[Ips-dsgr] IPS Daily Report - 18 May 04
rwc
rwc at ips.gov.au
Wed May 19 09:49:21 EST 2004
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 18/2330Z MAY 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 18 MAY AND FORECAST FOR 19 MAY - 21 MAY
STATUS INDICATORS SOL:GREEN MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 18 May: Low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 18 May: 108/58
1B. SOLAR FORECAST
19 May 20 May 21 May
Activity Low Low Low
Fadeouts None expected None expected None expected
10.7cm/SSN 105/54 105/54 100/48
COMMENT: Solar activity was low over the last 24 hours. Some
minor flare activity was observed, with region 612 the source
of a C2-class flare at 0200UT and region 615 the source of a
C3-class event at 0815UT and a C1-class flare at 1550UT. Region
609 has shown some decay over the past few days and was not active
over the last 24 hours. Further C-class events are expected for
the next few days with the possible chance of M-class. The solar
wind rose from 300km/s to 360km/s bewtween 0700UT and 1000UT
and then gradually fell to 320km/s at the time of this report.
Bz ranged between +/-5nT for the UT day with very few periods
where it was southwards.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 18 May: Quiet
Estimated Indices 18 May : A K
Australian Region 2 2111 1001
Darwin 3 1111 2101
Townsville 3 2112 2001
Learmonth 6 310- ----
Culgoora 6 310- ----
Canberra 1 1011 1001
Hobart 1 1011 1001
Casey(Ant) 2 2121 0001
Observed Regional daily pc3 Indices 18 MAY :
Townsville 13 (Quiet)
Learmonth 4 (Quiet)
Culgoora NA
Canberra 2 (Quiet)
Hobart 4 (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 18 May : A
Fredericksburg 6
Planetary 7
Observed AFr/Ap Indices 17 May : A K
Fredericksburg 3
Planetary 5 2101 2322
2B. MAGNETIC FORECAST
Date Ap Conditions
19 May 8 Quiet to Unsettled
20 May 10 Quiet to Unsettled
21 May 10 Quiet to Unsettled
COMMENT: Quiet conditions were observed over the last 24 hours.
Quiet to Unsettled conditions are expected for the next few days,
with the chance of possible isolated Active periods.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
18 May Normal Normal Normal
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
19 May Normal Normal Normal-Fair
20 May Normal Normal Normal-Fair
21 May Normal Normal Normal-Fair
COMMENT: Normal HF conditions are expected for the next few days
with possible degradations for 20-May. Minor degradations for
HF conditions at higher latitudes possible over the next few
days.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
18 May 54
Observed Australian Regional MUFs
Equatorial PNG Region:
Enhanced by 20% during local day,
Near predicted monthly values during local night.
Northern Australian Region:
Near predicted monthly values during local day,
Depressed by 15% during local night.
Southern Australian and New Zealand Region:
Near predicted monthly values.
Antarctic Region (Casey/Scott Base):
Enhanced by 50% over the UT day.
Predicted Monthly T index for May: 43
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
19 May 55 near predicted monthly values
20 May 50 near predicted monthly values
21 May 50 near predicted monthly values
COMMENT: Mostly normal to good HF conditions are expected over
the next 24 hours with similar conditions expected over the next
few days. Possible degradations at mid to high latitudes on 20-May.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 17 May
Daily Proton Fluence >1 MeV: 1.2E+05
Daily Proton Fluence >10 MeV: 1.4E+04
Daily Electron Fluence >2 MeV: 1.20E+06 (normal)
X-ray background: B2.3
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 17 May
Speed: 334 km/sec Density: 4.0 p/cc Temp: 47700 K Bz: 1 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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