[Ips-dsgr] IPS Daily Report - 05 December 09

rwc rwc at ips.gov.au
Sun Dec 6 10:47:00 EST 2009


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 05/2330Z DECEMBER 2009 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 05 DECEMBER AND FORECAST FOR 06 DECEMBER - 08 DECEMBER
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: ** YELLOW **
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 05 Dec:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 05 Dec:  72/8

1B. SOLAR FORECAST
             06 Dec             07 Dec             08 Dec
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    73/9               73/9               73/9
COMMENT: Solar activity stayed at very low levels over the last 
24 hours with no active regions on the visible disc. Solar wind 
speed remained low in the 230-260 km/s range till around 1500UT 
and then increased to around 370 km/s due to the onset of a
co-rotating interaction region. Interplanetary Magnetic Field 
IMF Bz component stayed close to normal value until around mid 
day and then showed fluctuations between +/-5nT. Solar activity 
is expected to stay mostly at quiet levels for the next three 
days. However some strengthening in the solar wind stream may 
continue on 06 December. 

-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 05 Dec: Mostly quiet, isolated
unsettled periods. 

Estimated Indices 05 Dec :  A   K           
   Australian Region       6   11321222
      Darwin               6   11211223
      Townsville           8   11322232
      Learmonth            6   01222232
      Canberra             2   00210112
      Hobart               5   01311122
      Casey(Ant)          10   12422223
    
Observed Regional daily pc3 Indices 05 Dec : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice_Springs        0   (Quiet)
      Gnangara             0   (Quiet)
      Canberra             0   (Quiet)
      Hobart               4   (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 05 Dec : A 
           Fredericksburg         2
           Planetary              5                         

Observed AFr/Ap Indices 04 Dec :  A   K
           Fredericksburg         0
           Planetary              0   0000 0000     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
06 Dec     4    Mostly quiet, isolated unsettled periods possible. 
07 Dec     3    Quiet 
08 Dec     2    Quiet 
COMMENT: Geomagnetic activity stayed mostly on quiet levels with 
some unsettled periods on 05 December. Similar conditions are 
expected on 06 decmber. Activity level is expected to decline 
to quiet levels on 7 and 8 December. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
06 Dec      Normal         Normal         Normal
07 Dec      Normal         Normal         Normal
08 Dec      Normal         Normal         Normal
COMMENT: HF conditions remained mostly normal on most 
locations on 05 December with some MUF depressions 
at low latitudes and blanketing by sporadic E layer on 
low and some mid latitude stations. No significant variation 
to the HF conditions is expected for the next three days. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
05 Dec   -25

Observed Australian Regional MUFs
   Cocos Island Region:
      Depressed by 30% during local day,
      Near predicted monthly values during local night.
   Niue Island Region:
      Depressed by 35% during local day,
      Near predicted monthly values during local night.
   Northern Australian Region:
      Depressed by 20% 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):
      Depressed by 15% over the UT day.

Predicted Monthly T index for December:   1

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
06 Dec   -24    near predicted monthly values/depressed 5 to 
                20% 
07 Dec   -24    near predicted monthly values/depressed 5 to 
                20% 
08 Dec   -24    near predicted monthly values/depressed 5 to 
                20% 
COMMENT: Some depressions in MUFs and blanketing by sporadic 
E-layer were observed in Aus/NZ regions on 05 December. No 
significant variations in HF conditions is expected for the 
next three days in this region. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 04 Dec
       Daily Proton Fluence >1 MeV:   4.7E+05
       Daily Proton Fluence >10 MeV:  2.0E+04
       Daily Electron Fluence >2 MeV: 5.40E+05   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.4

ACE Satellite Solar Wind Day Averaged Data for 04 Dec
Speed: 253 km/sec  Density:    0.3 p/cc  Temp:    14600 K  Bz:   0 nT

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