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Summary and Forecasts 
Weekly Report

Last updated 02 Feb 2012 02:11 UT

B
SUBJ: IPS WEEKLY GEOPHYSICAL REPORT 
ISSUED ON 02 FEBRUARY 2012, BY IPS RADIO AND SPACE SERVICES,
FROM THE AUSTRALIAN SPACE FORECAST CENTRE

1. SUMMARY (24 JANUARY - 01 FEBRUARY)
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 Jan   3322 3543   18    A weak (38nT) impulse was observed in the IPS
magnetometer data at 1504UT on 24 Jan. 
 25 Jan   2343 3212   12     
 26 Jan   2222 2312    7    
 27 Jan   2222 2211    6    
 28 Jan   2221 2112    5    
 29 Jan   2212 0212    5    
 30 Jan   1111 1333    7    
 31 Jan   2221 1012    4    
 01 Feb   2332 2112    8    

*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 Space Environment Research Center, Japan.


active on 24 Jan.
quiet to unsettled on other days.

2. FORECAST (02 FEBRUARY - 03 MARCH)
Disturbed Periods: 
No strong recurrent patterns, however mild activity may be experienced on:
  4 Feb,   12 Feb,  18 Feb to 21 Feb.

Best Quiet Periods: 
 2 Feb to 3 Feb,  5 Feb to 11 Feb,  13 Feb to 17 Feb,  22 Feb to 28 Feb.

3. FORECAST FOR HIGH RESOLUTION AEROMAGNETIC SURVEYS

Northern Australian Regions:
 Disturbed Periods: None.
 Best Quiet Periods: 2 Feb to 28 Feb.

Central Australian Regions:
 Mildly Disturbed Periods: 21-23 Feb 
 Best Quiet Periods: 2 Feb to 19 Feb,  25 Feb to 28 Feb.

Southern Australian Regions:
 Disturbed Periods: 21-23 Feb
 Best Quiet Periods: 2 Feb to 19 Feb,  25 Feb to 28 Feb.

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.

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