[Ips-dsgr] IPS Daily Report - 22 July 03
rwc
rwc at ips.gov.au
Wed Jul 23 09:45:40 EST 2003
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 22/2330Z JULY 2003 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 22 JULY AND FORECAST FOR 23 JULY - 25 JULY
STATUS INDICATORS SOL:GREEN MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 22 Jul: Low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 22 Jul: 153/108
1B. SOLAR FORECAST
23 Jul 24 Jul 25 Jul
Activity Low Low Low
Fadeouts Possible Possible Possible
10.7cm/SSN 150/105 145/99 135/89
COMMENT: Solar activity was low today. Several C-class
flares were recorded- the largest being a C5.2 flare at
0718UT from region 417(S21W64). The solar wind slowed
down further and remained between 420 km/s and 460 km/s
throughout the UT day. The N/S component of the
inter-planetary magnetic field remained mildly but
predominantly northwards. The solar activity is expected
to remain at low levels during the next 3 days. Region
417 showed further growth today whereas region 410(S13W53),
which is still the largest region on the disk, has further
simplified. There is slight chance of isolated M-flare
from region 417.
Previously M-flare(s) producing region 397 is due for return
to the north-east limb around 24 Jul.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 22 Jul: Mostly quiet with
isolated unsettled periods.
Estimated Indices 22 Jul : A K
Australian Region 5 2122 1122
Darwin 5 2122 1220
Townsville 4 1122 1122
Learmonth 4 2120 ---2
Canberra 5 1122 2223
Hobart 4 1112 1121
Casey(Ant) 9 2332 1131
Observed Regional daily pc3 Indices 22 JUL :
Townsville 0 (Quiet)
Learmonth 0 (Quiet)
Canberra 0 (Quiet)
Hobart 0 (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 22 Jul : A
Fredericksburg 10
Planetary 12
Observed AFr/Ap Indices 21 Jul : A K
Fredericksburg 8
Planetary 12 4421 2232
2B. MAGNETIC FORECAST
Date Ap Conditions
23 Jul 10 Mostly quiet. Isolated unsettled periods possible.
24 Jul 10 Mostly quiet.
25 Jul 8 Mostly quiet.
COMMENT: The coronal hole induced solar wind stream seems
to have further slowed down. The geomagnetic activity is
expected to gradually slow down to 'mostly quiet with
isolated unsettled periods' on day 1 and to 'mostly quiet'
levels thereafter.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
22 Jul Normal Normal Normal-fair
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
23 Jul Normal Normal Normal-fair
24 Jul Normal Normal Normal
25 Jul Normal Normal Normal
COMMENT: The HF conditions are expected to remain mostly
normal during the next three days.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
22 Jul 82
Observed Australian Regional MUFs
Equatorial PNG Region:
Enhanced by 25% during local day,
Enhanced by 15% during local night.
Northern Australian Region:
Near predicted monthly values.
Southern Australian and New Zealand Region:
Enhanced by 15% during local day,
Near predicted monthly values during local night.
Antarctic Region (Casey/Scott Base):
Near predicted monthly values over the UT day
with periods of degradations.
Predicted Monthly T index for July: 63
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
23 Jul 82 Near predicted monthly values/enhanced by 20%.
24 Jul 84 Near predicted monthly values/enhanced by 20%.
25 Jul 85 Near predicted monthly values/enhanced by 20%.
COMMENT: MUFs are expected to remain mostly normal in the
Australian/NZ regions during the next three days.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 21 Jul
Daily Proton Fluence >1 MeV: 3.9E+05
Daily Proton Fluence >10 MeV: 1.2E+04
Daily Electron Fluence >2 MeV: 7.10E+07 (normal)
X-ray background: B6.6
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 21 Jul
Speed: 474 km/sec Density: 1.4 p/cc Temp: 119000 K
Bz: 3 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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