[Ips-dsgr] IPS Daily Report - 06 June 05
rwc
rwc at ips.gov.au
Tue Jun 7 09:42:22 EST 2005
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 06/2330Z JUNE 2005 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 06 JUNE AND FORECAST FOR 07 JUNE - 09 JUNE
STATUS INDICATORS SOL:GREEN MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 06 Jun: Low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 06 Jun: 106/55
1B. SOLAR FORECAST
07 Jun 08 Jun 09 Jun
Activity Low Low Low
Fadeouts None expected None expected None expected
10.7cm/SSN 110/60 110/60 110/60
COMMENT: Solar activity was low over the last 24 hours with only
C-class events from both regions 772 and 776. The largest event
was from region 772 with a C1.2 class flare at 1844UT. Solar
wind speed declined from 600km/s to be 450km/s at the tiome of
this report, indicating the end of the current coronal hole high
speed solar wind stream. The north-south component of the
interplanetary magnetic field (Bz), remained between +/-5nT.
Further C-class events are expected for the next few days with
the chance of isolated M-class events.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 06 Jun: Quiet to Unsettled
Estimated Indices 06 Jun : A K
Australian Region 7 3230 2022
Learmonth 6 2220 3022
Culgoora - ---- ----
Canberra 6 3230 2012
Hobart 6 3230 2012
Casey(Ant) 9 3331 2122
Observed Regional daily pc3 Indices 06 Jun :
Townsville NA
Learmonth NA
Culgoora NA
Canberra NA
Hobart NA
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 06 Jun : A
Fredericksburg 7
Planetary 10
Observed AFr/Ap Indices 05 Jun : A K
Fredericksburg 14
Planetary 20 4353 2333
2B. MAGNETIC FORECAST
Date Ap Conditions
07 Jun 12 Unsettled
08 Jun 8 Quiet to Unsettled
09 Jun 8 Quiet to Unsettled
COMMENT: Quiet to Unsettled conditions observed over the last
24 hours. With the drop in solar wind speed and the recent coronal
hole disappearing, predominently Quiet conditions are expected
with isolated Unsettled periods likely for the next 3 days.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
06 Jun Normal Normal Normal-fair
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
07 Jun Normal Normal Normal-Fair
08 Jun Normal Normal Normal-Fair
09 Jun Normal Normal Normal-Fair
COMMENT: Degraded HF conditions observed for high latitudes over
the last 24 hours. Good HF conditions for mid to low latitudes,
with improving conditions for high latitudes, are expected over
the next 2 days.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
06 Jun 38
Observed Australian Regional MUFs
Equatorial PNG Region:
Enhanced by 15% during local day,
Enhanced by 15% during local night.
Northern Australian Region:
Mostly near predicted monthly values,
Southern Australian and New Zealand Region:
Near predicted monthly values.
Antarctic Region (Casey/Scott Base):
Enhanced by 15% over the UT day.
Predicted Monthly T index for June: 26
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
07 Jun 35 near predicted monthly values
08 Jun 40 near predicted monthly values
09 Jun 40 near predicted monthly values
COMMENT: IPS HF Communications Warning 26 was issued on 5 June
and is current for interval 5-7 June. Southern Aus/NZ region
MUFs may experience some isolated depressed periods, but generally
good HF conditions are expected over all regions for the next
3 days.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 05 Jun
Daily Proton Fluence >1 MeV: 7.8E+05
Daily Proton Fluence >10 MeV: 1.7E+04
Daily Electron Fluence >2 MeV: 3.20E+07 (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 5%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
X-ray background: B2.7
ACE Satellite Solar Wind Day Averaged Data for 05 Jun
Speed: 605 km/sec Density: 1.8 p/cc Temp: 289000 K Bz: 1 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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