[Ips-dsgr] IPS Daily Report - 23 May 04
rwc
rwc at ips.gov.au
Mon May 24 09:34:50 EST 2004
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 23/2330Z MAY 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 23 MAY AND FORECAST FOR 24 MAY - 26 MAY
STATUS INDICATORS SOL:GREEN MAG:GREEN ION: GREEN
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1A. SOLAR SUMMARY
Activity 23 May: Low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 23 May: 104/53
1B. SOLAR FORECAST
24 May 25 May 26 May
Activity Low Low Low
Fadeouts None expected None expected None expected
10.7cm/SSN 105/54 105/54 100/48
COMMENT: Active region 618 produced only B to minor C-class flare
activity over the past 24 hours. This region has maintained moderate
magnetic complexity and a trend to increasing size. There is
a possibility of isolated high C- to low M-class activity from
this region.
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2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 23 May: Quiet to Unsettled
Estimated Indices 23 May : A K
Australian Region 7 3212 2221
Darwin 7 3212 2222
Townsville 8 3222 2221
Learmonth 8 3222 2222
Culgoora 7 3212 2221
Canberra 7 3212 2221
Hobart 6 2212 2221
Casey(Ant) 9 3322 2222
Observed Regional daily pc3 Indices 23 MAY :
Townsville 2 (Quiet)
Learmonth 8 (Quiet)
Culgoora 35 (Quiet to unsettled)
Canberra 45 (Unsettled)
Hobart 61 (Active)
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 23 May : A
Fredericksburg 10
Planetary 10
Observed AFr/Ap Indices 22 May : A K
Fredericksburg 7
Planetary 11 2343 3222
2B. MAGNETIC FORECAST
Date Ap Conditions
24 May 8 Quiet to unsettled
25 May 8 Mostly quiet with unsettled periods.
26 May 8 Mostly quiet with unsettled periods.
COMMENT: There was little change in solar wind parameters over
the UT day. Solar wind speed remains slightly elevated at 460-480
km/s. The Bz component of the IMF has fluctuated mildly about
neutral. Some extended intervals of southward bias in Bz have
resulted in isolated active periods at high latitudes only. Geomagnetic
conditions should continue at mainly quiet levels with isolated
unsettled intervals at low to mid latitudes and possible active
periods at high latitudes. A decline to generally quiet conditions
is anticipated by day three.
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3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
23 May Normal Normal Normal-fair
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
24 May Normal Normal Normal-Fair
25 May Normal Normal Normal-Fair
26 May Normal Normal Normal-Fair
COMMENT: Normal HF conditions are expected for the next few days
with possible isolated degradations at high latitudes.
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
23 May 59
Observed Australian Regional MUFs
Equatorial PNG Region:
Enhanced by 20% during local day,
Enhanced by 30% 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 May: 43
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
24 May 60 5 to 15% above predicted monthly values
25 May 65 5 to 15% above predicted monthly values
26 May 65 5 to 15% above predicted monthly values
COMMENT: Periods of spread-F observed S Aus and Antarctic region.
Mostly normal to good HF conditions are expected over the next
three days. Possible isolated degradations at high latitudes
in association with mild geomagnetic disturbances.
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5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 22 May
Daily Proton Fluence >1 MeV: 2.1E+05
Daily Proton Fluence >10 MeV: 1.4E+04
Daily Electron Fluence >2 MeV: 3.30E+06 (normal)
X-ray background: B2.0
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 22 May
Speed: 494 km/sec Density: 2.2 p/cc Temp: 132000 K Bz: -1 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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