[Ips-dsgr] IPS Daily Report - 21 May 04
rwc
rwc at ips.gov.au
Sat May 22 09:36:07 EST 2004
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 21/2330Z MAY 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 21 MAY AND FORECAST FOR 22 MAY - 24 MAY
STATUS INDICATORS SOL:GREEN MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 21 May: Low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 21 May: 107/57
1B. SOLAR FORECAST
22 May 23 May 24 May
Activity Low Low Low
Fadeouts None expected None expected None expected
10.7cm/SSN 105/54 105/54 100/48
COMMENT: Only B to minor C-class flare activity observed over
the past 24 hours, mainly from region 618. There is a small equatorial
coronal hole in the western solar hemisphere producing a mildly
elevated solar wind stream.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 21 May: Quiet to Unsettled
Estimated Indices 21 May : A K
Australian Region 6 3221 1210
Darwin 7 3311 1221
Townsville 5 3211 1211
Learmonth 6 3221 1210
Culgoora 4 2211 1210
Canberra 6 3221 1210
Hobart 5 2221 1210
Casey(Ant) 11 4422 1211
Observed Regional daily pc3 Indices 21 MAY :
Townsville 12 (Quiet)
Learmonth 2 (Quiet)
Culgoora NA
Canberra 72 (Active)
Hobart 85 (Minor 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 21 May : A
Fredericksburg 12
Planetary 10
Observed AFr/Ap Indices 20 May : A K
Fredericksburg 11
Planetary 13 2235 2233
2B. MAGNETIC FORECAST
Date Ap Conditions
22 May 10 Quiet to Unsettled. Chance active periods.
23 May 8 Quiet to unsettled
24 May 8 Quiet to unsettled
COMMENT: Solar wind speed declined steadily over the UT day.
The Bz component of the IMF showed minor polarity fluctuations
over the UT day under the influence of a mild coronal hole wind
stream. There was a briedf period of active geomagnetic conditions
at high latitudes only early in the UT day. Geomagnetic conditions
should continue to decline today. Expect mostly quiet conditions
days two and three.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
21 May Normal Normal Normal-fair
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
22 May Normal Normal Normal-Fair
23 May Normal Normal Normal-Fair
24 May Normal Normal Normal-Fair
COMMENT: Normal HF conditions are expected for the next few days
with possible isolated degradations at mid to high latitudes
on day one.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
21 May 58
Observed Australian Regional MUFs
Equatorial PNG Region:
Mostly near predicted monthly values,
Enhanced by 30% after local dawn.
Northern Australian Region:
Mostly near predicted monthly values,
Enhanced by 25% after local dawn.
Southern Australian and New Zealand Region:
Near predicted monthly values.
Antarctic Region (Casey/Scott Base):
Near predicted monthly values to enhanced
over the UT day.
Predicted Monthly T index for May: 43
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
22 May 65 5 to 15% above predicted monthly values
23 May 70 10 to 20% above predicted monthly values
24 May 70 10 to 20% above predicted monthly values
COMMENT: Mild overnight spread-F observed S Aus region. Periods
of spread-F observed Antarctic region. The significant low latitude
enhancements of the preceding few days were not observed over
the past 24 hours. Mostly normal to good HF conditions are expected
over the next three days. Possible isolated degradations at mid
to high latitudes on day one in association with mild geomagnetic
disturbances.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 20 May
Daily Proton Fluence >1 MeV: 2.0E+05
Daily Proton Fluence >10 MeV: 1.3E+04
Daily Electron Fluence >2 MeV: 1.10E+06 (normal)
X-ray background: B2.1
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 20 May
Speed: 485 km/sec Density: 5.7 p/cc Temp: 229000 K Bz: 1 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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