[Ips-dsgr] IPS Daily Report - 26 March 07

rwc rwc at ips.gov.au
Tue Mar 27 09:30:26 EST 2007


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 26/2330Z MARCH 2007 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 26 MARCH AND FORECAST FOR 27 MARCH - 29 MARCH
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 26 Mar:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 26 Mar:  74/11

1B. SOLAR FORECAST
             27 Mar             28 Mar             29 Mar
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    75/13              75/13              75/13
COMMENT: The solar activity remained very low on 26 March 
UT day. The effect of the coronal hole kept the solar wind 
stream strengthened. The solar wind velocity increased from 
440 to 520 km/s during the first seven hours of the UT day 
today and then gradually decreased to 460 km/s by the time 
of this report (around 2300UT). The north-south component 
(Bz) showed minor to moderate (mostly around +/-5 nT) 
fluctuations on both sides of the normal value almost the 
whole day. The effect of this coronal hole is expected to 
keep the solar wind stream strengthened for the next one to 
two days. Solar activity is expected to remain at very low 
levels for the next few days. 

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 26 Mar: Quiet to unsettled
with some active periods. 

Estimated Indices 26 Mar :  A   K           
   Australian Region       9   23222322
      Darwin               7   22122322
      Townsville           8   12222332
      Learmonth           10   23222422
      Camden               6   12221312
      Canberra             9   12222422
      Hobart               9   13222412
      Casey(Ant)          13   34322313
    
Observed Regional daily pc3 Indices 26 Mar : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Camden              31   (Quiet to unsettled)
      Canberra            31   (Quiet to unsettled)
      Hobart              20   (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 26 Mar : A 
           Fredericksburg         8
           Planetary             10                         

Observed AFr/Ap Indices 25 Mar :  A   K
           Fredericksburg         8
           Planetary             10   2124 4212     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
27 Mar    12    Mostly quiet to unsettled, active periods possible. 
28 Mar     8    Mostly quiet, unsettled periods possible. 
29 Mar     5    Quiet 
COMMENT: The effect of a high speed solar wind stream from 
a coronal hole may raise the geomagnetic activity levels to 
unsettled and sometimes to active levels on 27 March. The 
effect of the coronal hole is expected to gradually diminish 
thereafter. 

-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
26 Mar      Fair-normal    Fair-normal    Normal-poor    
PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
27 Mar      Normal         Normal         Fair          
28 Mar      Normal         Normal         Normal-fair   
29 Mar      Normal         Normal         Normal        
COMMENT: Mild to moderate degradations in HF conditions and
depressions in MUFs are possible on high latitude circuits 
on 27 March due to the possibility of an enhancement in 
geomagnetic activity levels on this day. Minor to mild 
degradations in HF conditions and deprssesions in MUFs may 
also be observed at times on high latitudes on 28 March. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
26 Mar    12

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Depressions observed after local dawn.
      Near predicted monthly values during local night.
   Northern Australian Region:
      Near predicted monthly values.
   Southern Australian and New Zealand Region:
      Depressed by 15% during local day,
      Near predicted monthly values during local night.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day
      with periods of degradations.

Predicted Monthly T index for March:  10

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
27 Mar    14    near predicted monthly values 
28 Mar    16    Near predicted monthly values 
29 Mar    18    Near predicted monthly values 
COMMENT: HF conditions are expected to remain mostly normal 
for most parts of the Aus/NZ region for the next three days 
with some possibility of minor degrdations and MUF depressions 
in the Southern Aus/NZ regions at times on 27 March. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 25 Mar
       Daily Proton Fluence >1 MeV:   1.1E+06
       Daily Proton Fluence >10 MeV:  1.7E+04
       Daily Electron Fluence >2 MeV: 4.00E+06   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.0

ACE Satellite Solar Wind Day Averaged Data for 25 Mar
Speed: 432 km/sec  Density:    6.0 p/cc  Temp:   105000 K  Bz:   3 nT

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