[Ips-dsgr] IPS Daily Report - 27 October 06

rwc rwc at ips.gov.au
Sat Oct 28 09:47:00 EST 2006


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 27/2330Z OCTOBER 2006 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 27 OCTOBER AND FORECAST FOR 28 OCTOBER - 30 OCTOBER
STATUS INDICATORS SOL:GREEN   MAG:** YELLOW **     ION: ** YELLOW **
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1A. SOLAR SUMMARY
Activity 27 Oct:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 27 Oct:  72/8

1B. SOLAR FORECAST
             28 Oct             29 Oct             30 Oct
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 remained at very low levels today 
as well. Solar wind speed gradually decreased from 360 to 
290 km/s by around 1700UT and then showed a gradual increase 
to 340 km/s by around 2300UT. This increase in the solar 
wind speed may have been caused by the anticipated effect 
of the coronal hole that is currently taking a geoeffective 
position. The solar wind stream may remain strengthened due 
to the effect of this coronal hole for the next 48 hours. 
The north-south component of the interplanetary magnetic 
field (Bz) remained close to the normal value until around 
1700UT and then showed minor to moderate (upto +5 and -7 nT) 
fluctuations on both sides of the normal value during the 
rest of the UT day. Solar activity is expected to remain 
very low for the next few days. 

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 27 Oct: Quiet to Unsettled 

Estimated Indices 27 Oct :  A   K           
   Australian Region       6   21112123
      Darwin               6   22111123
      Learmonth            5   21011123
      Culgoora             5   11112123
      Camden               4   11112013
      Canberra             5   11022113
      Hobart               3   11112012
      Casey(Ant)           9   33311123
    
Observed Regional daily pc3 Indices 27 Oct : 
      Charters_Towers      0   (Quiet)
      Learmonth            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. 


Estimated AFr/Ap Indices 27 Oct : A 
           Fredericksburg         5
           Planetary             10                         

Observed AFr/Ap Indices 26 Oct :  A   K
           Fredericksburg         1
           Planetary              1   0010 1000     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
28 Oct    20    Unsettled to active, minor storm periods possible. 
29 Oct    14    Unsettled to active 
30 Oct     8    Quiet to unsettled 
COMMENT: IPS Geomagnetic Warning 14 was issued on 25 October 
and is current for interval 26-28 October. Geomagnetic 
activity may rise to active to minor storm levels on 28 
October due to an expected effect of a high speed solar 
wind stream from a recurrent coronal hole. The activity 
level is then expected to gradually subside to unsettled 
to active levels on 29 October and quiet to unsettled on 
30 October. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
28 Oct      Fair           Fair           Fair          
29 Oct      Fair-normal    Fair-normal    Fair          
30 Oct      Fair-normal    Normal         Normal-fair   
COMMENT: Pre-dawn depressions in MUFs may continue for the 
next few days. An expected rise in the geomagnetic activity 
levels late on 28 October may result in minor to moderate 
depressions in MUFs and degradations in HF conditions on 
this day. Minor depressions in MUFs and degradations in HF 
conditions may also be possible on 29 October. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
27 Oct   -11

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Depressed by 25% during local day,
      Depressed by 50% during local night.
   Northern Australian Region:
      Depressed by 30% during local day,
      Depressed by 20% during local night.
   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.

Predicted Monthly T index for October:  10

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
28 Oct   -12    near predicted monthly values/depressed 10 to 
                40% 
29 Oct    -7    near predicted monthly values/depressed 10 to 
                30% 
30 Oct    -3    near predicted monthly values/depressed 5 to 
                20% 
COMMENT: The pre-dawn depressions in MUFs, 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 28 and possibly 29 October due to 
an expected rise in geomagnetic activity during this period. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 26 Oct
       Daily Proton Fluence >1 MeV:   1.6E+06
       Daily Proton Fluence >10 MeV:  1.6E+04
       Daily Electron Fluence >2 MeV: 1.70E+08 (moderate fluence)  
Electron Fluence Daily Deep Dielectric Discharge Probability:14%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A2.7

ACE Satellite Solar Wind Day Averaged Data for 26 Oct
Speed: 394 km/sec  Density:    3.4 p/cc  Temp:    48900 K  Bz:   0 nT

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