[Ips-dsgr] IPS Daily Report - 20 March 04
rwc
rwc at ips.gov.au
Sun Mar 21 10:31:27 EST 2004
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 20/2330Z MARCH 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 20 MARCH AND FORECAST FOR 21 MARCH - 23 MARCH
STATUS INDICATORS SOL:GREEN MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 20 Mar: Low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 20 Mar: 114/65
1B. SOLAR FORECAST
21 Mar 22 Mar 23 Mar
Activity Low Low Low
Fadeouts None expected None expected None expected
10.7cm/SSN 115/66 115/66 115/66
COMMENT: No significant flare activity was observed today. Possibility
of isolated C- to M-class activity from region 578.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 20 Mar: Quiet to Unsettled
Estimated Indices 20 Mar : A K
Australian Region 6 2211 2312
Darwin 5 2211 2213
Townsville 6 2221 2223
Learmonth 5 2211 2--2
Culgoora 5 2211 2212
Canberra 6 2211 2312
Hobart 6 2211 2312
Casey(Ant) 13 34-2 2322
Observed Regional daily pc3 Indices 20 MAR :
Townsville 6 (Quiet)
Learmonth 0 (Quiet)
Culgoora 6 (Quiet)
Canberra 19 (Quiet)
Hobart 25 (Quiet to 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 20 Mar : A
Fredericksburg 8
Planetary 10
Observed AFr/Ap Indices 19 Mar : A K
Fredericksburg 5
Planetary 6 2302 2222
2B. MAGNETIC FORECAST
Date Ap Conditions
21 Mar 12 Unsettled
22 Mar 8 Quiet to Unsettled
23 Mar 8 Quiet to Unsettled
COMMENT: Geomagnetic conditions have been mostly quiet to unsettled,
with isolated active intervals at high latitudes only. Solar
wind speed appears to have peaked at around 400 km/s. The north-south
component of the interplanetary magnetic field has been mostly
positively biased. There was a period of sustained negative bias
late in the UT day, possibily in association with a solar sector
boundary crossing. A brief period of active to storm levels was
observed at southern polar cusp latitude. Expect possible unsettled
intervals today, with conditions declining to quiet on days two
and three.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
20 Mar Normal Normal Normal-fair
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
21 Mar Normal Normal Normal-Fair
22 Mar Normal Normal Normal-Fair
23 Mar Normal Normal Normal-Fair
COMMENT: Generally good HF conditions expected. Mild degradations
possible on day one at high latitudes in association with anticipated
mild geomagnetic disturbance.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
20 Mar 74
Observed Australian Regional MUFs
Equatorial PNG Region:
Near predicted monthly values during local day,
Enhanced by 30% during local night.
Northern Australian Region:
Enhanced by 20% over the UT day.
Southern Australian and New Zealand Region:
Mostly near predicted monthly values,
Enhanced by 25% after local dawn.
Antarctic Region (Casey/Scott Base):
Generally above predicted monthly values,
with variable local disturbances.
Predicted Monthly T index for March: 49
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
21 Mar 75 10 to 20% above predicted monthly values
22 Mar 75 10 to 20% above predicted monthly values
23 Mar 75 10 to 20% above predicted monthly values
COMMENT: Evening spread-F observed S Aus/NZ regions. Generally
good HF conditions expected next three days. Expect localised
minor degradations at high latitudes. Mildly degraded HF communication
conditions may be experienced local night hours 21 Mar S Aus/NZ
regions.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 19 Mar
Daily Proton Fluence >1 MeV: 3.2E+05
Daily Proton Fluence >10 MeV: 1.3E+04
Daily Electron Fluence >2 MeV: 5.70E+07 (normal)
X-ray background: B4.2
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 19 Mar
Speed: 352 km/sec Density: 3.6 p/cc Temp: 51500 K Bz: 3 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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