[Ips-wgr] IPS Weekly Geo. Report (02 February 12) issued 0211 UT on 02 Feb 2012
rwc
rwc at ips.gov.au
Thu Feb 2 13:11:34 EST 2012
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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