[Ips-dsgr] IPS Daily Report - 15 March 07

rwc rwc at ips.gov.au
Fri Mar 16 09:52:11 EST 2007


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 15/2330Z MARCH 2007 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 15 MARCH AND FORECAST FOR 16 MARCH - 18 MARCH
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 15 Mar:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 15 Mar:  69/3


1B. SOLAR FORECAST
             16 Mar             17 Mar             18 Mar
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    70/5               70/5               70/5
COMMENT: The visible solar disk remains spotless. Solar wind 
speeds have remained elevated over the past 24 hours due to a 
recurrent coronal hole wind stream. The speed has been declining 
less rapidly than expected but fell below 600km/s around 16UT. 
IMF Bz has been fluctuating widely but averaged slightly northward 
so merging was minimal. 

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 15 Mar: Quiet to Unsettled 

Estimated Indices 15 Mar :  A   K           
   Australian Region       7   12232212
      Darwin               0   00000000
      Townsville          10   22333222
      Learmonth            -   --------
      Camden               9   12333212
      Canberra             9   12333212
      Hobart               9   12333222
      Casey(Ant)          11   3--32223
    
Observed Regional daily pc3 Indices 15 Mar : 
      Darwin              NA
      Townsville           0   (Quiet)
      Learmonth            6   (Quiet)
      Camden              39   (Quiet to unsettled)
      Canberra            37   (Quiet to unsettled)
      Hobart              17   (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 15 Mar : A 
           Fredericksburg         5
           Planetary              8                         

Observed AFr/Ap Indices 14 Mar :  A   K
           Fredericksburg         9
           Planetary              8   3212 3221     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
16 Mar     8    Quiet to Unsettled 
17 Mar     4    Quiet 
18 Mar     3    Quiet 
COMMENT: Geomagnetic activity is expected to be quiet to unsettled 
for 16 March, trending to quiet as solar wind speed decreases 
with westward passage of the coronal hole. The decrease has been 
slower than expected. IMF Bz has fluctuated widely and averaged 
slightly northwards so merging has been weak and not contributed 
to global activity. Conditions should be mostly quiet for 17-18 
March. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
16 Mar      Normal         Normal         Normal-Fair
17 Mar      Normal         Normal         Normal
18 Mar      Normal         Normal         Normal
COMMENT: Mild depressions were observed during nightime hours 
during 15 March UT day at equatorial latitudes. Mid- latitudes 
looked to be returning to normal. Polar latitudes were only slightly 
disturbed from global geomagnetic activity and possibly the widely 
fluctuating IMF Bz. HF conditions should be returning to normal 
for 15 March with although recovery may be slow due to the absence 
of sunspots and ionising flux. Equatorial regions recovery may 
lag mid-latitudes. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
15 Mar     3

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Near predicted monthly values during local day,
      Depressed by 20% during local night.
      Niue showed an unusual daytime depression 01-05UT
      which was local.
   Northern Australian Region:
      Mostly near predicted monthly values,
   Southern Australian and New Zealand Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day.

Predicted Monthly T index for March:  10

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
16 Mar     6    about 5% below predicted monthly values 
17 Mar     8    Near predicted monthly values 
18 Mar    10    Near predicted monthly values 
COMMENT: HF conditions were mostly near normal for mid-latitudes 
with some slight depressions in the local evening. Equatorial 
latitudes showed MUF depressions of up to 20% during evening 
and local night, apparently a delayed reaction to the recent 
geogmetic activity. Conditions should be returning to normal 
for 15 March at mid latitudes with the continuing chance of equatorial
latitude depressions in MUF. Recovery is slow due to lack of 
sunspot activity and the solar wind declining less quickly than 
expected. Polar latitudes remain slightly disturbed and MUFs 
are volatile as usual. 
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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 14 Mar
       Daily Proton Fluence >1 MeV:   2.7E+06
       Daily Proton Fluence >10 MeV:  1.6E+04
       Daily Electron Fluence >2 MeV: 6.80E+07   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 8%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.0

ACE Satellite Solar Wind Day Averaged Data for 14 Mar
Speed: 666 km/sec  Density:    2.3 p/cc  Temp:   197000 K  Bz:   1 nT

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