[Ips-dsgr] IPS Daily Report - 16 March 04
rwc
rwc at ips.gov.au
Wed Mar 17 10:08:59 EST 2004
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 16/2330Z MARCH 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 16 MARCH AND FORECAST FOR 17 MARCH - 19 MARCH
STATUS INDICATORS SOL:GREEN MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 16 Mar: Very low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 16 Mar: 110/60
1B. SOLAR FORECAST
17 Mar 18 Mar 19 Mar
Activity Low Low Low
Fadeouts None expected None expected None expected
10.7cm/SSN 115/66 115/66 110/60
COMMENT: The solar disk has been quiet over the past 24 hours.
Solar wind speed remains steady at around 450km/sec over past
24 hours. The north-south component of the interplanetary magnetic
field was mostly neutral over the UT day. A narrow north polar
extension coronal hole is now at the centre of the solar disk.
This narrow hole may produce a brief mild increase in solar wind
speed around 19-20 Mar. Two new solar regions are expected to
rotate onto the solar disk just north of the solar equator in
coming days. There is an outside chance of a very weak shock
on 17 Mar from a recent erupting filament.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 16 Mar: Quiet to Unsettled
Estimated Indices 16 Mar : A K
Australian Region 7 2212 2322
Darwin 7 2212 1322
Townsville 7 2212 1323
Learmonth 8 3212 1322
Culgoora 7 2202 2322
Canberra 8 2213 2322
Hobart 8 2213 2322
Casey(Ant) 14 34-2 2333
Observed Regional daily pc3 Indices 16 MAR :
Townsville 0 (Quiet)
Learmonth 0 (Quiet)
Culgoora 23 (Quiet to unsettled)
Canberra 79 (Active)
Hobart 45 (Unsettled)
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 16 Mar : A
Fredericksburg 8
Planetary 10
Observed AFr/Ap Indices 15 Mar : A K
Fredericksburg 11
Planetary 13 4323 3332
2B. MAGNETIC FORECAST
Date Ap Conditions
17 Mar 15 Unsettled to Active
18 Mar 4 Quiet
19 Mar 15 Unsettled to Active
COMMENT: Generally quiet conditions expected. The solar filament
may cause active periods on 17 Mar. A coronal hole may cause
active periods during 19-20 Mar.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
16 Mar Normal Normal Normal
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
17 Mar Normal Normal Normal-Fair
18 Mar Normal Normal Normal
19 Mar Normal Normal Normal-Fair
COMMENT: Generally good HF conditions expected. Mild degradation
possible 17 Mar and 19 Mar for mid to high latitudes.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
16 Mar 58
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 during local day,
Enhanced by 15% during local night.
Southern Australian and New Zealand Region:
Near predicted monthly values during local day,
Enhanced by 15% during local night.
Antarctic Region (Casey/Scott Base):
Near predicted monthly values over the UT day.
Predicted Monthly T index for March: 49
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
17 Mar 50 Near predicted monthly values
18 Mar 50 Near predicted monthly values
19 Mar 50 Near predicted monthly values
COMMENT: MUFs are generally expected to return to near predicted
monthly values over the next few days. Mildly degraded HF communication
conditions may be experienced local nigt hours 17 and 19-20 Mar.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 15 Mar
Daily Proton Fluence >1 MeV: 6.2E+05
Daily Proton Fluence >10 MeV: 1.2E+04
Daily Electron Fluence >2 MeV: 3.20E+08 (moderate)
X-ray background: B1.3
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 15 Mar
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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