[Ips-dsgr] IPS Daily Report - 27 February 06

rwc rwc at ips.gov.au
Tue Feb 28 10:04:52 EST 2006


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 27/2330Z FEBRUARY 2006 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 27 FEBRUARY AND FORECAST FOR 28 FEBRUARY - 02 MARCH
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 27 Feb:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 27 Feb:  77/16


1B. SOLAR FORECAST
             28 Feb             01 Mar             02 Mar
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 continues to be very low. The new region 
on the SE limb AR856 continues to produce low-level B class flares 
and may produce C flares. Solar wind speed is average 320-360 
km/sec and shows no sign yet of recurrent coronal hole activity 
that may occur on the 28th. IMF Bz drifted back towards zero 
for 04-17UT and then northward for 12-17UT, effectively shutting 
off merging of geomagnetic and solar fields after the prolonged 
southward period. After a brief excursion southward 17-21UT it 
has now returned northward to +5nT so merging with the geomagnetic 
field is again turned off. 




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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 27 Feb: Quiet 

Estimated Indices 27 Feb :  A   K           
   Australian Region       3   22112001
      Darwin               3   11112---
      Learmonth            2   21002001
      Culgoora             1   -1002001
      Camden               4   22112011
      Canberra             2   11002001
      Hobart               2   12102001
      Casey(Ant)           8   33322011
    
Observed Regional daily pc3 Indices 27 Feb : 
      Canberra             0   (Quiet)
      Learmonth            0   (Quiet)
      Culgoora             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. 


Estimated AFr/Ap Indices 27 Feb : A 
           Fredericksburg         5
           Planetary              5                         

Observed AFr/Ap Indices 26 Feb :  A   K
           Fredericksburg         3
           Planetary              5   0210 1212     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
28 Feb     8    Quiet to Unsettled 
01 Mar     5    Quiet 
02 Mar     5    Quiet 
COMMENT: Solar wind speed continues at average levels so the 
geomagnetic field is not being affected (see solar report). A 
recurrent coronal hole wind speed increase is possible on the 
28th but shows no sign as yet, late on the 27th. Prolonged (~20hrs) 
magnetic merging of the southwards solar IMF Bz and geomagnetic 
fields was shut off ~04UT by Bz tending to zero and then northwards 
for 14 hours till 18UT. This prevented the enhanced polar magnetic 
activity expanding globally. IMF now looks strongly northwards 
to the field is expected to remain at Quiet levels. 


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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
27 Feb      Normal         Normal         Fair-normal    
PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
28 Feb      Normal         Normal         Normal-Fair
01 Mar      Normal         Normal         Normal
02 Mar      Normal         Normal         Normal
COMMENT: Propagation conditions should be normal for the next 
three days in the absence of significant geomagnetic activity, 
apart from localised sporadic E or spread F conditions where 
they are usually prone. High latitude conditions may continue 
fair but improve on the 28th during recovery from the prolonged 
which caused polar ionospheric convection. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
27 Feb    16

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Near predicted monthly values. Dusk enhancements noted
      at PNG (Vanimo, Pt Moresby) and Western Pacific (Niue).
   Northern Australian Region:
      Near predicted monthly values.
   Southern Australian and New Zealand Region:
      Near predicted monthly values. Spread F observed overnight
      in the Southern Ocean at Christchurch and MacQuarie Is.
      Strong sporadic E was also observed overnight at
      Hobart.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day. Strong
      Spread F observd inside the polar cap at Casey due to
      ionospheric convection resulting from prolonged
      ~20hr southward IMF Bz merging with the geomagnetic
      field.

Predicted Monthly T index for February:  16

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
28 Feb    15    ÿon.forecast 
01 Mar    12    Near predicted monthly values 
02 Mar    14    Near predicted monthly values 
COMMENT: Conditions average at low and mid latitudes. Conditions 
improving at higher latitudes after prolonged merging (~20hrs) 
with the solar IMF, which drove polar cap ionospheric convection, 
was shut off by Bz turning zero to northwards for several hours. 
Overall conditions expected to be average apart from local sporadic 
E and spread F. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 26 Feb
       Daily Proton Fluence >1 MeV:   7.7E+05
       Daily Proton Fluence >10 MeV:  1.6E+04
       Daily Electron Fluence >2 MeV: 1.70E+08 (moderate fluence)  
Electron Fluence Daily Deep Dielectric Discharge Probability:14%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A2.1

ACE Satellite Solar Wind Day Averaged Data for 26 Feb
Speed: 362 km/sec  Density:    2.7 p/cc  Temp:    67700 K  Bz:  -2 nT

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