[Ips-dsgr] IPS Daily Report - 20 February 05
rwc
rwc at ips.gov.au
Mon Feb 21 10:41:08 EST 2005
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 20/2330Z FEBRUARY 2005 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 20 FEBRUARY AND FORECAST FOR 21 FEBRUARY - 23 FEBRUARY
STATUS INDICATORS SOL:GREEN MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 20 Feb: Very low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 20 Feb: 96/43
1B. SOLAR FORECAST
21 Feb 22 Feb 23 Feb
Activity Low Low Low
Fadeouts None expected None expected None expected
10.7cm/SSN 95/41 95/41 90/34
COMMENT: Solar activity was very low over the last 24 hours with
only B-class events observed. The solar wind speed declined from
a maximum of 520km/s at the beginning of the UT day to be 440km/s
at the time of this report. The north-south component of the
interplanetary magnetic field (Bz) was northward (5nT) for the
first half of the UT day, after which it was close to neutral
for the remainder. Solar activity is expected to remain at low
levels for the next 24 hours, with no increase in size or magnetic
complexity of any regions currently on disk.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 20 Feb: Quiet to Unsettled
Estimated Indices 20 Feb : A K
Australian Region 11 3322 2332
Darwin 12 3331 2332
Learmonth 10 3222 2332
Culgoora 8 2221 1332
Canberra 8 2221 2332
Hobart 8 2221 2332
Casey(Ant) 17 44-3 2332
Observed Regional daily pc3 Indices 20 Feb :
Townsville NA
Learmonth NA
Culgoora NA
Canberra NA
Hobart 2 (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 20 Feb : A
Fredericksburg 6
Planetary 10
Observed AFr/Ap Indices 19 Feb : A K
Fredericksburg 8
Planetary 14 1234 4332
2B. MAGNETIC FORECAST
Date Ap Conditions
21 Feb 10 Quiet to Unsettled
22 Feb 10 Quiet to Unsettled
23 Feb 9 Quiet to Unsettled
COMMENT: The geomagnetic activity is expected to range from Quiet
to Unsettled levels for the next 2 days. Slight chance of isolated
Active periods possible.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
20 Feb Normal-fair Normal-fair Normal
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
21 Feb Normal Normal Normal-Fair
22 Feb Normal Normal Normal-Fair
23 Feb Normal Normal Normal-Fair
COMMENT: HF conditions are expected to remain mostly normal over
all latitudes for the next two days. Mild depressed periods observed
for low-mid lattitudes over the UT day. Slight chance of minor
degradations, more so at high latitudes, are possible.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
20 Feb 26
Observed Australian Regional MUFs
Equatorial PNG Region:
Near predicted monthly values during local day,
Enhanced by 35% during local night.
Northern Australian Region:
Near predicted monthly values.
Southern Australian and New Zealand Region:
Depressed by 15% during local day,
Near predicted monthly values during local night.
Antarctic Region (Casey/Scott Base):
Near predicted monthly values over the UT day.
Predicted Monthly T index for February: 33
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
21 Feb 25 near predicted monthly values/depressed 5 to
10%
22 Feb 40 near predicted monthly values
23 Feb 55 near predicted monthly values
COMMENT: Chance of mild depressions possible during local day
for mid latitudes and Southern Aus/NZ regions. Otherwise normal
HF conditions are expected.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 19 Feb
Daily Proton Fluence >1 MeV: 1.6E+06
Daily Proton Fluence >10 MeV: 1.4E+04
Daily Electron Fluence >2 MeV: 3.40E+07 (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 5%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
X-ray background: B1.6
ACE Satellite Solar Wind Day Averaged Data for 19 Feb
Speed: 501 km/sec Density: 3.0 p/cc Temp: 138000 K Bz: -1 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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