[Ips-dsgr] IPS Daily Report - 04 October 03
rwc
rwc at ips.gov.au
Sun Oct 5 09:41:57 EST 2003
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 04/2330Z OCTOBER 2003 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:* YELLOW * ION: GREEN
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1A. SOLAR SUMMARY
Activity 04 Oct: Moderate
Flares Max Fadeout Freq. Sectors
M1/SF 1547UT possible lower South American/
Atlantic
Observed 10.7 cm flux/Equivalent Sunspot Number for 04 Oct: 119/71
1B. SOLAR FORECAST
05 Oct 06 Oct 07 Oct
Activity Low Low Low
Fadeouts None expected None expected None expected
10.7cm/SSN 120/72 115/66 115/66
COMMENT: Most of the observed flare activity over the UT day
was from region 471. A westward directed CME was observed in
LASCO C3 imagery at 1313UT. Region of origin was probably AR
464 which is now behind the west solar limb. There is a possibility
of C to M class activity again today from region 471.
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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 4 1122 2102
Darwin 0 1000 0001
Townsville 6 2122 3113
Learmonth 4 2122 2002
Canberra 3 1122 2002
Hobart 5 1132 2001
Casey(Ant) 9 ---3 22--
Observed Regional daily pc3 Indices 04 OCT :
Townsville 0 (Quiet)
Learmonth 4 (Quiet)
Canberra 59 (Unsettled)
Hobart 41 (Unsettled)
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.
Estimated AFr/Ap Indices 04 Oct : A
Fredericksburg 10
Planetary 10
Observed AFr/Ap Indices 03 Oct : A K
Fredericksburg 11
Planetary 16 3533 3332
2B. MAGNETIC FORECAST
Date Ap Conditions
05 Oct 10 Quiet to Unsettled
06 Oct 15 Unsettled to Active
07 Oct 18 active
COMMENT: Solar wind speed remained elevated at around 470 km/s,
declining to around 400 km/s late in the UT day. There was a
period of IMF fluctuation early in the UT day, resulting in isolated
active conditions at high latitudes. Otherwise IMF maintained
a mostly northward polarity resulting in unsettled conditions,
becoming quiet later in the UT day. Expect mostly quiet conditions
today, with a possibility of weak coronal hole wind stream effects
commencing on day two and strengthening on day three.
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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-Fair
06 Oct Normal Normal Normal-Fair
07 Oct Normal Normal-Fair Fair
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
04 Oct 91
Observed Australian Regional MUFs
Equatorial PNG Region:
Near predicted monthly values during local day,
Enhanced by 40% during local night.
Northern Australian Region:
Enhanced by 15-20% over the UT day.
Southern Australian and New Zealand Region:
Enhanced by 30-35% over the UT day.
Antarctic Region (Casey/Scott Base):
Near predicted monthly values over the UT day.
Predicted Monthly T index for October: 54
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
05 Oct 90 10 to 20% above predicted monthly values
06 Oct 90 10 to 20% above predicted monthly values
07 Oct 80 5 to 15% above predicted monthly values
COMMENT: Mild overnight spread-F conditions observed NZ region.
Occasional intense spread-F conditions observed overnight Antarctic
region. Expect normal to enhanced ionospheric propagation conditions
today. Possibile periods of degradation on days two and three
in association with increased geomagnetic activity, especially
at high latitudes.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 03 Oct
Daily Proton Fluence >1 MeV: 3.1E+05
Daily Proton Fluence >10 MeV: 1.2E+04
Daily Electron Fluence >2 MeV: 6.90E+06 (normal)
X-ray background: B4.0
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 03 Oct
Speed: 481 km/sec Density: 4.5 p/cc Temp: 179000 K Bz: 4 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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