[Ips-dsgr] IPS Daily Report - 28 January 11

rwc rwc at ips.gov.au
Sat Jan 29 10:14:11 EST 2011


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 28/2330Z JANUARY 2011 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 28 JANUARY AND FORECAST FOR 29 JANUARY - 31 JANUARY
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: ** YELLOW **
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 28 Jan:  Moderate

Flares    Max     Fadeout    Freq.  Sectors
 M1/--    0103UT  possible   lower  West Pacific

Observed 10.7 cm flux/Equivalent Sunspot Number for 28 Jan:  81/22


1B. SOLAR FORECAST
             29 Jan             30 Jan             31 Jan
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    80/20              80/20              80/20
COMMENT: Solar activity was moderate today. Region 1149 produced 
an M1 flare at 0103 UT and two C1 flares that respectively peaked 
at 0435 and 1022 UT. The M1 flare was associated with a Type II 
radio sweep and a CME with its speed estimated as 900 km/s 
by Culgoora observatory. This CME is not earthward directed. 
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 levels of solar activity with some 
possibility of C-class activity may be expected for the next 
three days. 
-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 28 Jan: Quiet 

Estimated Indices 28 Jan :  A   K           
   Australian Region       4   22111211
      Darwin               6   32111212
      Townsville           -   --------
      Learmonth            7   32112312
      Canberra             2   11011210
      Hobart               3   11011211
      Casey(Ant)           9   3-322222
    
Observed Regional daily pc3 Indices 28 Jan : 
      Darwin               0   (Quiet)
      Townsville          NA
      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 28 Jan : A 
           Fredericksburg         4
           Planetary              5                         

Observed AFr/Ap Indices 27 Jan :  A   K
           Fredericksburg         2
           Planetary              3   1011 1120     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
29 Jan     3    Quiet 
30 Jan     3    Quiet 
31 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 
28 Jan      Normal-fair    Normal-fair    Normal-fair    
PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
29 Jan      Normal-fair    Normal-fair    Normal-fair   
30 Jan      Normal-fair    Normal-fair    Normal-fair   
31 Jan      Normal-fair    Normal-fair    Normal-fair   
COMMENT: Mostly normal to fair HF conditions were observed 
on most locations today. 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
28 Jan     7

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values during local day,
      Depressed by 35% during local night.
   Niue Island Region:
      Mostly near predicted monthly values,
      Depressed by 20% after local dawn.
   Northern Australian Region:
      Depressed by 25% during local day,
      Depressed by 15% during local night.
   Southern Australian and New Zealand Region:
      Depressed by 25% 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
29 Jan     3    near predicted monthly values/depressed 5 to 
                20% 
30 Jan     3    near predicted monthly values/depressed 5 to 
                20% 
31 Jan     3    near predicted monthly values/depressed 5 to 
                20% 
COMMENT: Mostly normal to fair HF conditions were observed 
in the Aus/NZ regions today alongwith the presence of sporadic 
E-layers at times. 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 27 Jan
       Daily Proton Fluence >1 MeV:   2.2E+05
       Daily Proton Fluence >10 MeV:  1.5E+04
       Daily Electron Fluence >2 MeV: 2.90E+06   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A7.2

ACE Satellite Solar Wind Day Averaged Data for 27 Jan
Speed: 298 km/sec  Density:    1.8 p/cc  Temp:    27300 K  Bz:   0 nT

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


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