[Ips-dsgr] IPS Daily Report - 17 February 04
rwc
rwc at ips.gov.au
Wed Feb 18 10:37:16 EST 2004
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 17/2330Z FEBRUARY 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 17 FEBRUARY AND FORECAST FOR 18 FEBRUARY - 20 FEBRUARY
STATUS INDICATORS SOL:GREEN MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 17 Feb: Very low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 17 Feb: 102/50
1B. SOLAR FORECAST
18 Feb 19 Feb 20 Feb
Activity Very low Very low Very low
Fadeouts None expected None expected None expected
10.7cm/SSN 100/48 100/48 95/41
COMMENT: Solar activity was very low today. Three B-class
flares were recorded- the largest being a B4.9 at 2006UT.
As expected, the solar wind stream weakened further with
the passage of the coronal hole from the geoeffective
position. The solar wind speed decreased from 550 km/s to
400km/s (approx.) over the UT day. The north-south component
of the interplanetary magnetic field (Bz) remained mildly
positive (upto approximately +5nT) for most part of the day.
Bz is currently close to the normal value. The solar activity
is expected to remain very low during the next three days.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 17 Feb: Quiet with isolated
unsettled periods recorded at some high latitude locations.
Estimated Indices 17 Feb : A K
Australian Region 2 0101 1212
Darwin 3 1101 1212
Townsville 1 0101 0202
Learmonth 1 0001 0212
Culgoora 1 0000 0202
Canberra 2 1101 0202
Hobart 2 0101 1202
Casey(Ant) 9 12-3 2322
Observed Regional daily pc3 Indices 17 FEB :
Townsville 0 (Quiet)
Learmonth 0 (Quiet)
Culgoora 0 (Quiet)
Canberra 6 (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 17 Feb : A
Fredericksburg 3
Planetary 7
Observed AFr/Ap Indices 16 Feb : A K
Fredericksburg 6
Planetary 7 3113 3221
2B. MAGNETIC FORECAST
Date Ap Conditions
18 Feb 8 Quiet
19 Feb 6 Quiet
20 Feb 6 Quiet
COMMENT: As expected, the geomagnetic activity has continued
to decline with the weakening of the solar wind stream. The
geomagnetic activity is expected to remain mostly at quiet
levels during the next 3 days.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
17 Feb Normal Normal Normal-poor
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
18 Feb Normal Normal Normal-Fair
19 Feb Normal Normal Normal
20 Feb Normal Normal Normal
COMMENT: HF conditions are expected to remain mostly normal
at most locations during the next 3 days. However there is
a slight chance of isolated minor degradations at some high
latitude locations on 18 February.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
17 Feb 68
Observed Australian Regional MUFs
Equatorial PNG Region:
Near predicted monthly values during local day,
Enhanced by 35% during local night.
Northern Australian Region:
Near predicted monthly values.
Southern Australian and New Zealand Region:
Mostly near predicted monthly values,
Depressed by 25% after local dawn.
Antarctic Region (Casey/Scott Base):
Near predicted monthly values over the UT day
with periods of depressions and degradations.
Predicted Monthly T index for February: 53
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
18 Feb 68 5 to 15% above predicted monthly values
19 Feb 70 5 to 20% above predicted monthly values
20 Feb 70 5 to 20% above predicted monthly values
COMMENT: HF conditions are expected to remain normal in
Aus/NZ regions during the next three days.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 16 Feb
Daily Proton Fluence >1 MeV: 1.2E+06
Daily Proton Fluence >10 MeV: 1.3E+04
Daily Electron Fluence >2 MeV: 1.30E+09 (very high)
X-ray background: A9.0
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 16 Feb
Speed: 547 km/sec Density: 0.3 p/cc Temp: 454000 K Bz: 1 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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