[Ips-dsgr] IPS Daily Report - 11 October 05
rwc
rwc at ips.gov.au
Wed Oct 12 09:29:07 EST 2005
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 11/2330Z OCTOBER 2005 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 11 OCTOBER AND FORECAST FOR 12 OCTOBER - 14 OCTOBER
STATUS INDICATORS SOL:** YELLOW ** MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 11 Oct: Low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 11 Oct: 78/17
1B. SOLAR FORECAST
12 Oct 13 Oct 14 Oct
Activity Low Low Low to moderate
Fadeouts None expected None expected Possible
10.7cm/SSN 80/20 85/27 85/27
COMMENT: Solar activity was low over the previous UT day. Minor
flaring is currently occurring in newly numbered region 814 (S06W11)
which produced a C1.0 flare at 1720Z and a B3.5 at 2212Z. Background
solar X-ray flux remains at very low levels. Overall solar activity
is expected to continue at low levels over the next 24 hours,
with further minor flaring possible from region 814. The solar
wind velocity has dropped back to pre-coronal hole speeds as
the Earth moves out of the coronal hole wind stream and was just
below 450km/s at the time of this report.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 11 Oct: Quiet
Estimated Indices 11 Oct : A K
Australian Region 4 2111 2211
Darwin 4 2111 2212
Learmonth 4 2101 2221
Culgoora 4 2112 2111
Canberra 4 2101 3111
Hobart 3 2110 2111
Casey(Ant) 11 4-32 2222
Observed Regional daily pc3 Indices 11 Oct :
Townsville NA
Learmonth 0 (Quiet)
Culgoora 0 (Quiet)
Canberra 15 (Quiet)
Hobart 16 (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 11 Oct : A
Fredericksburg 5
Planetary 5
Observed AFr/Ap Indices 10 Oct : A K
Fredericksburg 7
Planetary 10 2333 2013
2B. MAGNETIC FORECAST
Date Ap Conditions
12 Oct 5 Quiet
13 Oct 5 Quiet
14 Oct 8 Quiet to Unsettled
COMMENT: The geomagnetic field was generally quiet over the previous
24 hours, except for the high latitudes which experienced active
periods in response to continuous high solar wind speeds and
occasional southward turnings of the IMF. As the Earth has now
moved out of the coronal hole wind stream this high latitude
activity is expected to settle back to quiet-unsettled levels.
Quiet geomagnetic conditions are expected to prevail at mid-low
latitudes for the next 24-48 hours.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
11 Oct Normal Normal Normal-fair
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
12 Oct Normal Normal Normal
13 Oct Normal Normal Normal
14 Oct Normal Normal Normal-Fair
COMMENT: HF conditions were near normal at mid and low latitudes
over the previous 24 hours, with isolated periods of degraded
HF at high latitudes in response to the unsettled geomagnetic
field. Expect HF conditions to be normal over the next 24-48
hours.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
11 Oct 22
Observed Australian Regional MUFs
near predicted monthly values
Predicted Monthly T index for October: 23
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
12 Oct 26 near predicted monthly values
13 Oct 28 near predicted monthly values
14 Oct 30 about 10% above predicted monthly values
COMMENT: The ionosphere in the Australian region was stable over
the past 24 hours. MUFs were near predicted monthly values. Expect
normal HF conditions to continue over the next 24-48 hours in
the Australian region.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 10 Oct
Daily Proton Fluence >1 MeV: 1.7E+06
Daily Proton Fluence >10 MeV: 1.3E+04
Daily Electron Fluence >2 MeV: 2.60E+08 (moderate fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability:17%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
X-ray background: A4.5
ACE Satellite Solar Wind Day Averaged Data for 10 Oct
Speed: 625 km/sec Density: 1.4 p/cc Temp: 247000 K Bz: 1 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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