[Ips-dsgr] IPS Daily Report - 12 September 09

rwc rwc at ips.gov.au
Sun Sep 13 09:46:13 EST 2009


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 12/2330Z SEPTEMBER 2009 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 12 SEPTEMBER AND FORECAST FOR 13 SEPTEMBER - 15 SEPTEMBER
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 12 Sep:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 12 Sep:  69/3

1B. SOLAR FORECAST
             13 Sep             14 Sep             15 Sep
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    69/3               68/2               68/2
COMMENT: Solar activity was very low over the last 24 hours. 
The visible disk remains spotless. Solar wind speed stayed 
between 300 and 340 km/s for most parts of the UT day today. 
The Bz component of the interplanetary magnetic field stayed 
between +/- 4 nT almost the whole day today. Some strengthening 
in solar wind stream may be observed on 14 and 15 September due 
to a recurrent pattern. Solar activity is expected to stay at 
very low levels for the next 3 days. 
-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 12 Sep: Quiet 

Estimated Indices 12 Sep :  A   K           
   Australian Region       3   11111111
      Darwin               2   11100102
      Townsville           5   12211222
      Learmonth            1   11001101
      Canberra             0   00011000
      Hobart               3   11122101
      Casey(Ant)           5   23211111
    
Observed Regional daily pc3 Indices 12 Sep : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice_Springs        0   (Quiet)
      Gnangara             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 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 12 Sep : A 
           Fredericksburg         3
           Planetary              5                         

Observed AFr/Ap Indices 11 Sep :  A   K
           Fredericksburg         2
           Planetary              4   0111 1112     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
13 Sep     3    Quiet 
14 Sep     6    Moslty quiet, isolated unsettled periods possible. 
15 Sep     9    Quiet to unsettled 
COMMENT: The geomagnetic field was quiet over the last 24 
hours. Similar conditions are expected on 13 September. 
Isolated unsettled periods may be observed on 14 September 
and quiet to unsettled conditions are expected for 15 September. 
This rise in geomagnetic conditions is expected due to a 
recurrent pattern. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
13 Sep      Normal         Normal         Normal
14 Sep      Normal         Normal         Normal
15 Sep      Normal         Normal         Normal-Fair
COMMENT: HF conditions remained mostly normal on most locations 
on 12 September with periods of presence of strong sporadic 
E-layer on low latitudes. Mostly normal HF conditions may be 
expected on most locations for the next three days with the 
possibility of minor to moderate degradations on high latitudes 
on 15 Septebmer. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
12 Sep    -7

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Near predicted monthly values during local day,
      Depressed by 20% during local night.
   Northern Australian Region:
      Near predicted montly values to depressed by 
      15% during local day,
      Depressed by 25% during local night.
   Southern Australian and New Zealand Region:
      Near predicted monthly values during local day,
      Enhanced by 30% during local night.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day.

Predicted Monthly T index for September:   0

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
13 Sep    -5    Near predicted monthly values 
14 Sep    -6    Near predicted monthly values 
15 Sep    -8    Mostly near predicted monthly values, minor
		depressions possible in southern regions. 
COMMENT: HF conditions remained mostly normal across Aus/NZ 
regions on 12 September. Similar HF conditions may be expected 
for the next 3 days with small possibility of isolated periods 
of minor MUF depressions in the Southern Aus/NZ regions on 
15 September. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 11 Sep
       Daily Proton Fluence >1 MeV:   6.5E+05
       Daily Proton Fluence >10 MeV:  2.0E+04
       Daily Electron Fluence >2 MeV: 1.30E+05   (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 11 Sep
Speed: 302 km/sec  Density:    1.8 p/cc  Temp:    27700 K  Bz:  -2 nT

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


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