[Ips-dsgr] IPS Daily Report - 25 February 04
rwc
rwc at ips.gov.au
Thu Feb 26 10:29:13 EST 2004
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 25/2330Z FEBRUARY 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 25 FEBRUARY AND FORECAST FOR 26 FEBRUARY - 28 FEBRUARY
STATUS INDICATORS SOL:* YELLOW * MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 25 Feb: Low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 25 Feb: 119/71
1B. SOLAR FORECAST
26 Feb 27 Feb 28 Feb
Activity Low to moderate Low to moderate Low to moderate
Fadeouts Possible Possible Possible
10.7cm/SSN 115/66 115/66 115/66
COMMENT: Active region 564 produced a number of minor flares
over the UT day, including a C8 level flare at 1220 UT. Although
the flare was of moderate duration, no CME was observed in LASCO
imagery in association with this event. This region maintains
moderate magnetic complexity and has potential for further flare
activity. Radio noise and burst activity has been observed for
some hours on the Culgoora radiospectrograph at the time of report
issue.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 25 Feb: Quiet to Unsettled
Estimated Indices 25 Feb : A K
Australian Region 5 2113 2012
Darwin 4 2112 1112
Townsville 3 1103 1012
Learmonth 3 20-- ----
Culgoora 4 1113 1012
Canberra 4 1113 2012
Hobart 4 1113 2012
Casey(Ant) 9 3332 2121
Observed Regional daily pc3 Indices 25 FEB :
Townsville 0 (Quiet)
Learmonth 0 (Quiet)
Culgoora 6 (Quiet)
Canberra 20 (Quiet)
Hobart 8 (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 25 Feb : A
Fredericksburg 10
Planetary 10
Observed AFr/Ap Indices 24 Feb : A K
Fredericksburg 9
Planetary 11 3333 3322
2B. MAGNETIC FORECAST
Date Ap Conditions
26 Feb 15 Unsettled to Active
27 Feb 13 Unsettled to Active
28 Feb 10 Quiet to Unsettled
COMMENT: Mostly quiet geomagnetic conditions were observed over
the UT day. Solar wind speed remained steady at about 350 km/s.
The north-south component of the interplanetary magnetic field
was mostly neutral, but developed a southward bias of about 4
nT late in the UT day. Expect mostly quiet to unsettled conditions,
with the chance of isolated active periods, for the next few
days.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
25 Feb Normal Normal Normal
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
26 Feb Normal Normal Normal-Fair
27 Feb Normal Normal Normal-Fair
28 Feb Normal Normal Normal-Fair
COMMENT: HF conditions mostly near normal. Chance of isolated
periods of disturbance at high latitudes in association with
geomagnetic activity.
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
25 Feb 53
Observed Australian Regional MUFs
Equatorial PNG Region:
Near predicted monthly values during local day,
Enhanced by 20% 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 over the UT day.
Predicted Monthly T index for February: 53
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
26 Feb 50 near predicted monthly values
27 Feb 50 Near predicted monthly values
28 Feb 55 Near predicted monthly values
COMMENT: HF conditions mostly near normal. Mid to southern Aus
regions may experience mild depressions overnight and around
local dawn. Chance of isolated periods of disturbance in Antrarctic
regions.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 24 Feb
Daily Proton Fluence >1 MeV: 4.6E+05
Daily Proton Fluence >10 MeV: 1.4E+04
Daily Electron Fluence >2 MeV: 3.40E+07 (normal)
X-ray background: B1.2
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 24 Feb
Speed: 398 km/sec Density: 1.9 p/cc Temp: 48400 K Bz: 0 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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