[Ips-dsgr] IPS Daily Report - 28 October 06

rwc rwc at ips.gov.au
Sun Oct 29 10:45:13 EST 2006


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 28/2330Z OCTOBER 2006 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 28 OCTOBER AND FORECAST FOR 29 OCTOBER - 31 OCTOBER
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 28 Oct:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 28 Oct:  75/13

1B. SOLAR FORECAST
             29 Oct             30 Oct             31 Oct
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    75/13              70/5               70/5
COMMENT: Solar activity continued to remain at very low 
levels today as well. Solar wind speed remained around 
320 km/s in the first half of the UT day and then gradually 
increased to around 550 km/s by 2300UT. This increase in 
the solar wind speed seems to have been caused by the 
anticipated effect of the coronal hole. The coronal hole 
effect seems to have eventuated later than expected. Periods 
of strengthened solar wind stream due to the effect of 
this coronal hole can be expected for the next one and a 
half to two days. The north-south component of the 
interplanetary magnetic field (Bz) remained slightly to 
moderately negative (upto around -5nT) for most part of 
the UT day today. 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 28 Oct: Quiet to Unsettled 

Estimated Indices 28 Oct :  A   K           
   Australian Region      11   22233323
      Darwin              11   22233323
      Learmonth           12   22233333
      Culgoora             -   --------
      Camden              10   12233323
      Canberra            11   22233323
      Hobart              11   12333323
      Casey(Ant)          15   33333333
    
Observed Regional daily pc3 Indices 28 Oct : 
      Charters_Towers      0   (Quiet)
      Learmonth            0   (Quiet)
      Hobart              21   (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 and have been shown to be
well correlated with rejection of high resolution aeromagnetic
survey flight-line data. 


Estimated AFr/Ap Indices 28 Oct : A 
           Fredericksburg        10
           Planetary             15                         

Observed AFr/Ap Indices 27 Oct :  A   K
           Fredericksburg         3
           Planetary              2   1001 0012     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
29 Oct    15    Mostly unsettled to active, slight chance of 
                isolated minor storm periods. 
30 Oct     7    Quiet to unsettled 
31 Oct     5    Quiet 
COMMENT: Geomagnetic activity may rise to active levels 
with some possibility of minor storm periods at times on 
29 October due to the effect of a high speed solar wind 
stream from a geoeffectively located coronal hole. Activity 
level is then expected to gradually decline to mostly 
unsettled and then quiet levels during the following two days. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
29 Oct      Fair-normal    Normal-fair    Normal-fair   
30 Oct      Fair-normal    Normal         Normal        
31 Oct      Fair-normal    Normal         Normal        
COMMENT: Pre-dawn depressions in MUFs on low latitudes may 
continue for the next few days. An expected rise in the 
geomagnetic activity levels on 29 October may result in 
minor to moderate depressions in MUFs and degradations in 
HF conditions on this day especially on high latitudes. 
Minor depressions in MUFs and degradations in HF conditions 
on these circuits may also be possible on 30 October. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
28 Oct    -2

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Depressed by 25% during local day,
      Depressed by 40% during local night.
      Enhanced by 20% after local dawn.
   Northern Australian Region:
      Depressed by 25% 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/Davis/Mawson):
      Near predicted monthly values over the UT day.

Predicted Monthly T index for October:  10

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
29 Oct    -6    near predicted monthly values/depressed 10 to 
                30% 
30 Oct    -3    near predicted monthly values/depressed 5 to 
                20% 
31 Oct    -2    Near predicted monthly values 
COMMENT: The pre-dawn depressions in MUFs on low latitudes, 
that are being observed for the last few days, are expected 
to continue for the next few days. HF conditions may show 
mild to moderate degradations on 29 October especially in 
the Southern Aus/NZ regions due to an expected rise in 
geomagnetic conditions during this period. Minor degradations 
in HF conditions in these regions may also be possible at 
times on 30 October. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 27 Oct
       Daily Proton Fluence >1 MeV:   2.3E+06
       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: A1.0

ACE Satellite Solar Wind Day Averaged Data for 27 Oct
Speed: 308 km/sec  Density:    5.4 p/cc  Temp:    15700 K  Bz:   0 nT

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