[Ips-dsgr] IPS Daily Report - 30 March 04
rwc
rwc at ips.gov.au
Wed Mar 31 09:55:27 EST 2004
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 30/2330Z MARCH 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 30 MARCH AND FORECAST FOR 31 MARCH - 02 APRIL
STATUS INDICATORS SOL:*YELLOW* MAG:GREEN ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 30 Mar: Low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number for 30 Mar: 127/80
1B. SOLAR FORECAST
31 Mar 01 Apr 02 Apr
Activity Low to moderate Low to moderate Low to moderate
Fadeouts Possible Possible Possible
10.7cm/SSN 130/84 130/84 135/89
COMMENT: M-class flare activity is possible from solar region
582. Solar wind speeds have declined very slowly over the past
24 hours, remaining elevated at approximately 550km/s. The north-south
component of the IMF continues to fluctuate between +5 to -5
nT. This coronal hole solar wind stream is expected to continue
to abate over the next couple of days and geomagnetic activity
should be mostly quiet to unsettled levels.
-----------------------------------------------------------
2A. MAGNETIC SUMMARY
Geomagnetic field for Australian Region 30 Mar: Quiet to Active
Estimated Indices 30 Mar : A K
Australian Region 11 2233 4212
Darwin 11 1233 4222
Townsville 8 2223 3213
Learmonth 10 2223 4211
Culgoora 9 1233 3211
Canberra 13 2234 4212
Hobart 11 2233 4211
Casey(Ant) 13 3-43 3212
Observed Regional daily pc3 Indices 30 MAR :
Townsville 0 (Quiet)
Learmonth 2 (Quiet)
Culgoora 9 (Quiet)
Canberra 15 (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 30 Mar : A
Fredericksburg 12
Planetary 17
Observed AFr/Ap Indices 29 Mar : A K
Fredericksburg 12
Planetary 12 2333 3332
2B. MAGNETIC FORECAST
Date Ap Conditions
31 Mar 12 Quiet to unsettled with the chance of isolated
active periods.
01 Apr 8 Quiet to unsettled
02 Apr 6 Quiet
COMMENT: Isolated active periods were observed over the past
24 hours due to a persisting coronal hole solar wind stream.
Geomagnetic activity is expected to decline over the next couple
of days as solar wind speeds are anticipated to decrease.
-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
Latitude Band
Date Low Middle High
30 Mar Normal Normal Normal-fair
PCA Event : No event.
3B. GLOBAL HF PROPAGATION FORECAST
Latitude Band
Date Low Middle High
31 Mar Normal Normal Normal-Fair
01 Apr Normal Normal Normal-Fair
02 Apr Normal Normal Normal
COMMENT: Mostly normal to good HF conditions are expected for
the next few days.
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date T index
30 Mar 86
Observed Australian Regional MUFs
Equatorial PNG Region:
Enhanced by 25% during local day,
Enhanced by 50% during local night.
Enhanced by 30% after local dawn.
Northern Australian Region:
Enhanced by 20% during local day,
Enhanced by 30% during local night.
Enhanced by 35% after local dawn.
Southern Australian and New Zealand Region:
Enhanced by 20% during local day,
Enhanced by 20% during local night.
Antarctic Region (Casey/Scott Base):
Mostly near predicted monthly values.
Predicted Monthly T index for March: 49
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date T index MUFs
31 Mar 75 Mostly near predicted monthly values to enhanced
5-15% at times.
01 Apr 80 10 to 20% above predicted monthly values
02 Apr 80 10 to 20% above predicted monthly values
COMMENT: Mostly normal to good HF conditions are expected for
the next few days.
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY
GOES satellite data for 29 Mar
Daily Proton Fluence >1 MeV: 1.2E+06
Daily Proton Fluence >10 MeV: 1.2E+04
Daily Electron Fluence >2 MeV: 3.60E+08 (moderate)
X-ray background: B3.4
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
ACE Satellite Solar Wind Day Averaged Data for 29 Mar
Speed: 612 km/sec Density: 2.0 p/cc Temp: 157000 K Bz: 0 nT
(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
-----------------------------------------------------------
IPS Radio and Space Services | email: asfc at ips.gov.au
PO Box 1386 | WWW: http://www.ips.gov.au
Haymarket NSW 1240 AUSTRALIA | FTP: ftp://ftp.ips.gov.au
tel: +61 2 9213 8010 | fax: +61 2 9213 8060
IMPORTANT: This e-mail, including any attachments, may contain,confidential
or copyright information. The views expressed in this message are those of
the individual sender, unless specifically stated to be the views of IPS.
If you are not the intended recipient, please contact the sender immediately
and delete all copies of this e-mail and attachments.
More information about the ips-dsgr
mailing list