[Ips-dsgr] IPS Daily Report - 29 March 07

rwc rwc at ips.gov.au
Fri Mar 30 09:38:10 EST 2007


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 29/2330Z MARCH 2007 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 29 MARCH AND FORECAST FOR 30 MARCH - 01 APRIL
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 29 Mar:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 29 Mar:  74/11


1B. SOLAR FORECAST
             30 Mar             31 Mar             01 Apr
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    75/13              75/13              75/13
COMMENT: Solar activity was very low over the last 24 hours. 
Solar wind velocity declined from 430km/s to be 400km/s at the 
time of this report. The north-south component (Bz) of the
interplanetary magnetic field (IMF) fluctuated between +/-2nT for
the first half of the UT day after which its magnitude increased
to 4nT but with no southward excursions. Solar wind parameters
are expected to increase on 01Apr with the arrival of a high
speed solar wind stream from a equatorial positioned geoeffective
coronal hole. Solar activity is expected to remain at very low
levels for the next few days with no changes expected in the
only sunspot on disk, region 949. 




-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 29 Mar: Quiet 

Estimated Indices 29 Mar :  A   K           
   Australian Region       4   22111112
      Darwin               4   21111112
      Townsville           6   22212222
      Learmonth            5   22111122
      Camden               2   11101002
      Canberra             2   11001002
      Hobart               2   12001001
      Casey(Ant)           6   23212111
    
Observed Regional daily pc3 Indices 29 Mar : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Camden              15   (Quiet)
      Canberra             0   (Quiet)
      Hobart               0   (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 and have been shown to be
well correlated with rejection of high resolution aeromagnetic
survey flight-line data. 

NOTE: Indices may have been generated from data obtained in 
cooperation with the following organisations: Geoscience Australia, 
University of Newcastle Space Physics Group, Australian Government 
Antarctic Division and Space Environment Research Center, Japan.


Estimated AFr/Ap Indices 29 Mar : A 
           Fredericksburg         5
           Planetary              5                         

Observed AFr/Ap Indices 28 Mar :  A   K
           Fredericksburg         6
           Planetary              7   3321 0101     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
30 Mar     5    Quiet 
31 Mar     5    Quiet 
01 Apr     8    Quiet to Unsettled 
COMMENT: Quiet conditions observed over the last 24 hours. Quiet 
geomag levels are expected for the next 2 days. An increase in
geomagnetic activity is expected from 01Apr onwards with the
anticipated arrival of a high speed solar wind stream from
a equatorial positioned coronal hole that will then be
geoeffective. 

-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
29 Mar      Normal         Normal         Normal-fair    
PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
30 Mar      Normal         Normal         Normal
31 Mar      Normal         Normal         Normal
01 Apr      Normal         Normal         Normal-Fair
COMMENT: Mostly normal HF conditions observed over the last 24 
hours for low to mid latitudes, with mild to moderate degradations 
for high latitudes. Similar conditions are expected for the next 
3 days. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
29 Mar    12

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      No data available during local day,
      Depressed by 15% during local night.
      Depressed by 25% after local dawn.
   Northern Australian Region:
      Near predicted monthly values.
   Southern Australian and New Zealand Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day.

Predicted Monthly T index for March:  10

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
30 Mar    10    near predicted monthly values 
31 Mar    15    near predicted monthly values 
01 Apr    15    near predicted monthly values 
COMMENT: Normal HF conditions observed for Southern Aus/NZ regions 
over the last 24 hours. Mostly normal ionospheric support for 
Northern AUS and Equatorial regions, with depressions observed 
after local dawn and during local night along with sporadic E 
in the first half of the UT day. Normal conditions for Antarctic 
regions with some disturbed periods observed for the later half 
of the UT day. Similar HF conditions are expected for each region 
over the next 2 days. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 28 Mar
       Daily Proton Fluence >1 MeV:   7.8E+05
       Daily Proton Fluence >10 MeV:  1.7E+04
       Daily Electron Fluence >2 MeV: 9.90E+06   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 2%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.0

ACE Satellite Solar Wind Day Averaged Data for 28 Mar
Speed: 552 km/sec  Density:    1.9 p/cc  Temp:   137000 K  Bz:   0 nT

(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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