[Ips-wgr] IPS Weekly Geo. Report (14 June 12) issued 0347 UT on 14 Jun 2012

rwc rwc at ips.gov.au
Thu Jun 14 13:47:18 EST 2012


SUBJ: IPS WEEKLY GEOPHYSICAL REPORT 
ISSUED ON 14 JUNE 2012, BY IPS RADIO AND SPACE SERVICES,
FROM THE AUSTRALIAN SPACE FORECAST CENTRE

1. SUMMARY (05 JUNE - 13 JUNE)
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               
 05 Jun   2432 4323   15  
 06 Jun   3323 3232   12  In the IPS magnetometer data for 06 
                          Jun, a weak (18nT) impulse was observed 
                          at 1150UT.
 07 Jun   2212 1221    5  
 08 Jun   1233 1011    6  
 09 Jun   2212 1121    5  
 10 Jun   1111 1112    3  
 11 Jun   2232 2233   10  
 12 Jun   3211 1111    5  
 13 Jun   2222 0001    3  

*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.


Quiet to unsettled conditions.

2. FORECAST (14 JUNE - 14 JULY)
Disturbed Periods: 
19-20 Jun,  1-5 Jul.

Best Quiet Periods: 
 14-17 Jun,  21-28 Jun,  6-14 Jul.

3. FORECAST FOR HIGH RESOLUTION AEROMAGNETIC SURVEYS
Northern Australian Regions: 
Disturbed Periods: None.
 Best Quiet Periods: 14-17 Jun,  21-28 Jun, 6-14 Jul.

Central Australian Regions:
 Disturbed Periods: Mildly disturbed on 16 Jun, 19-20 Jun, 1-5 Jul.
 Best Quiet Periods: 14-17 Jun,  21-28 Jun, 6-14 Jul.

Southern Australian Regions:
 Disturbed Periods: Mildly disturbed on 16 Jun, 19-20 Jun, 1-5 Jul.
 Best Quiet Periods: 14-17 Jun,  21-28 Jun, 6-14 Jul.


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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