[Ips-dsgr] IPS Daily Report - 02 September 03
rwc
rwc at ips.gov.au
Wed Sep 3 09:44:10 EST 2003
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 02/2330Z SEPTEMBER 2003 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 02 SEPTEMBER AND FORECAST FOR 03 SEPTEMBER - 05 SEPTEMBER
STATUS INDICATORS SOL:GREEN MAG:* YELLOW * ION: GREEN
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1A. SOLAR SUMMARY
Activity 02 Sep: Very low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 02 Sep: 106/55
1B. SOLAR FORECAST
03 Sep 04 Sep 05 Sep
Activity Very low Very low Low
Fadeouts None expected None expected None expected
10.7cm/SSN 115/66 125/78 130/84
COMMENT: No significant changes to visible active regions observed.
Isolated C-class activity is possible.
Previously M-flare(s) producing region 431 is due for return
to the south-east limb around 3 Sep.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 02 Sep: Quiet to Active
Estimated Indices 02 Sep : A K
Australian Region 11 3132 4223
Darwin 9 223- 3223
Townsville 9 2222 4223
Learmonth 10 3122 4223
Canberra 10 2122 4323
Hobart 8 2121 4223
Casey(Ant) 22 4-43 43--
Observed Regional daily pc3 Indices 02 SEP :
Townsville 0 (Quiet)
Learmonth 14 (Quiet)
Canberra 89 (Minor storm)
Hobart 107 (Major storm)
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 02 Sep : A
Fredericksburg 14
Planetary 15
Observed AFr/Ap Indices 01 Sep : A K
Fredericksburg 11
Planetary 14 2441 2333
2B. MAGNETIC FORECAST
Date Ap Conditions
03 Sep 18 active
04 Sep 25 active
05 Sep 25 active
COMMENT: Although solar wind speed has remained elevated above
500 km/s for most of the UT day, sustained northward polarity
of the interplanetary magnetic field Bz has resulted in mostly
unsettled geomagnetic conditions with isolated active periods.
Later in the UT day, Bz fluctuations increased in amplitude as
polarity trended towards neutral. A large north-polar extension
of the current coronal hole is moving into geoeffective position.
Solar wind parameters are expected to increase as this occurs,
with the possibility of active to minor storm geomagnetic conditions
over the next few days.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
02 Sep Normal Normal Normal-fair
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
03 Sep Normal Normal Normal-fair
04 Sep Normal Normal Fair-poor
05 Sep Normal Normal-fair Fair-poor
COMMENT: Possible degraded HF conditions during the next few
days in association with increased geomagnetic activity.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
02 Sep 82
Observed Australian Regional MUFs
Equatorial PNG Region:
Enhanced by 15% during local day,
Enhanced by 20-30% during local night.
Northern Australian Region:
Near predicted monthly values during local day,
Enhanced by 15% during local night and after
local dawn.
Southern Australian and New Zealand Region:
Enhanced by 15% during local day,
Enhanced by 20% during local night and after
local dawn.
Antarctic Region (Casey/Scott Base):
Near predicted monthly values with periods
of disturbance local night hours.
Predicted Monthly T index for September: 57
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
03 Sep 75 10 to 20% above predicted monthly values
04 Sep 65 near predicted monthly values
05 Sep 60 Near predicted monthly values
COMMENT: Generally good HF conditions at time of report issue.
Possible degradations later today and for the next few days due
to anticipated high speed coronal hole wind stream effects.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 01 Sep
Daily Proton Fluence >1 MeV: 4.3E+05
Daily Proton Fluence >10 MeV: 1.1E+04
Daily Electron Fluence >2 MeV: 3.00E+07 (normal)
X-ray background: B2.2
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 01 Sep
Speed: 434 km/sec Density: 2.6 p/cc Temp: 124000 K Bz: 4 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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