[Ips-dsgr] IPS Daily Report - 10 May 04
rwc
rwc at ips.gov.au
Tue May 11 09:41:35 EST 2004
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 10/2330Z MAY 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 10 MAY AND FORECAST FOR 11 MAY - 13 MAY
STATUS INDICATORS SOL:GREEN MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 10 May: Very low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 10 May: 93/38
1B. SOLAR FORECAST
11 May 12 May 13 May
Activity Very low Very low Very low
Fadeouts None expected None expected None expected
10.7cm/SSN 95/41 90/34 90/34
COMMENT: The solar activity has been very low today.
Only a few B-class flares were recorded- the largest
flare being a B4.4 at 0926UT from region 606(S09E39).
Solar wind speed decreased from 420 km/s to 390 km/s
(approx.) by 2000UT and then increased to 420 km/s
(approx.) by the time of this report. The north-south
component of the interplanetary magnetic field (Bz)
showed minor fluctuations on both sides of the normal
value throughout the UT day. The solar activity is
expected to remain very low during the next few days.
Slight strengthening in the solar wind stream is
possible on 13 May due to a disappearing filament from
the area of region 606 observed on 10 May.
A possible weak shock was observed in the solar wind at
2200UT on 10 May.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 10 May: Quiet
Estimated Indices 10 May : A K
Australian Region 4 1211 1122
Darwin 3 1111 0122
Townsville 3 1111 1112
Learmonth 4 2210 1121
Culgoora 2 1100 1112
Canberra 3 1210 1122
Hobart 3 1111 1112
Casey(Ant) 7 3321 1122
Observed Regional daily pc3 Indices 10 MAY :
Townsville 8 (Quiet)
Learmonth 0 (Quiet)
Culgoora 0 (Quiet)
Canberra 18 (Quiet)
Hobart 12 (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.
Estimated AFr/Ap Indices 10 May : A
Fredericksburg 6
Planetary 5
Observed AFr/Ap Indices 09 May : A K
Fredericksburg 7
Planetary 6 2321 2321
2B. MAGNETIC FORECAST
Date Ap Conditions
11 May 6 Quiet
12 May 6 Quiet
13 May 10 Mostly quiet. Isolated unsettled periods possible.
COMMENT: Generally quiet geomagnetic conditions are expected
for the next few days. However, isolated unsettled conditions
are possible on 13 May.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
10 May Normal-fair Normal-fair Normal-poor
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
11 May Normal Normal Normal
12 May Normal Normal Normal
13 May Normal Normal Normal-Fair
COMMENT: HF conditions are expected to remain mostly normal
during the next two days. Minor degradations in HF conditions
are possible at high latitudes on 13 May.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
10 May 34
Observed Australian Regional MUFs
Equatorial PNG Region:
Near predicted monthly values during local day,
Depressed by 20% during local night.
Northern Australian Region:
Near predicted monthly values.
Southern Australian and New Zealand Region:
Near predicted monthly values.
Antarctic Region (Casey/Scott Base):
Near predicted monthly values over the UT day
with periods of depressions and degradations.
Predicted Monthly T index for May: 43
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
11 May 42 Near predicted monthly values
12 May 42 Near predicted monthly values
13 May 40 near predicted monthly values/depressed by about
5%.
COMMENT: HF conditions are expected to remain mostly normal
during the next two days. However, minor depressions in MUFs
are possible in Southern Aus/NZ regions on 13 May.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 09 May
Daily Proton Fluence >1 MeV: 2.4E+05
Daily Proton Fluence >10 MeV: 1.4E+04
Daily Electron Fluence >2 MeV: 1.90E+08 (moderate)
X-ray background: B1.0
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 09 May
Speed: 448 km/sec Density: 2.2 p/cc Temp: 98000 K Bz: 1 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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