[Ips-dsgr] IPS Daily Report - 26 July 07

rwc rwc at ips.gov.au
Fri Jul 27 09:44:42 EST 2007


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 26/2330Z JULY 2007 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 26 JULY AND FORECAST FOR 27 JULY - 29 JULY
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 26 Jul:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 26 Jul:  68/2


1B. SOLAR FORECAST
             27 Jul             28 Jul             29 Jul
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 was very low over the last 24 hours. 
With no active regions currently on the disk, solar activity 
is expected to remain very low for the next few days. Solar wind 
velocity began to increase at 1050UT from 300km/s to be ~460km/s 
at the time of this report. Bz, the north-south component of 
the interplanetary magnetic field increased in magnitude to fluctuate 
between +/-10nT for the later half of the UT day. The rise in 
solar wind paramters is due to a the onset of a high speed solar 
wind stream from a recurrent coronal hole. 




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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 26 Jul: Quiet to Unsettled 

Estimated Indices 26 Jul :  A   K           
   Australian Region       5   11111322
      Darwin               6   21112322
      Townsville           8   22212332
      Learmonth            6   12112322
      Camden               4   11001321
      Canberra             4   00001322
      Hobart               5   21101322
      Casey(Ant)           4   11111222
    
Observed Regional daily pc3 Indices 26 Jul : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Camden               4   (Quiet)
      Canberra             0   (Quiet)
      Hobart              35   (Quiet to unsettled)
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 Jul : A 
           Fredericksburg        10
           Planetary             15                         

Observed AFr/Ap Indices 25 Jul :  A   K
           Fredericksburg         2
           Planetary              2   0001 1110     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
27 Jul    12    Unsettled 
28 Jul     8    Quiet to Unsettled 
29 Jul     8    Quiet to Unsettled 
COMMENT: Geomagnetic activity was Quiet to Unsettled over the 
last 24 hours as the earth entered a high speed solar wind stream 
from the now geoeffective coronal hole. Predominently Unsettled 
geomagnetic conditions expected over the next 24 hours with possible 
Active periods. Quiet to Unsettled conditions expected for
28Jul-29Jul. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
27 Jul      Normal-fair    Normal-fair    Fair-poor     
28 Jul      Normal-fair    Normal-fair    Normal-fair   
29 Jul      Normal-fair    Normal         Normal-fair   
COMMENT: Depressed periods observed for low latitudes and disturbed 
conditions for high latitudes. Mostly normal conditions observed 
for mid latitudes. Similar conditions expected for low latitudes 
over the next 2 days with MUF depressions ~20% expected for mid 
to high latitudes due to increase in geomagnetic activity. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
26 Jul     1

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Mostly near predicted monthly values,
      Depressed by 20% after local dawn.
   Northern Australian Region:
      Depressed by 15% 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):
      Enhanced by 315% over the UT day.

Predicted Monthly T index for July:  10

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
27 Jul     0    near predicted monthly values/depressed 10 to 
                20% 
28 Jul     0    near predicted monthly values/depressed 10 to 
                20% 
29 Jul     5    near predicted monthly values/depressed 10 to 
                20% 
COMMENT: Depressed conditions observed after local dawn for both 
Northern AUS/Equatorial regions and Southern AUS/NZ regions, 
otherwise mostly normal ionospheric support. Enhanced periods 
along with disturbed conditions observed for Antarctic regions. 
Similar conditions are expected for the next 2 days with possible 
MUF depressions of 20% for Southern AUS/NZ and Antarctic regions 
due to an increase in geomagnetic activity. 
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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 25 Jul
       Daily Proton Fluence >1 MeV:   7.6E+05
       Daily Proton Fluence >10 MeV:  1.7E+04
       Daily Electron Fluence >2 MeV: 1.40E+07   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 3%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.0

ACE Satellite Solar Wind Day Averaged Data for 25 Jul
Speed: 313 km/sec  Density:    3.8 p/cc  Temp:    18200 K  Bz:   1 nT

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