[Ips-dsgr] IPS Daily Report - 06 October 05

rwc rwc at ips.gov.au
Fri Oct 7 09:41:39 EST 2005


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 06/2330Z OCTOBER 2005 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 06 OCTOBER AND FORECAST FOR 07 OCTOBER - 09 OCTOBER
STATUS INDICATORS SOL:GREEN   MAG:** RED **     ION: GREEN
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1A. SOLAR SUMMARY
Activity 06 Oct:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 06 Oct:  80/20


1B. SOLAR FORECAST
             07 Oct             08 Oct             09 Oct
Activity     Low                Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    80/20              80/20              80/20
COMMENT: Solar activity was very low over the previous UT day 
with just one B-class X-ray flare of magnitude B2.1 at 0603Z. 
Background solar X-ray flux was very low over the previous 24 
hours. Region 813 decayed slightly over the period and has been 
reclassified as DAI beta. This region has the potential to produce 
isolated C-class flares. Overall solar activity is expected to 
be low to very low over the next 24 hours. No new regions were 
numbered. The recurrent equatorial coronal hole currently passing 
solar central meridian should be geoeffective late on Saturday 
08 Oct. Currently the solar wind speed remains slow at ~310km/s, 
and IMF Bz was oscillating about 0 at the time of this report. 



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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 06 Oct: Quiet 

Estimated Indices 06 Oct :  A   K           
   Australian Region       4   1111 2211
      Darwin               3   1110 1211
      Learmonth            2   1000 1210
      Culgoora             3   1111 2111
      Canberra             3   1101 2111
      Hobart               2   1001 2111
      Casey(Ant)           9   3332 2212
    
Observed Regional daily pc3 Indices 06 Oct : 
      Townsville          NA
      Learmonth            0   (Quiet)
      Culgoora             0   (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. 


Estimated AFr/Ap Indices 06 Oct : A 
           Fredericksburg         4
           Planetary              5                         

Observed AFr/Ap Indices 05 Oct :  A   K
           Fredericksburg         2
           Planetary              4   0110 1121     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
07 Oct     5    Quiet 
08 Oct    15    Unsettled to Active 
09 Oct    20    active 
COMMENT: The geomagnetic field has been quiet over the UT day, 
conditions which are expected to continue over the next 24 hours. 
The solar wind speed remains at low levels and the IMF Bz was 
oscillating about 0nT at the time of this report. These quiet 
geomagnetic conditions are expected to continue through to Saturday 
08 Oct, increasing to active late on Sat 08 Oct due to the arrival 
of a high speed coronal hole wind stream associated with the 
recurrent equatorial coronal hole currently passing solar central 
meridian. Active conditions with isolated minor storm periods, 
particularly at high latitudes are possible late Sat 08 Oct continuing 
through Sun 09 Oct. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
07 Oct      Normal         Normal         Normal-fair   
08 Oct      Normal         Normal         Normal-fair   
09 Oct      Normal         Normal-fair    Fair          
COMMENT: Isolated periods of depression were observed at low 
latitudes over the UT day, otherwise conditions were mostly normal. 
Expect mostly normal HF conditions to continue through to late 
Saturday 08 Oct with subsequent periods of degradation possible 
on 09 Oct in association with the expected elevation in geomagnetic 
activity levels on that day. Further depressions at low latitudes 
possible over the next 24 hours. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
06 Oct    23

Observed Australian Regional MUFs
   Equatorial PNG Region:
      Depressed by 20% during local day,
      Depressed by 15% during local night.
   Northern Australian Region:
      Depressed by 15% during local day,
      Near predicted monthly values during local night.
   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 October:  23

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
07 Oct    26    Depressed 15-20% Equatorial/N.Aus region, Near 
                predicted monthly values elsewhere 
08 Oct    23    near predicted monthly values 
09 Oct    11    near predicted monthly values/depressed 10 to 
                20% 
COMMENT: Variable depressions observed Equatorial/N Aus regions. 
Expect generally normal HF conditions until late Sat 08 Oct, 
with variable depressions continuing in the Equatorial/N Aus 
regions. Isolated disturbances possible in the Antarctic region 
associated with periods of enhanced geomagnetic activity. Depressed 
conditions expected on 09 Oct in response to increased geomagnetic 
activity levels. 
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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 05 Oct
       Daily Proton Fluence >1 MeV:   4.3E+05
       Daily Proton Fluence >10 MeV:  1.6E+04
       Daily Electron Fluence >2 MeV: 1.30E+08 (moderate fluence)  
Electron Fluence Daily Deep Dielectric Discharge Probability:12%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B1.3

ACE Satellite Solar Wind Day Averaged Data for 05 Oct
Speed: 311 km/sec  Density:    2.7 p/cc  Temp:    27800 K  Bz:  -1 nT

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