[ips-sf] IPS Summary Forecast for 18 June - issued 2333UT/17-Jun-2013
rwc
rwc at ips.gov.au
Tue Jun 18 09:33:20 EST 2013
A large group of sunspots is located in the south east quadrant of the
Sun. This group produced four C class solar X-ray flares during the UT
day of June 17. The largest sunspot (Active Region 1775) is growing in
complexity and may produce an M class flare in comming days. There is
a small chance it will produce an X class flare. A large coronal hole
is located in the northern hemisphere and will rotate into a
geoeffective position in comming days. Spacecraft observations show
multiple Coronal Mass Ejections (CMEs) leaving the Sun throughout June
16-17, including a partial halo event towards the east, west and
south. The solar wind speed and density were very light today and they
are expected to increase late today and tomorrow. Geomagnetic
conditions may become unsettled late today and tomorrow. High
frequency radio communication may be slightly above predicted values
due to increasing solar EUV flux.
IPS Radio and Space Services email: asfc at ips.gov.au
PO Box 1386 WWW: http://www.ips.gov.au
Haymarket NSW 1240 AUSTRALIA FTP: ftp://ftp.ips.gov.au
tel: +61 2 9213 8010 fax: +61 2 9213 8060
IMPORTANT: This e-mail, including any attachments, may contain,
confidential or copyright information. The views expressed in
this message are those of the individual sender, unless
specifically stated to be the views of IPS. If you are not
the intended recipient, please contact the sender immediately
and delete all copies of this e-mail and attachments.
To unsubscribe from an IPS mail list either send an email to
"MAIL_LIST"-leave at ips.gov.au or go to
http://listserver.ips.gov.au/mailman/listinfo/"MAIL_LIST".
Information about training can be obtained from
http://listserver.ips.gov.au/mailman/listinfo/ips-training.
General information is available from
http://listserver.ips.gov.au/mailman/listinfo/ips-info.
More information about the ips-sf
mailing list