[Ips-wgr] ASWFC Weekly Geo. Report (30 May 24) issued 0114 UT on 30 May 2024 [SEC=OFFICIAL]

ASWFC aswfc at bom.gov.au
Thu May 30 11:14:55 AEST 2024


SUBJ: ASWFC WEEKLY GEOPHYSICAL REPORT 
ISSUED ON 30 MAY 2024
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx

1. SUMMARY (21 MAY - 29 MAY)
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               
 21 May   2112 2211    5  
 22 May   1100 0011    1  
 23 May   1111 1122    4  
 24 May   2213 2101    5  
 25 May   1120 0111    2  
 26 May   1211 3220    5  
 27 May   1123 2001    4  
 28 May   2220 0001    3  
 29 May   1122 0111    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 International Center for Space Weather 
Science and Education, Japan.


A quiet week, with G0 conditions observed all week.

2. FORECAST (30 MAY - 29 JUNE)
Disturbed Periods: 
1 Jun,  9 Jun, and 12-13 Jun.

Best Quiet Periods: 
 4-8 Jun, 17-18 Jun,  21 Jun,  24 Jun.

3. FORECAST FOR HIGH RESOLUTION AEROMAGNETIC SURVEYS
Northern Australian Regions:
 Disturbed Periods: None.
 Best Quiet Periods: 30 May to 5 Jun,  10-25 Jun.

Central Australian Regions:
 Disturbed Periods: None.
 Best Quiet Periods: 30 May to 5 Jun,  10-25 Jun.

Southern Australian Regions:
 Disturbed Periods: 03-Jun
 Best Quiet Periods: 31 May to 2 Jun,  4-5 Jun,  10-25 Jun.


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:
Two flare active solar regions are currently in the eastern solar 
hemisphere of the Sun. There is an increasing risk of CME induced 
geomagnetic storm activity as these regions move into a move geoeffective 
solar longitude range as the week progresses if these two regions 
produce further CMEs.

Geomagnetic activity can frequently be determined by short timescale 
solar events that cannot be forecast a week in advance, particularly
at solar maximum.

Australian Space Weather Forecasting Centre
Bureau of Meteorology
ASWFC at bom.gov.au
www.bom.gov.au | www.sws.bom.gov.au



More information about the ips-wgr mailing list