[Ips-dsgr] IPS Daily Report - 06 May 04
rwc
rwc at ips.gov.au
Fri May 7 09:59:53 EST 2004
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 06/2330Z MAY 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 06 MAY AND FORECAST FOR 07 MAY - 09 MAY
STATUS INDICATORS SOL:GREEN MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 06 May: Very low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 06 May: 86/29
1B. SOLAR FORECAST
07 May 08 May 09 May
Activity Very low Very low Very low
Fadeouts None expected None expected None expected
10.7cm/SSN 85/27 90/34 95/41
COMMENT: Solar regions currently visible show little sign of
significant activity for the next few days. Solar wind speeds
have declined during the past 24 hours from approximately 650km/s
down to 500km/s as a coronal rotates out of its geoeffective
position.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 06 May: Quiet
Estimated Indices 06 May : A K
Australian Region 6 2222 2122
Darwin 6 2222 2122
Townsville 6 2222 2122
Learmonth 7 222- ----
Culgoora 5 1222 2122
Canberra 5 1222 2122
Hobart 5 1222 2112
Casey(Ant) 13 3443 1122
Observed Regional daily pc3 Indices 06 MAY :
Townsville 2 (Quiet)
Learmonth 12 (Quiet)
Culgoora 76 (Active)
Canberra 79 (Active)
Hobart 73 (Active)
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 May : A
Fredericksburg 10
Planetary 10
Observed AFr/Ap Indices 05 May : A K
Fredericksburg 12
Planetary 13 2333 3333
2B. MAGNETIC FORECAST
Date Ap Conditions
07 May 12 Mostly quiet to unsettled with isolated active
peiods.
08 May 8 Quiet to Unsettled
09 May 6 Quiet
COMMENT: Solar wind speeds are abating as a coronal hole rotates
out of its geoeffective position. Geomagnetic activity is expected
to be mostly quiet to unsettled for the next few days with isolated
active periods possible for 7 May.
-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
06 May Normal Normal-fair Normal-fair
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
07 May Normal Normal Normal-Fair
08 May Normal Normal Normal-Fair
09 May Normal Normal Normal
COMMENT: HF conditions were mildly degraded at times for mid-high
latitudes for 6 May. Mostly normal conditions are expected for
the next few days with slight depressions again possible at times
for mid-high latitudes for 7 May.
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
06 May 46
Observed Australian Regional MUFs
Equatorial PNG Region:
Enhanced by 15% during local day,
Enhanced by 30% during local night.
Northern Australian Region:
Near predicted monthly values.
Southern Australian and New Zealand Region:
Depressed 10-20% at times during local day,
otherwise mostly near predicted monthly values.
Antarctic Region (Casey/Scott Base):
Depressed 10-20% at times to near predicted
monthly values.
Predicted Monthly T index for May: 43
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
07 May 45 depressed 5 to 10%/near predicted monthly values
08 May 50 Near predicted monthly values
09 May 55 Near predicted monthly values
COMMENT: HF conditions were mildly degraded at times for southern
regions for 6 May. Mostly normal conditions are expected for
the next few days with slight depressions again possible at times
for southern regions for 7 May.
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 05 May
Daily Proton Fluence >1 MeV: 2.9E+05
Daily Proton Fluence >10 MeV: 1.3E+04
Daily Electron Fluence >2 MeV: 5.40E+06 (normal)
X-ray background: A7.5
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 05 May
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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