[ips-sf] IPS Summary Forecast for 23 October - issued 2343UT/22-Oct-2012

rwc rwc at ips.gov.au
Tue Oct 23 10:43:23 EST 2012


There are currently numerous active sun spot regions on the visible
Sun. The high levels of ionising EUV flux produced by these regions is
resulting in a much denser than usual ionosphere. This is providing
good support for HF radio propagation with a significant increase in
the maximum useable frequency. An X-ray flare of M class magnitude
occurred at around 5am AEST on the 23rd of October. This did not
produce a coronal mass ejection (CME) however the flaring region on
the east limb of the Sun retains the potential for further flares and
will rotate into a more central position on the Sun over the next few
days. Isolated M class flares may occur over the next few days
potentially causing temporary disruption to HF communications.

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