[Ips-dsgr] IPS Daily Report - 23 October 05
rwc
rwc at ips.gov.au
Mon Oct 24 09:32:39 EST 2005
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 23/2330Z OCTOBER 2005 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 23 OCTOBER AND FORECAST FOR 24 OCTOBER - 26 OCTOBER
STATUS INDICATORS SOL:GREEN MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 23 Oct: Very low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 23 Oct: 74/11
1B. SOLAR FORECAST
24 Oct 25 Oct 26 Oct
Activity Very low Very low Low
Fadeouts None expected None expected None expected
10.7cm/SSN 75/13 75/13 75/13
COMMENT: Solar activity was very low over the last 24 hours with
no flare activity. Conditions are expected to remain like this
while there are no regions of considerable size or magnetic complexity
currently on disc. The solar wind velocity ranged between 360km/s
and 380km/s for the UT day. There is an expected increase in the solar
wind paramters due to the geoeffective coronal hole over the next
24 hours. The north south component of the interplanetary magnetic
field (Bz) fluctuated between neutral and 5nT throughout the UT day.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 23 Oct: Quiet
Estimated Indices 23 Oct : A K
Australian Region 3 2111 1111
Darwin 4 2111 1211
Learmonth - ---- ----
Culgoora 3 1111 1111
Canberra 3 1111 2111
Hobart 3 1111 1111
Casey(Ant) 7 33-2 1111
Observed Regional daily pc3 Indices 23 Oct :
Townsville NA
Learmonth 0 (Quiet)
Culgoora 0 (Quiet)
Canberra 24 (Quiet to unsettled)
Hobart 7 (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 23 Oct : A
Fredericksburg 7
Planetary 12
Observed AFr/Ap Indices 22 Oct : A K
Fredericksburg 7
Planetary 6 4210 1011
2B. MAGNETIC FORECAST
Date Ap Conditions
24 Oct 14 Unsettled to Active
25 Oct 14 Unsettled to Active
26 Oct 10 Quiet to Unsettled
COMMENT: Geomagnetic activity was Quiet over the last 24 hours.
Unsettled to Active conditions are expected over the next 2 days
due to anticipated elevated solar wind stream parameters from
a geoeffective coronal hole.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
23 Oct Normal Normal Normal
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
24 Oct Normal Normal Normal-Fair
25 Oct Normal Normal Normal-Fair
26 Oct Normal Normal Normal-Fair
COMMENT: Mostly normal conditions for HF Propagation are expected
for low to mid latitudes, with possible degradations for high
latitudes over the next 24 hours.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
23 Oct 21
Observed Australian Regional MUFs
Equatorial PNG Region:
Near predicted monthly values.
Northern Australian Region:
Mostly near predicted monthly values,
Southern Australian and New Zealand Region:
Mostly near predicted monthly values,
Antarctic Region (Casey/Scott Base):
Depressed by 15% over the UT day.
Predicted Monthly T index for October: 23
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
24 Oct 20 near predicted monthly values/depressed 5 to
10%
25 Oct 20 near predicted monthly values/depressed 5 to
10%
26 Oct 25 Near predicted monthly values
COMMENT: Mostly good HF conditions observed over all local regions
during the last 24 hours. Similar conditions are expected for
the next 2 days, with possible depressed periods for Southern
Aust. and NZ regions due to coronal hole effects.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 22 Oct
Daily Proton Fluence >1 MeV: 4.3E+05
Daily Proton Fluence >10 MeV: 1.4E+04
Daily Electron Fluence >2 MeV: 7.60E+05 (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 0%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
X-ray background: A1.0
ACE Satellite Solar Wind Day Averaged Data for 22 Oct
Speed: 395 km/sec Density: 5.5 p/cc Temp: 77500 K Bz: 2 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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