[Ips-dsgr] IPS Daily Report - 04 February 10
rwc
rwc at ips.gov.au
Fri Feb 5 10:16:07 EST 2010
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 04/2330Z FEBRUARY 2010 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 04 FEBRUARY AND FORECAST FOR 05 FEBRUARY - 07 FEBRUARY
STATUS INDICATORS SOL:GREEN MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 04 Feb: Very low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 04 Feb: 74/11
1B. SOLAR FORECAST
05 Feb 06 Feb 07 Feb
Activity Very low Very low Very low
Fadeouts None expected None expected None expected
10.7cm/SSN 75/13 77/16 80/20
COMMENT: Solar Activity was Very Low over the UT day with no
significant solar flares. Similar conditions are expected 05
Feb. Active region 1043 (N26W33) remains stable. The solar wind
speed has dropped back below 400km/s and the IMF Bz component
is stable near 0nT. A coronal hole wind stream is expected late
06 Feb.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 04 Feb: Quiet
Estimated Indices 04 Feb : A K
Australian Region 4 21111112
Darwin 2 21100102
Townsville 5 22211112
Learmonth 2 21100111
Canberra 1 11000001
Hobart 3 12111111
Casey(Ant) 8 3-321113
Observed Regional daily pc3 Indices 04 Feb :
Darwin 0 (Quiet)
Townsville 0 (Quiet)
Learmonth 0 (Quiet)
Alice_Springs 0 (Quiet)
Gnangara 0 (Quiet)
Canberra 0 (Quiet)
Hobart 0 (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 and have been shown to be
well correlated with rejection of high resolution aeromagnetic
survey flight-line data.
NOTE: Indices may have been generated from data obtained in
cooperation with the following organisations: Geoscience Australia,
University of Newcastle Space Physics Group, Australian Government
Antarctic Division and Space Environment Research Center, Japan.
Estimated AFr/Ap Indices 04 Feb : A
Fredericksburg 2
Planetary 5
Observed AFr/Ap Indices 03 Feb : A K
Fredericksburg 7
Planetary 9 3133 3221
2B. MAGNETIC FORECAST
Date Ap Conditions
05 Feb 3 Quiet
06 Feb 8 Quiet to Unsettled
07 Feb 12 Unsettled
COMMENT: Geomagnetic activity was Quiet over the UT day. Expect
Quiet conditions today (05 Feb), becoming Unsettled with isolated
Active periods from late 06 Feb due to the arrival of a coronal
hole wind stream. Mostly Unsettled with a chance of isolated
Active periods 07 Feb with Minor Storm conditions likely at high
latitudes.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
04 Feb Normal-fair Normal Normal
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
05 Feb Normal Normal Normal
06 Feb Normal Normal Normal-Fair
07 Feb Normal Normal Normal-Fair
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
04 Feb 2
Observed Australian Regional MUFs
near predicted monthly values
Predicted Monthly T index for February: 4
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
05 Feb 0 Near predicted monthly values
06 Feb -2 Near predicted monthly values
07 Feb 5 Near predicted monthly values
COMMENT: Ionospheric conditions in the Australian region were
mostly normal over the UT day with MUFs near predicted monthly
values. The sustained intervals of blanketing sporadic E observed
over previous days were not evident in the last 24 hours. Expect
mostly normal HF conditions 05 Feb with MUFs mostly near predicted
monthly values. Some minor MUF depressions possible at S.Aus
and Antarctic locations.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 03 Feb
Daily Proton Fluence >1 MeV: 1.2E+06
Daily Proton Fluence >10 MeV: 1.9E+04
Daily Electron Fluence >2 MeV: 1.00E+07 (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 2%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
X-ray background: A3.2
ACE Satellite Solar Wind Day Averaged Data for 03 Feb
Speed: 528 km/sec Density: 2.2 p/cc Temp: 131000 K Bz: 0 nT
(Courtesy Space Weather Prediction Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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