[Ips-wgr] IPS Weekly Geo. Report (21 April 11)
rwc
rwc at ips.gov.au
Thu Apr 21 12:16:08 EST 2011
SUBJ: IPS WEEKLY GEOPHYSICAL REPORT
ISSUED ON 21 APRIL 2011, BY IPS RADIO AND SPACE SERVICES,
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
1. SUMMARY (12 APRIL - 20 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
12 Apr 2335 4322 17
13 Apr 2333 2111 8
14 Apr 2221 1011 4
15 Apr 2112 1111 4
16 Apr 2211 1101 3
17 Apr 1112 2211 4
18 Apr 1143 3312 11 A weak (13nT) impulse was observed in the IPS
magnetometer data at 0652UT on 18 Apr.
19 Apr 2211 1112 4
20 Apr 3432 2111 10
*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.
A coronal hole high speed wind stream caused Active conditions
on the 12th and Unsettled on the 13th. Conditions were then mostly
Quiet until a weak CME strike on the 18th and a new coronal hole
stream caused Unsettled conditions on the 18th and 20th.
2. FORECAST (21 APRIL - 21 MAY)
Disturbed Periods:
30th April- 5th May, 9th May - 10 May
Best Quiet Periods:
21 Apr to 27 Apr, 7 May, 12 May to 17 May.
3. FORECAST FOR HIGH RESOLUTION AEROMAGNETIC SURVEYS
Northern Australian Regions:
Disturbed Periods: None.
Best Quiet Periods: 21 Apr to 25 Apr.
Central Australian Regions:
Midly Disturbed Periods: 30th April to 5th May, 9th May to 10th May
Southern Australian Regions:
Disturbed Periods: 30th April to 5th May, 9th May to 10th May.
Best Quiet Periods: 21 Apr to 25 Apr.
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
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