed CME-driven shock wave associated with 
the
X8.2 flare observed on September 10. The shock was followed by the post-

shock sheath region. The solar wind speed decreased rather fast and it 
is
presently about 460 km/s.The interplanetary magnetic field magnitude is

about 5 nT.
The longer intervals of the southward Bz component and fast solar wind

induced minor geomagnetic storm conditions starting at about 21:00 UT on

September 12 and lasting until about 03 UT on September 13 (local station

at Dourbes reported K=5 and NOAA reported Kp=5).
The fast solar wind, associated with the low latitude coronal hole in the

northern hemisphere which reached the central meridian on September 10, 
is
expected to arrive at the Earth today. We expect quiet to active conditions

within next 24 hours due to arrival of the fast solar wind.

TODAY'S ESTIMATED ISN  : 018, BASED ON 19 STATIONS.
99999
UGEOI 30512 70913 1230/ 12/// 
10012 20761 3019/ 4//// 80101 90060 
99999

NOTICEABLE EVENTS SUMMARY
DAY BEGIN MAX  END  LOC    XRAY OP  10CM Catania/NOAA RADIO_BURST_TYPES 

NONE
END

UGEOR 30512 70913 1230/ 13/07 13101 
10055 2//// 3//// 472// 50060 60002 13510 02000 
99999
USSPS 31405 13076 01242 55006 13510 2/902
USSPS 32404 11060 02322 68006 47916 2/802 75007 16510 2/801
USSPS 21305 11144 02432 75014 15908 2/801 69005 47717 0/103
USSPS 81202 12022 01132 69013 15209 2/801
UMAGF 30503 70913 1004/ 12063 1/031 22122 34542
UMAGF 31523 70913 0000/ 12003 1/019 22222 33355

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

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# Royal Observatory of Belgium                                       #

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