[Ips-dsgr] IPS Daily Report - 26 January 11

rwc rwc at ips.gov.au
Thu Jan 27 10:44:04 EST 2011


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 26/2330Z JANUARY 2011 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 26 JANUARY AND FORECAST FOR 27 JANUARY - 29 JANUARY
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: ** YELLOW **
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 26 Jan:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 26 Jan:  80/20

1B. SOLAR FORECAST
             27 Jan             28 Jan             29 Jan
Activity     Very low to low    Very low to low    Very low to low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    79/19              78/17              76/14
COMMENT: Solar activity was very low today. Solar wind speed 
varied between 280 and 320 km/s and the Bz component of IMF 
varied between +/-5 nT during most parts of the UT day today. 
Very low to low levels of solar activity may be expected for 
the next three days. C-class activity may be possible during 
this period. 
-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 26 Jan: Quiet 

Estimated Indices 26 Jan :  A   K           
   Australian Region       4   21111121
      Darwin               5   21112222
      Townsville           -   --------
      Learmonth            4   11112221
      Canberra             2   11100111
      Hobart               2   11101110
      Casey(Ant)           9   33311131
    
Observed Regional daily pc3 Indices 26 Jan : 
      Darwin               0   (Quiet)
      Townsville          NA
      Learmonth            0   (Quiet)
      Alice_Springs        0   (Quiet)
      Gnangara             5   (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 26 Jan : A 
           Fredericksburg         2
           Planetary              3                         

Observed AFr/Ap Indices 25 Jan :  A   K
           Fredericksburg         3
           Planetary              4   2110 1112     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
27 Jan     3    Quiet 
28 Jan     3    Quiet 
29 Jan     3    Quiet 
COMMENT: Geomagnetic activity is expected to stay mostly at 
quiet levels for the next three days. 
-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
26 Jan      Normal-fair    Normal-fair    Normal-fair    
PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
27 Jan      Normal-fair    Normal-fair    Normal-fair   
28 Jan      Normal-fair    Normal-fair    Normal-fair   
29 Jan      Normal-fair    Normal-fair    Normal-fair   
COMMENT: Mostly normal to fair HF conditions were observed 
on most locations today. Continued very low levels of solar 
activity seems to be the reason behind this as less ionising 
radiation is reaching the ionoshere. Nearly similar HF conditions 
may be expected for the next 3 days as no significant variation 
to the ionospheric conditions is expected during this period. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date   T index
26 Jan     1

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values during local day,
      Depressed by 25% during local night.
   Niue Island Region:
      Near predicted monthly values during local day,
      Depressed by 25% during local night.
      Depressed by 25% after local dawn.
   Northern Australian Region:
      Depressed by 15% during local day,
      Depressed by 25% during local night.
      Depressed by 20% after local dawn.
   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):
      Depressed by 15% over the UT day.

Predicted Monthly T index for January:  37

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
27 Jan     1    near predicted monthly values/depressed 5 to 
                20% 
28 Jan     1    near predicted monthly values/depressed 5 to 
                20% 
29 Jan     1    near predicted monthly values/depressed 5 to 
                20% 
COMMENT: Mostly normal to fair HF conditions were observed 
in the Aus/NZ regions today. Continued very low levels of 
solar activity seems to be the reason behind continued 
depressions in MUFs as less ionising radiation is reaching 
the ionosphere due to very low solar activity. Nearly similar 
conditions may be expected in this region for the next three 
days as no significant variation to the ionospheric conditions 
is expected during this period. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 25 Jan
       Daily Proton Fluence >1 MeV:   2.5E+05
       Daily Proton Fluence >10 MeV:  1.4E+04
       Daily Electron Fluence >2 MeV: 4.00E+06   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A5.7

ACE Satellite Solar Wind Day Averaged Data for 25 Jan
Speed: 328 km/sec  Density:    4.8 p/cc  Temp:    27800 K  Bz:  -3 nT

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


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