[Ips-dsgr] IPS Daily Report - 10 October 09

rwc rwc at ips.gov.au
Sun Oct 11 10:19:05 EST 2009


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 10/2330Z OCTOBER 2009 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 10 OCTOBER AND FORECAST FOR 11 OCTOBER - 13 OCTOBER
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 10 Oct:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 10 Oct:  70/5

1B. SOLAR FORECAST
             11 Oct             12 Oct             13 Oct
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    70/5               70/5               70/5
COMMENT: Solar activity remained at very low levels over 
the last 24 hours. Solar wind speed stayed between 250 
and 280 km/s for most parts of this period. The Bz component 
of the interplanetary magnetic field stayed mostly slightly 
negative (upto -2nT) during this period.The solar disc 
continues to remain spotless. Solar activity is expected to 
stay at very low levels for the next three days. However some 
strengthening in the solar wind stream is possible from 11 to 
13 October due to a recurrent pattern. 

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

Geomagnetic field for Australian Region 10 Oct: Quiet 

Estimated Indices 10 Oct :  A   K           
   Australian Region       3   11121111
      Darwin               2   11020002
      Townsville           5   12122112
      Learmonth            2   11020001
      Canberra             1   01020000
      Hobart               3   11121111
      Casey(Ant)           6   22321111
    
Observed Regional daily pc3 Indices 10 Oct : 
      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 10 Oct : A 
           Fredericksburg         2
           Planetary              5                         

Observed AFr/Ap Indices 09 Oct :  A   K
           Fredericksburg         1
           Planetary              3   0111 1111     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
11 Oct     4    Mostly quiet. Slight chance of isolated unsettled 
                periods. 
12 Oct     5    Mostly quiet. Slight chance of isolated unsettled 
                periods. 
13 Oct     5    Mostly quiet. Slight chance of isolated unsettled 
                periods. 
COMMENT: Geomagnetic conditions remained at quiet levels on 
10 October. Similar conditions may be expected for the next 
3 days with a  slight chance of isolated  unsettled periods 
during these days. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
11 Oct      Normal         Normal         Normal
12 Oct      Normal         Normal         Normal
13 Oct      Normal         Normal         Normal
COMMENT: HF conditions remained mostly at normal levels on 
most locations on 10 October. Wide spread sporadic E-layer 
on low and mid latitudes resulted in unexpected variations 
to HF conditions at these locations. HF conditions are expected 
to remain mostly normal on most locations for the next three 
days with a slight chance of isolated minor degradation periods 
at high latitudes during this period. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
10 Oct    -5

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

Predicted Monthly T index for October:   1

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
11 Oct    -4    near predicted monthly values 
12 Oct    -4    near predicted monthly values 
13 Oct    -4    near predicted monthly values 
COMMENT: HF conditions are expected to remain mostly normal 
across Aus/NZ regions for the next three days with slight 
possibility of isolated periods of minor degradations during 
this period in the southern parts of this region. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 09 Oct
       Daily Proton Fluence >1 MeV:   3.5E+05
       Daily Proton Fluence >10 MeV:  2.0E+04
       Daily Electron Fluence >2 MeV: 3.70E+04   (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 09 Oct
Speed: 300 km/sec  Density:    0.2 p/cc  Temp:    19000 K  Bz:  -2 nT

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


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