[Ips-dsgr] IPS Daily Report - 11 March 04
rwc
rwc at ips.gov.au
Fri Mar 12 10:15:30 EST 2004
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 11/2330Z MARCH 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 11 MARCH AND FORECAST FOR 12 MARCH - 14 MARCH
STATUS INDICATORS SOL:** YELLOW ** MAG:GREEN ION: ** YELLOW **
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1A. SOLAR SUMMARY
Activity 11 Mar: Low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 11 Mar: 113/64
1B. SOLAR FORECAST
12 Mar 13 Mar 14 Mar
Activity Low to moderate Low to moderate Low to moderate
Fadeouts Possible Possible Possible
10.7cm/SSN 110/60 110/60 100/48
COMMENT: Solar wind speed showed an overall declining trend over
past 24 hours. This indicates that the Earth is gradually leaving
the recent coronal hole high speed wind stream. The north-south
component of the interplanetary magnetic field was southward 5 to
10 nT during the second half of the UT day. Solar region 570 is now
nearing the centre of the solar disk. There is chance for an
islolated low level M class flare from this region, as some magnetic
polarity mixing is apparent in the leader spots of this region.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 11 Mar: Quiet to Minor Storm
Estimated Indices 11 Mar : A K
Australian Region 23 3334 3454
Darwin 18 3333 3443
Townsville 20 3334 3444
Learmonth 25 4234 4454
Culgoora 25 2334 3554
Canberra 23 3334 3454
Hobart 26 3334 3554
Casey(Ant) 28 --44 3455
Observed Regional daily pc3 Indices 11 MAR :
Townsville 27 (Quiet to unsettled)
Learmonth 67 (Active)
Culgoora 97 (Minor storm)
Canberra 172 (Severe storm)
Hobart 146 (Severe storm)
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 11 Mar : A
Fredericksburg 20
Planetary 45
Observed AFr/Ap Indices 10 Mar : A K
Fredericksburg 36
Planetary 40 5664 5334
2B. MAGNETIC FORECAST
Date Ap Conditions
12 Mar 15 Active to unsettled
13 Mar 12 Unsettled
14 Mar 10 Quiet to Unsettled
COMMENT: Declining trend in geomagnetic activity expected over
next 24 hours as the Earth leaves the coronal hole wind stream.
Active conditions with chance of minor storm periods may be experienced
during next 24 hours if southward IMF conditions persist.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
11 Mar Normal Fair-normal Fair-normal
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
12 Mar Normal Fair-Normal Fair
13 Mar Normal Normal Fair-normal
14 Mar Normal Normal Fair-normal
COMMENT: Improving HF conditions at mid to high latitudes as
the effects of coronal hole wind stream subside.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
11 Mar 77
Observed Australian Regional MUFs
Equatorial PNG Region:
Near predicted monthly values during local day,
Enhanced by 20% during local night.
Northern Australian Region:
Enhanced by 15% during local day,
Enhanced by 35% during local night.
Southern Australian and New Zealand Region:
Near predicted monthly values during local day,
Enhanced by 30% 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
12 Mar 20 depressed 10 to 15% (southern Aus/NZ region)
12 Mar 50 near predicted monthly values (Northern Aus region)
13 Mar 50 near predicted monthly values
14 Mar 50 near predicted monthly values
COMMENT: Depressed MUFs observed after local dawn for
southern Aus/NZ regiuon. Northern Aus region MUFs near
predicted monthly values.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 10 Mar
Daily Proton Fluence >1 MeV: 2.0E+06
Daily Proton Fluence >10 MeV: 1.3E+04
Daily Electron Fluence >2 MeV: 1.60E+07 (normal)
X-ray background: B2.2
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 10 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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