[Ips-dsgr] IPS Daily Report - 25 September 06

rwc rwc at ips.gov.au
Tue Sep 26 09:47:48 EST 2006


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 25/2330Z SEPTEMBER 2006 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 25 SEPTEMBER AND FORECAST FOR 26 SEPTEMBER - 28 SEPTEMBER
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 25 Sep:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 25 Sep:  70/5


1B. SOLAR FORECAST
             26 Sep             27 Sep             28 Sep
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    70/5               80/20              75/13
COMMENT: Solar wind speed is still elevated from the recurrent 
coronal hole, but is declining slowly. Vsw is currently down 
to 550km/sec and likely to return to average speeds in a day. 
Geomagnetic activity should correspondingly decrease as solar 
wind interaction with the geomagnetic field decreases. IMF Bz 
was southwards from ~08-11UT, merging with the geomagnetic field 
and causing elevated activity. Since 11UT Bz has been predominantly 
northwards, and recently oscillating N-S since 19UT with an increase 
in solar wind density. The combination of these two conditions 
may be causing observed increase in polar geomagnetic activity 
as Bz southward has not been sustained. AR910 has decayed to 
a plage region with no flares recorded. Flare activity is expected 
to be nil in the next 2-3 days in the absence of a new active 
region. The Type II radio emissions observed on the 23rd and 
24th do not appear to have produced geoeffective shock fronts 
from the SOHO spacecraft LASCO C3 imagery. 




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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 25 Sep: Quiet to Unsettled 

Estimated Indices 25 Sep :  A   K           
   Australian Region       6   22132102
      Darwin               7   22232112
      Learmonth            8   21243102
      Culgoora             5   12132101
      Camden               4   12132001
      Canberra             7   12143002
      Hobart               7   12143001
      Casey(Ant)          10   33-32113
    
Observed Regional daily pc3 Indices 25 Sep : 
      Charters_Towers      0   (Quiet)
      Learmonth           14   (Quiet)
      Camden               8   (Quiet)
      Hobart              25   (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 25 Sep : A 
           Fredericksburg         6
           Planetary              8                         

Observed AFr/Ap Indices 24 Sep :  A   K
           Fredericksburg        15
           Planetary             23   5545 3222     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
26 Sep    10    Quiet to Unsettled 
27 Sep     8    Quiet to Unsettled 
28 Sep     6    Quiet 
COMMENT: Solar wind speed observed by ACE spacecraft at L1 is 
still elevated at 550km/sec from the recurrent coronal hole, 
but is declining slowly and likely to return to average speeds 
in a day. Geomagnetic activity should correspondingly decrease 
as solar wind interaction with the geomagnetic field decreases. 
IMF Bz was southwards from ~08-11UT, merging with the geomagnetic 
field and causing elevated activity at polar and mid latitudes. 
Bz predominantly northwards from 11UT caused magnetic activity 
to decrease. However north-south oscillating Bz since 19UT with 
an increase in solar wind density seems to be be causing an observed 
increase in polar geomagnetic activity as Bz southward has not 
been sustained. There is a slight indication of increasing
mid-latitude 
activity also. 

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
25 Sep      Fair           Normal         Fair           
PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
26 Sep      Fair           Normal         Fair          
27 Sep      Fair-normal    Normal         Fair-normal   
28 Sep      Normal         Normal         Normal        
COMMENT: Low latitudes have shown ionospheric depressions,
particularly 
during the daytime and pre-dawn. This is presumed due to geomagnetic 
activity from the coronal-hole induced solar-wind speed elevation. 
Mid-latitudes appear to be still be holding better but are a 
little depressed. conditions should return to normal in a day 
as Vsw declines to average. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
25 Sep     6

Observed Australian Regional MUFs
slightly below predicted monthly values

Predicted Monthly T index for September:  11

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
26 Sep    10    5 to 10% below predicted monthly values 
27 Sep    12    Near predicted monthly values 
28 Sep    12    Near predicted monthly values 
COMMENT: Equatorial latitudes (PNG, Niue, Nth QLD) have shown 
ionospheric depressions, particularly during the daytime and 
pre-dawn. This is presumed due to geomagnetic activity from the 
coronal-hole induced solar-wind speed elevation. Mid-latitudes 
appear to be still be holding better but are a little depressed. 
Conditions should return to normal in a day as Vsw declines to 
average. Spread F was not as prevalent as expected but did occur 
significantly at mid to higher latitudes (e.g. Hobart) 
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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 24 Sep
       Daily Proton Fluence >1 MeV:   7.0E+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 24 Sep
Speed: NA km/sec  Density:  NA p/cc  Temp:  NA K  Bz:  NA nT

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