| |
OK0NAG > SOLAR 22.02.18 13:34l 130 Lines 4278 Bytes #999 (0) @ EU
BID : M2SOK0NAG003
Read: GUEST
Subj: GEOALERT SIDC
Path: IW8PGT<IR2UBX<DB0RES<SR4BBX<SR8BBS<SR1BSZ<SR6BBA<OK0NAG
Sent: 180222/1230z @:OK0NAG.#BOH.CZE.EU [TCP/IP BBS Praha Strahov] bcm2.01e-zia
X-Info: Prijato od 127.0.0.1 za pomoci SMTP gatewaye
From: ok0nag <ok0nag>
Reply-to: no-reply-sidc@oma.be
To: solar@eu
Received-spf: Pass (sender SPF authorized) identity=mailfrom; client-ip=193.190.230.20; helo=smtp2.oma.be; envelope-from=no-reply-sidc@oma.be; receiver=solar@asu.cas.cz
Subject: GEOALERT SIDC
Date: Thu, 22 Feb 2018 12:30:17 GMT
X-clacks-overhead: GNU Terry Pratchett
X-spam-flag: NO
X-spam-score: -0.394
:Issued: 2018 Feb 22 1230 UTC
:Product: documentation at http://www.sidc.be/products/xut
#--------------------------------------------------------------------#
# GEOALERT message from the SIDC (RWC-Belgium) #
#--------------------------------------------------------------------#
GEOALERT BRU053
UGEOA 30512 80222 1230/ 9930/
10222 21222 30222
99999
PLAIN
NOTE: the above forecasts are valid from 1230UT, 22 Feb 2018 until 24 Feb
2018
PREDICTIONS FOR 22 Feb 2018 10CM FLUX: 068 / AP: 012
PREDICTIONS FOR 23 Feb 2018 10CM FLUX: 068 / AP: 012
PREDICTIONS FOR 24 Feb 2018 10CM FLUX: 068 / AP: 007
COMMENT: There are no sunspot regions on the visible hemisphere of the
Sun
and flaring level is very low. The chance for a C flare in the next 24
hours is estimated at 5%.
No Earth-directed Coronal Mass Ejections (CMEs) were observed in available
coronagraphic imagery.
The greater than 10 MeV proton flux was at nominal levels in the past 24
hours, and is expected to stay at nominal levels in the next 24 hours.
The solar wind speed (recorded by DSCOVR) varied between about 380 and
430
km/s in the past 24 hours, with current values around 405 km/s. The
Interplanetary Magnetic Field (IMF) was directed mainly toward the Sun
and
its magnitude ranged between about 1 and 10 nT. Bz had excursions below
-5
nT between 07:40 and 09:30 UT on February 22. On February 22, 23 and 24
the
solar wind is expected to be at nominal levels, possibly with occasional
periods of enhanced solar wind as the Earth comes close to the high speed
stream associated with the negative polarity south polar coronal hole.
Quiet geomagnetic conditions (K Dourbes between 1 and 2; NOAA Kp between
1
and 2) were registered in the past 24 hours. Quiet to unsettled geomagnetic
levels (K Dourbes < 4) are expected on February 22, 23 and 24, with a
chance for active intervals (K Dourbes = 4) when the Earth comes close
to
the high speed stream associated with the negative polarity south polar
coronal hole.
TODAY'S ESTIMATED ISN : 000, BASED ON 22 STATIONS.
99999
UGEOI 30512 80222 1230/ 21///
10000 20680 3003/ 4//// 80000 90000
99999
NOTICEABLE EVENTS SUMMARY
DAY BEGIN MAX END LOC XRAY OP 10CM Catania/NOAA RADIO_BURST_TYPES
NONE
END
UGEOR 30512 80222 1230/ ///// /////
99999
UMAGF 30503 80222 1004/ 21068 1/008 21211 31121
UMAGF 31523 80222 0000/ 21000 1/003 20012 31111
#--------------------------------------------------------------------#
# 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 #
# #
# For more information, see http://www.sidc.be. Please do not reply #
# directly to this message, but send comments and suggestions to #
# 'sidctech@oma.be'. If you are unable to use that address, use #
# 'rvdlinden@spd.aas.org' instead. #
# To unsubscribe, visit http://sidc.be/registration/unsub.php #
# #
# Legal notices: #
# - Intellectual Property Rights: #
# http://www.astro.oma.be/common/internet/en/data-policy-en.pdf #
# - Liability Disclaimer: #
# http://www.astro.oma.be/common/internet/en/disclaimer-en.pdf #
# - Use and processing of your personal information: #
# http://www.astro.oma.be/common/internet/en/privacy-policy-en.pdf #
#--------------------------------------------------------------------#
Read previous mail | Read next mail
| |
