[Ips-dsgr] IPS Daily Report - 17 December 03
rwc
rwc at ips.gov.au
Thu Dec 18 10:38:34 EST 2003
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 17/2330Z DECEMBER 2003 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 17 DECEMBER AND FORECAST FOR 18 DECEMBER - 20 DECEMBER
STATUS INDICATORS SOL:* YELLOW * MAG:** RED ** ION: GREEN
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1A. SOLAR SUMMARY
Activity 17 Dec: Low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 17 Dec: 118/70
1B. SOLAR FORECAST
18 Dec 19 Dec 20 Dec
Activity Low Low Low to moderate
Fadeouts None expected None expected Possible
10.7cm/SSN 125/78 130/84 135/89
COMMENT: A C8 level flare was produced from region 525 at 0300UT.
Other minor B- to C-class activity also observed. Surging was
observed in Culgoora H-Alpha imagery around 2030UT on the East
equatorial limb, indicating a possible approaching active region
behind the limb.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 17 Dec: Quiet
Estimated Indices 17 Dec : A K
Australian Region 6 2222 2212
Darwin 5 2211 2222
Townsville 6 2222 2213
Learmonth 5 2112 2211
Culgoora 5 1222 2202
Canberra 5 1222 2202
Hobart 5 1222 2211
Casey(Ant) 9 ---3 2221
Observed Regional daily pc3 Indices 17 DEC :
Townsville 2 (Quiet)
Learmonth 0 (Quiet)
Culgoora 10 (Quiet)
Canberra 22 (Quiet to unsettled)
Hobart 31 (Quiet to 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 17 Dec : A
Fredericksburg 11
Planetary 12
Observed AFr/Ap Indices 16 Dec : A K
Fredericksburg 9
Planetary 11 3333 3332
2B. MAGNETIC FORECAST
Date Ap Conditions
18 Dec 10 Quiet to Unsettled
19 Dec 15 Unsettled to Active
20 Dec 20 active
COMMENT: IPS Geomagnetic Warning 58 was issued on 15 December
and is current for interval 19-20 December. As solar wind parameters
decline towards normal levels, geomagnetic conditions were mostly
at quiet levels over the UT day at low to mid latitudes. Isolated
active to minor storm periods were observed in the first half
of the UT day at high latitudes. A smaller equatorial coronal
hole is expected to rotate into geoeffective position by Dec
19, bringing a brief return to active conditions on Dec 19-20.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
17 Dec Normal Normal Normal
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
18 Dec Normal Normal Normal-Fair
19 Dec Normal Normal Normal-Fair
20 Dec Normal Normal-Fair Fair
COMMENT: Improved HF conditions today and for most of 18 Dec.
Mid to high latitudes are expected to become moderately degraded
around 19 Dec due to another coronal hole high speed wind stream.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
17 Dec 70
Observed Australian Regional MUFs
Equatorial PNG Region:
Near predicted monthly values.
Northern Australian Region:
Enhanced by 15% over the UT day.
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 December: 50
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
18 Dec 80 about 10% above predicted monthly values
19 Dec 65 near predicted monthly values
20 Dec 45 near predicted monthly values/depressed 5 to
10%
COMMENT: IPS HF Communications Warning 97 was issued on 15 December
and is current for interval 19-20 December. MUFs are expected
to be generally near predicted monthly values over coming days.
Another mild to moderately disturbed interval from a coronal
hole wind stream is expected 19 to 20 Dec.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 16 Dec
Daily Proton Fluence >1 MeV: 2.4E+06
Daily Proton Fluence >10 MeV: 1.1E+04
Daily Electron Fluence >2 MeV: 9.00E+08 (high)
X-ray background: B2.4
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 16 Dec
Speed: 600 km/sec Density: 1.5 p/cc Temp: 122000 K Bz: -1 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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