[Ips-dsgr] IPS Daily Report - 04 June 06
rwc
rwc at ips.gov.au
Mon Jun 5 09:35:29 EST 2006
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 04/2330Z JUNE 2006 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 04 JUNE AND FORECAST FOR 05 JUNE - 07 JUNE
STATUS INDICATORS SOL:GREEN MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 04 Jun: Very low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 04 Jun: 76/14
1B. SOLAR FORECAST
05 Jun 06 Jun 07 Jun
Activity Low Very low Very low
Fadeouts None expected None expected None expected
10.7cm/SSN 80/20 80/20 80/20
COMMENT: Increased solar wind speed from the coronal hole had
less effect over the weekend than expected. This is possibly
due to the dipole tilt of the magnetic axis at solstice reducing
coupling of the magnetic field to the solar wind. The solar wind
speed declined over the UT day from ~480km/sec to 380km/sec.
IMF Bz has been mostly northwards so reconnection is not occurring
with the geomagnetic field. B class flare activity observed from
new AR892 and it has th epossibility for a C-class flare. Another
recurrent coronal hole is expected to take effect about 7th June.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 04 Jun: Quiet
Estimated Indices 04 Jun : A K
Australian Region 2 11101101
Darwin 2 11111001
Learmonth 0 10100000
Culgoora 1 01100001
Camden 5 21112221
Canberra 0 00100000
Hobart 0 00100100
Casey(Ant) 4 22111111
Observed Regional daily pc3 Indices 04 Jun :
Canberra 4 (Quiet)
Learmonth 0 (Quiet)
Culgoora 2 (Quiet)
Hobart 6 (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 04 Jun : A
Fredericksburg 2
Planetary 3
Observed AFr/Ap Indices 03 Jun : A K
Fredericksburg 2
Planetary 4 1110 1111
2B. MAGNETIC FORECAST
Date Ap Conditions
05 Jun 6 Quiet
06 Jun 6 Quiet
07 Jun 15 Unsettled to Active
COMMENT: Another recurrent coronal hole is expected to become
geoeffective about 7 June. Solar wind speed has decreased to
380km/sec. Geomagnetic field activity over the weekend, during
the period of coronal hole high speeds, was weaker than expected.
This may be due to the magnetic field axis tilt at solstices
causing weak coupling to the solar wind, possibly also reducing
the effect of the next coronal hole. IMF Bz has been northwards
over the UT day so no merging with the geomagnetic field which
is currently very quiet.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
04 Jun Normal Normal Fair-normal
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
05 Jun Normal Normal Normal
06 Jun Normal Normal Normal
07 Jun Normal Normal Normal-Fair
COMMENT: Conditions are generally normal and recovering from
the less than expected effect of the solar coronal hole. Another
coronal hole high speed solar wind stream is expected to take
effect ~7 June.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
04 Jun 18
Observed Australian Regional MUFs
near predicted monthly values
Predicted Monthly T index for June: 15
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
05 Jun 18 Near predicted monthly values
06 Jun 20 near predicted monthly values
07 Jun 20 about 10% below predicted monthly values
COMMENT: The T index is trending downwards from the effect of
the recent coronal hole but perhaps not as much as expected.
Spread F is still occurring at tropical stations although conditions
generally look normal.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 03 Jun
Daily Proton Fluence >1 MeV: 1.4E+05
Daily Proton Fluence >10 MeV: 1.6E+04
Daily Electron Fluence >2 MeV: 1.30E+06 (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 0%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
X-ray background: A4.4
ACE Satellite Solar Wind Day Averaged Data for 03 Jun
Speed: NA km/sec Density: NA p/cc Temp: NA K Bz: NA nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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