[Ips-dsgr] IPS Daily Report - 28 January 04
rwc
rwc at ips.gov.au
Thu Jan 29 10:07:17 EST 2004
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 28/2330Z JANUARY 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 28 JANUARY AND FORECAST FOR 29 JANUARY - 31 JANUARY
STATUS INDICATORS SOL:GREEN MAG:** YELLOW ** ION: **YELLOW**
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1A. SOLAR SUMMARY
Activity 28 Jan: Very low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 28 Jan: 89/33
1B. SOLAR FORECAST
29 Jan 30 Jan 31 Jan
Activity Very low Low Low
Fadeouts None expected None expected None expected
10.7cm/SSN 100/48 105/54 105/54
COMMENT: Solar region 536 is returning to the solar south-east
limb. This region though reasonably large produced no solar flares
on its previous transit. A coronal hole is visible near solar
central meridian. It appears that the Earth has entered the wind
stream from this hole early in the UT day on 28 Jan. Moderately
elevated solar wind speeds are expected from this hole over coming
days.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 28 Jan: Quiet to Active
Estimated Indices 28 Jan : A K
Australian Region 17 4333 4322
Darwin 14 4323 3323
Townsville 17 4333 4322
Learmonth 21 5333 4331
Culgoora 13 4323 3222
Canberra 17 4333 4322
Hobart 17 4333 4322
Casey(Ant) 27 6--4 3223
Observed Regional daily pc3 Indices 28 JAN :
Townsville 0 (Quiet)
Learmonth 14 (Quiet)
Culgoora NA
Canberra 96 (Minor storm)
Hobart 112 (Major storm)
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 28 Jan : A
Fredericksburg 15
Planetary 19
Observed AFr/Ap Indices 27 Jan : A K
Fredericksburg 13
Planetary 16 3423 3333
2B. MAGNETIC FORECAST
Date Ap Conditions
29 Jan 18 Unsettled to active, chance minor storm period.
30 Jan 18 Unsettled to active, chance minor storm period.
31 Jan 18 Unsettled to active, chance minor storm period.
COMMENT: 27 day recurrence suggests that active periods can be
expected over coming days. The recuurent pattern from this coronal
hole may be showing signs of weakening.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
28 Jan Normal Normal Fair
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
29 Jan Normal Normal-Fair Fair
30 Jan Normal Normal-Fair Fair
31 Jan Normal Normal-Fair Fair
COMMENT: Mild to moderate degradation in HF communications quality
expected at mid to high latitudes due to anticpated activity
induced by solar coronal hole.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
28 Jan 73
Observed Australian Regional MUFs
Equatorial PNG Region:
Near predicted monthly values during local day,
Enhanced by 30% during local night.
Northern Australian Region:
Near predicted monthly values during local day,
Enhanced by 30% 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: 56
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
29 Jan 70 near predicted monthly values/depressed 10 to 15%
30 Jan 50 depressed 10 to 15%/near predicted monthly values
31 Jan 45 depressed 10 to 15%/near predicted monthly values
COMMENT: Generally good HF conditions expected today. Mild to
moderate depressions may be experienced in southern Aus/NZ regions
over next few days due to anticipated moderate activity associated
with coronal hole high wind stream entry.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 27 Jan
Daily Proton Fluence >1 MeV: 8.3E+05
Daily Proton Fluence >10 MeV: 1.1E+04
Daily Electron Fluence >2 MeV: 5.90E+07 (normal)
X-ray background: B1.2
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 27 Jan
Speed: 485 km/sec Density: 9.7 p/cc Temp: 94400 K Bz: -1 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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