[Ips-dsgr] IPS Daily Report - 29 March 04
rwc
rwc at ips.gov.au
Tue Mar 30 09:52:22 EST 2004
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 29/2330Z MARCH 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 29 MARCH AND FORECAST FOR 30 MARCH - 01 APRIL
STATUS INDICATORS SOL:** YELLOW ** MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 29 Mar: Low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 29 Mar: 129/82
1B. SOLAR FORECAST
30 Mar 31 Mar 01 Apr
Activity Low to moderate Low to moderate Low to moderate
Fadeouts Possible Possible Possible
10.7cm/SSN 130/84 130/84 135/89
COMMENT: M-class flare activity is possible from solar region
582. Solar wind speeds have continued to decline slowly over
the past 24 hours down to approximately 550km/s. The north-south
component of the IMF has been fluctuating between +5 to -5 nT.
This coronal hole solar wind stream is expected to continue to
abate over the next couple of days and geomagnetic activity should
be mostly quiet to unsettled levels.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 29 Mar: Quiet to Unsettled
Estimated Indices 29 Mar : A K
Australian Region 10 2232 3322
Darwin 9 2321 3322
Townsville 9 2222 3322
Learmonth 9 2222 3322
Culgoora 8 2221 3322
Canberra 9 1232 3322
Hobart 9 1232 3322
Casey(Ant) 21 -442 3442
Observed Regional daily pc3 Indices 29 MAR :
Townsville 4 (Quiet)
Learmonth 24 (Quiet to unsettled)
Culgoora 50 (Unsettled)
Canberra 88 (Minor storm)
Hobart 49 (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 29 Mar : A
Fredericksburg 12
Planetary 13
Observed AFr/Ap Indices 28 Mar : A K
Fredericksburg 12
Planetary 17 3533 3322
2B. MAGNETIC FORECAST
Date Ap Conditions
30 Mar 12 Quiet to unsettled with the chance of isolated
active periods.
31 Mar 8 Quiet to Unsettled
01 Apr 8 Quiet to unsettled
COMMENT: Isolated active periods have been observed over the
past 24 hours due to a persisting coronal hole solar wind stream.
Geomagnetic activity is expected to decline over the next couple
of days as solar wind speeds are anticipated to decrease.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
29 Mar Normal Normal Normal-fair
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
30 Mar Normal Normal Normal-Fair
31 Mar Normal Normal Normal-Fair
01 Apr Normal Normal Normal-Fair
COMMENT: Slightly degraded HF conditions are possible at times
at mid to high latitudes for 30 March due to recent coronal hole
induced geomagnetic activity, otherwise mostly good HF conditions
are expected.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
29 Mar 86
Observed Australian Regional MUFs
Equatorial PNG Region:
Enhanced by 35% during local day,
Enhanced by 50% during local night.
Northern Australian Region:
Enhanced by 20% during local day,
Enhanced by 30% during local night.
Southern Australian and New Zealand Region:
Enhanced by 25% during local day,
Enhanced by 30% during local night.
Antarctic Region (Casey/Scott Base):
Mostly near predicted monthly values to
depressed 10-20% at times.
Predicted Monthly T index for March: 49
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
30 Mar 75 Mostly enhanced 10-20% to depressed 5-10% at
times.
31 Mar 80 10 to 20% above predicted monthly values
01 Apr 80 10 to 20% above predicted monthly values
COMMENT: Slightly degraded HF conditions are possible at times
for southern Aus/NZ regions for 30 March due to recent coronal
hole induced geomagnetic activity, otherwise mostly good HF conditions
are expected.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 28 Mar
Daily Proton Fluence >1 MeV: 1.5E+06
Daily Proton Fluence >10 MeV: 1.3E+04
Daily Electron Fluence >2 MeV: 1.80E+08 (moderate)
X-ray background: B3.8
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 28 Mar
Speed: 792 km/sec Density: 0.9 p/cc Temp: 465000 K Bz: 0 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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