[Ips-dsgr] IPS Daily Report - 05 January 05
rwc
rwc at ips.gov.au
Thu Jan 6 11:02:55 EST 2005
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 05/2330Z JANUARY 2005 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 05 JANUARY AND FORECAST FOR 06 JANUARY - 08 JANUARY
STATUS INDICATORS SOL:GREEN MAG:** YELLOW ** ION: GREEN
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1A. SOLAR SUMMARY
Activity 05 Jan: Very low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 05 Jan: 88/32
1B. SOLAR FORECAST
06 Jan 07 Jan 08 Jan
Activity Very low Very low Very low
Fadeouts None expected None expected None expected
10.7cm/SSN 85/27 85/27 85/27
COMMENT: Solar activity was Very Low over the last 24 hours with
only minor B class events. A large north east positioned filament
dissapeared, and from LASCO imagery was the cause of a westward
non earth directed CME. The north-south component of the interplanetary
magnetic field, Bz fluctuated between +/-5nT for the entire UT
day. Continued elevated solar wind conditions (from the coronal
hole wind stream) were observed for most of the UT day, but began
to decline, with the solar wind velocity dropping from 700km/s
to be almost 550km/s at the time of this report.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 05 Jan: Quiet to Active
Estimated Indices 05 Jan : A K
Australian Region 12 3233 3322
Darwin 12 3233 3323
Learmonth 14 3234 3322
Culgoora 12 3233 3322
Canberra 14 3243 3322
Hobart 13 3243 3312
Casey(Ant) 18 4--4 3322
Observed Regional daily pc3 Indices 05 Jan :
Townsville NA
Learmonth 111 (Major storm)
Culgoora 17 (Quiet)
Canberra 47 (Unsettled)
Hobart 43 (Unsettled)
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 05 Jan : A
Fredericksburg 20
Planetary 22
Observed AFr/Ap Indices 04 Jan : A K
Fredericksburg 16
Planetary 23 4434 4433
2B. MAGNETIC FORECAST
Date Ap Conditions
06 Jan 16 active
07 Jan 16 active
08 Jan 16 active
COMMENT: Active periods are expected over the next 2 days due
to both coronal hole wind stream, weak coronal mass ejection
induced activity and possible glancing effects of a dissappearing
filament.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
05 Jan Normal Normal Normal
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
06 Jan Normal Normal-Fair Fair
07 Jan Normal Normal-Fair Fair
08 Jan Normal Normal-Fair Fair
COMMENT: Mild degradation periods possible for the next 2 days
over mid to high latitudes, otherwise conditons are expected
to be normal.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
05 Jan 45
Observed Australian Regional MUFs
Equatorial PNG Region:
Enhanced by 20% during local day,
Near predicted monthly values during local night.
Northern Australian Region:
Enhanced by 15% during local day,
Near predicted monthly values during local night.
Southern Australian and New Zealand Region:
Near predicted monthly values during local day,
Enhanced by 20% during local night.
Antarctic Region (Casey/Scott Base):
Near predicted monthly values over the UT day.
Predicted Monthly T index for January: 33
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
06 Jan 40 near predicted monthly values
07 Jan 40 near predicted monthly values
08 Jan 45 near predicted monthly values
COMMENT: Normal conditons expected for the next few days, with
the chance of isolated peiods of degradation for Southern AUS/NZ
regions.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 04 Jan
Daily Proton Fluence >1 MeV: 4.8E+06
Daily Proton Fluence >10 MeV: 1.1E+04
Daily Electron Fluence >2 MeV: 5.30E+08 (high fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability:24%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
X-ray background: A8.3
ACE Satellite Solar Wind Day Averaged Data for 04 Jan
Speed: 714 km/sec Density: 1.9 p/cc Temp: 285000 K Bz: 0 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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