[Ips-dsgr] IPS Daily Report - 05 July 04
rwc
rwc at ips.gov.au
Tue Jul 6 09:43:37 EST 2004
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 05/2330Z JULY 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 05 JULY AND FORECAST FOR 06 JULY - 08 JULY
STATUS INDICATORS SOL:GREEN MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 05 Jul: Very low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 05 Jul: 78/17
1B. SOLAR FORECAST
06 Jul 07 Jul 08 Jul
Activity Very low Very low Very low
Fadeouts None expected None expected None expected
10.7cm/SSN 76/14 78/17 80/20
COMMENT: Only minor flare activity observed in the past 24 hours,
mainly from region 639. A weak Type II radio sweep was observed
on the Culgoora Radiospectrograph at 2233UT.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 05 Jul: Quiet
Estimated Indices 05 Jul : A K
Australian Region 4 2111 1122
Darwin 4 2111 1122
Townsville 4 1211 1122
Learmonth 3 2101 1121
Culgoora 3 1101 1122
Canberra 3 1101 1121
Hobart 2 1101 1112
Casey(Ant) 6 3221 1122
Observed Regional daily pc3 Indices 05 JUL :
Townsville 0 (Quiet)
Learmonth 0 (Quiet)
Culgoora 11 (Quiet)
Canberra 31 (Quiet to unsettled)
Hobart 12 (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 05 Jul : A
Fredericksburg 5
Planetary 6
Observed AFr/Ap Indices 04 Jul : A K
Fredericksburg 4
Planetary 6 2222 1222
2B. MAGNETIC FORECAST
Date Ap Conditions
06 Jul 12 Unsettled
07 Jul 10 Quiet to Unsettled
08 Jul 10 Quiet to Unsettled
COMMENT: Geomagnetic conditions were predominantly quiet, with
isolated unsettled periods observed at high latitudes only. Solar
wind speed remains steady at around 420 km/s. The Bz component
of the interplanetary magnetic field has shown minor to moderate
polarity fluctuations about neutral. An equatorial coronal hole
may produce slightly elevated geomagnetic conditions over the
next three days.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
05 Jul Normal Normal Normal-fair
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
06 Jul Normal Normal Normal-Fair
07 Jul Normal Normal Normal-Fair
08 Jul Normal Normal Normal-Fair
COMMENT: Extended periods of disturbance observed at high latitudes
over the UT day. Mostly normal HF conditions expected for the
next three days at low to mid latitudes. Periods of disturbance
possible at high latitudes in association with geomagnetic activity.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
05 Jul 38
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.
Southern Australian and New Zealand Region:
Near predicted monthly values.
Antarctic Region (Casey/Scott Base):
Near predicted monthly values with extended periods of
disturbance.
Predicted Monthly T index for July: 39
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
06 Jul 35 Near predicted monthly values
07 Jul 35 Near predicted monthly values
08 Jul 40 Near predicted monthly values
COMMENT: Variable overnight enhancements observed equatorial
region, normalising before local dawn. Extended periods of spread-F
and disturbance observed Antarctic region. Mostly normal HF conditions
expected at low to mid latitudes for the next few days, with
variable conditions possible at low and high latitudes. Possible
evening spread-F conditions S Aus/NZ regions.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 04 Jul
Daily Proton Fluence >1 MeV: 1.6E+05
Daily Proton Fluence >10 MeV: 1.4E+04
Daily Electron Fluence >2 MeV: 1.00E+08 (normal)
X-ray background: A3.2
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 04 Jul
Speed: 420 km/sec Density: 2.8 p/cc Temp: 71800 K Bz: 1 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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