[Ips-dsgr] IPS Daily Report - 07 February 05
rwc
rwc at ips.gov.au
Tue Feb 8 10:18:45 EST 2005
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 07/2330Z FEBRUARY 2005 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 07 FEBRUARY AND FORECAST FOR 08 FEBRUARY - 10 FEBRUARY
STATUS INDICATORS SOL:** YELLOW ** MAG:** YELLOW ** ION: ** YELLOW **
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1A. SOLAR SUMMARY
Activity 07 Feb: Low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 07 Feb: 103/52
1B. SOLAR FORECAST
08 Feb 09 Feb 10 Feb
Activity Low to moderate Low to moderate Low to moderate
Fadeouts Possible Possible Possible
10.7cm/SSN 110/60 115/66 115/66
COMMENT: Solar wind speed increased from 400 to 700km/sec over
the UT day, indicating the Earth has entered the anticipated
coronal hole wind stream. The north-south component of the interplanetary
magnetic field fluctuated southward over the UT day. Solar region
732 (the return of very active 720) has been mostly quiet over
the past 24 hours. Another solar region has rotated around the
south east limb (mentioned in yesterdays report). This region
has been numbered 733 by US SEC, and has produced some C class
events. Low to moderate activity may be experienced today.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 07 Feb: Quiet to Minor Storm
Estimated Indices 07 Feb : A K
Australian Region 20 3233 4352
Darwin 17 3233 4341
Learmonth 22 3223 5353
Culgoora 22 2233 535-
Canberra 22 2233 5353
Hobart 7 2--- ----
Casey(Ant) 37 4--5 336-
Observed Regional daily pc3 Indices 07 Feb :
Townsville NA
Learmonth NA
Culgoora NA
Canberra NA
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.
Estimated AFr/Ap Indices 07 Feb : A
Fredericksburg 15
Planetary 20
Observed AFr/Ap Indices 06 Feb : A K
Fredericksburg 6
Planetary 9 2241 1123
2B. MAGNETIC FORECAST
Date Ap Conditions
08 Feb 17 active
09 Feb 17 active
10 Feb 12 Unsettled
COMMENT: IPS Geomagnetic Warning 7 was issued on 7 February and
is current for interval 8-9 February. Active periods expected
next two days due to coronal hole wind stream induced geomagnetic
activity. Chance minor storm periods.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
07 Feb Normal Normal-fair Normal-fair
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
08 Feb Normal Normal-Fair Fair
09 Feb Normal Normal-Fair Fair
10 Feb Normal Normal Normal-Fair
COMMENT: Mid to high latitude HF communications mildly degraded
next two days.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
07 Feb 38
Observed Australian Regional MUFs
Equatorial PNG Region:
No data available during local day,
Enhanced by 45% during local night.
Northern Australian Region:
Mostly near predicted monthly values,
Depressed by 25% after local dawn.
Southern Australian and New Zealand Region:
Mostly near predicted monthly values,
Depressed by 30% after local dawn.
Antarctic Region (Casey/Scott Base):
Enhanced by 60% over the UT day.
Predicted Monthly T index for February: 33
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
08 Feb 5 depressed 10 to 20%/near predicted monthly values
09 Feb 5 depressed 10 to 15%/near predicted monthly values
10 Feb 20 Near predicted monthly values
COMMENT: IPS HF Communications Warning 10 was issued on 7 February
and is current for interval 8-9 February. Lower than normal MUFs
observed after local dawn this morning following cooronal hole
wind stream induced activity.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 06 Feb
Daily Proton Fluence >1 MeV: 1.5E+06
Daily Proton Fluence >10 MeV: 1.6E+04
Daily Electron Fluence >2 MeV: 1.50E+07 (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 3%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
X-ray background: B1.8
ACE Satellite Solar Wind Day Averaged Data for 06 Feb
Speed: 405 km/sec Density: 1.7 p/cc Temp: 98000 K Bz: 0 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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