[Ips-wgr] IPS Weekly Geo. Report (01 May 14) issued 0234 UT on 01 May 2014

rwc rwc at ips.gov.au
Thu May 1 12:34:51 EST 2014


SUBJ: IPS WEEKLY GEOPHYSICAL REPORT 
ISSUED ON 01 MAY 2014, BY IPS RADIO AND SPACE SERVICES,
FROM THE AUSTRALIAN SPACE FORECAST CENTRE

1. SUMMARY (22 APRIL - 30 APRIL)
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               
 22 Apr   2211 0101    3  
 23 Apr   1111 2222    5  
 24 Apr   2222 1222    6  
 25 Apr   3201 2331    8  
 26 Apr   1211 1111    3  
 27 Apr   1000 0001    0  
 28 Apr   2112 1001    3  
 29 Apr   1000 1013    3  
 30 Apr   2233 3341   13  

*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.


Quiet to unsettled conditions.

2. FORECAST (01 MAY - 31 MAY)
Disturbed Periods: 
No strong recurrent patterns, however mild activity may be experienced on:
 4 May,  8-9 May,  14 May,  16-18 May,  21-23 May,  25 May.

Best Quiet Periods: 
 1-3 May,  5-7 May,  10-13 May,  15 May,  19-20 May,  24 May,  26-27 May.

3. FORECAST FOR HIGH RESOLUTION AEROMAGNETIC SURVEYS
Northern Australian Regions:
 Disturbed Periods: None.
 Best Quiet Periods: 1-27 May.

Central Australian Regions:
 Mildly Disturbed Periods: 17-18 May
 Best Quiet Periods: 1-16 May,  19-27 May.

Southern Australian Regions:
 Disturbed Periods: 17-18 May.
 Best Quiet Periods: 1-15 May,  20-27 May.


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
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 

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