[Ips-dsgr] IPS Daily Report - 04 October 09
rwc
rwc at ips.gov.au
Mon Oct 5 10:04:57 EST 2009
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 04/2330Z OCTOBER 2009 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 04 OCTOBER AND FORECAST FOR 05 OCTOBER - 07 OCTOBER
STATUS INDICATORS SOL:GREEN MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 04 Oct: Very low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 04 Oct: 71/6
1B. SOLAR FORECAST
05 Oct 06 Oct 07 Oct
Activity Very low Very low Very low
Fadeouts None expected None expected None expected
10.7cm/SSN 70/5 69/3 69/3
COMMENT: The solar wind speed ranged from 300 to 410 km/s and
is expected to remain in this range for the next three days.
A weak shock was observed in the solar wind at 0308UT on 04 Oct.
The solar disc is spotless at this time.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 04 Oct: Quiet to Unsettled
Estimated Indices 04 Oct : A K
Australian Region 7 13132112
Darwin 7 13132112
Townsville 8 23232122
Learmonth 6 13132201
Canberra 5 03132001
Hobart 6 13131112
Observed Regional daily pc3 Indices 04 Oct :
Darwin 2 (Quiet)
Townsville 0 (Quiet)
Learmonth 0 (Quiet)
Alice_Springs 0 (Quiet)
Gnangara 0 (Quiet)
Canberra 0 (Quiet)
Hobart 0 (Quiet)
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.
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.
Estimated AFr/Ap Indices 04 Oct : A
Fredericksburg 3
Planetary 5
Observed AFr/Ap Indices 03 Oct : A K
Fredericksburg 1
Planetary 1 0000 1001
2B. MAGNETIC FORECAST
Date Ap Conditions
05 Oct 2 Quiet
06 Oct 2 Quiet
07 Oct 2 Quiet
COMMENT: Due to an increase in the solar wind speed there was
quiet to unsettled conditions in the Australian region and quiet
to active conditions in the Antarctic region. Expect quiet conditions
for the next three days.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
04 Oct Normal Normal Normal-fair
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
05 Oct Normal Normal Normal
06 Oct Normal Normal Normal
07 Oct Normal Normal Normal
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
04 Oct -6
Observed Australian Regional MUFs
Equatorial PNG/Niue Region:
Near predicted monthly values during local day,
Depressed by 25% during local night.
Northern Australian Region:
Depressed by 10% during local day,
Near predicted monthly values during local night.
Southern Australian and New Zealand Region:
Near predicted monthly values during local day,
Enhanced by 25% during local night.
Antarctic Region (Casey/Scott Base/Davis/Mawson):
Near predicted monthly values over the UT day.
Predicted Monthly T index for October: 1
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
05 Oct 1 near predicted monthly values
06 Oct 1 near predicted monthly values
07 Oct 1 Near predicted monthly values
COMMENT: Normal ionospheric support expected for all regions
over the next 24 hours with a possibilty of slight depressions
in the equitorial and north Australian regions. Similar conditions
expected for the next three days.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 03 Oct
Daily Proton Fluence >1 MeV: 6.2E+05
Daily Proton Fluence >10 MeV: 2.0E+04
Daily Electron Fluence >2 MeV: 5.40E+04 (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
X-ray background: A1.0
ACE Satellite Solar Wind Day Averaged Data for 03 Oct
Speed: 319 km/sec Density: 0.3 p/cc Temp: 12900 K Bz: 1 nT
(Courtesy Space Weather Prediction Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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