[Ips-wgr] IPS Weekly Geo. Report (05 March 15) issued 0242 UT on 05 Mar 2015

rwc rwc at ips.gov.au
Thu Mar 5 13:42:04 EST 2015


SUBJ: IPS WEEKLY GEOPHYSICAL REPORT 
ISSUED ON 05 MARCH 2015, BY IPS RADIO AND SPACE SERVICES,
FROM THE AUSTRALIAN SPACE FORECAST CENTRE

1. SUMMARY (24 FEBRUARY - 04 MARCH)
K indices are in UT (0-24). For conversion to local time:

AEST = UT + 10 hours; ACST = UT + 9.5 hours; AWST = UT + 8 hours
        Australian Region*              
 Date     K-INDICES    A               
 24 Feb   3433 3223   14  
 25 Feb   1132 3221    7  
 26 Feb   2122 1012    4  
 27 Feb   1011 1202    3  
 28 Feb   1222 2333    9  
 01 Mar   3333 2223   12  
 02 Mar   2444 3322   16  
 03 Mar   2223 3122    8  
 04 Mar   1213 3012    6  

*estimated from real time data

NOTE: Indices may have been generated from data obtained in 
cooperation with the following organisations: Geoscience Australia, 
University of Newcastle Space Physics Group, Australian Government 
Antarctic Division and International Center for Space Weather 
Science and Education, Japan.

Active conditions on 24Feb, 01Mar-02Mar due to coronal hole effects.  
Quiet to Unsettled conditions expected for the next 7 days with only
minor coronal hole effects possible 7Mar.

2. FORECAST (05 MARCH - 04 APRIL)
Disturbed Periods: 28-29 Mar.

Best Quiet Periods:  8-15 Mar,  18-21 Mar,  24-26 Mar.

3. FORECAST FOR HIGH RESOLUTION AEROMAGNETIC SURVEYS
Northern Australian Regions: Quiet

Central Australian Regions:
 Mild Disturbed Periods: 28-29 Mar, possible 7Mar. 
 Best Quiet Periods: 5-23 Mar,  25-26 Mar,  30-31 Mar.

Southern Australian Regions:
 Disturbed Periods: 28-29 Mar, possible 7Mar.
 Best Quiet Periods: 5-22 Mar,  25-26 Mar,  30 Mar.


Pc3 pulsations are high frequency (10-45 second period) variations 
of the Earths magnetic field. Daily pc3-indices are the daily sum of 
20 minute pc3-indices for that station and have been shown to be well 
correlated with rejection of high resolution aeromagnetic survey 
flight-line data.

PLEASE NOTE:
Geomagnetic activity can frequently be determined by short timescale 
solar events that cannot be forecast a week in advance, particularly
at solar maximum.

IPS Radio and Space Services        email: asfc at ips.gov.au
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Haymarket NSW 1240  AUSTRALIA       FTP: ftp://ftp.ips.gov.au 
tel: +61 2 9213 8010                fax: +61 2 9213 8060 

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