[Ips-dsgr] IPS Daily Report - 10 March 08

rwc rwc at ips.gov.au
Tue Mar 11 10:44:26 EST 2008


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 10/2330Z MARCH 2008 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 10 MARCH AND FORECAST FOR 11 MARCH - 13 MARCH
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: ** YELLOW **
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1A. SOLAR SUMMARY
Activity 10 Mar:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 10 Mar:  70/5


1B. SOLAR FORECAST
             11 Mar             12 Mar             13 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: Solar activity was Very Low over the last 24 hours, 
and expected to continue at this level. Solar wind speeds remain 
elevated at 620-680km/sec, due to a high speed coronal hole wind 
stream. The Interplanetary Magnetic Field (IMF) had large fluctuations

in the wake of the Co-rotating Interaction Region (CIR) and IMF 
sector boundary crossing. IMF Bz had no north-south preference 
and varied +/-4nT. The size of the coronal hole and also recurrence 
patterns suggests elevated solar wind speeds can be expected 
for the next 4-5 days. However the IMF fluctuations should decrease 
later in this interval, resulting in less geoeffective conditions. 




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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 10 Mar: Quiet to Unsettled 

Estimated Indices 10 Mar :  A   K           
   Australian Region      12   33233223
      Darwin               8   23123222
      Townsville          12   33223233
      Learmonth           13   43233223
      Camden              12   33233223
      Canberra            12   33233223
      Hobart              11   33233222
      Casey(Ant)          16   34-33333
    
Observed Regional daily pc3 Indices 10 Mar : 
      Darwin               2   (Quiet)
      Townsville           3   (Quiet)
      Learmonth           NA
      Canberra            62   (Active)
      Hobart              48   (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 10 Mar : A 
           Fredericksburg        10
           Planetary             15                         

Observed AFr/Ap Indices 09 Mar :  A   K
           Fredericksburg        14
           Planetary             25   4553 3224     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
11 Mar    12    Unsettled 
12 Mar    10    Quiet to Unsettled 
13 Mar     8    Quiet to Unsettled 
COMMENT: The geomagnetic field was variable, from Quiet to Active 
at mid and equatorial latitudes, in response to elevated solar 
wind speed from the recurrent coronal hole wind stream. The high 
latitudes varied from Unsettled to Minor Storm levels, responding 
more directly to the strong IMF fluctuations (see solar section) 
than mid/low latitudes. The general trend is toward less disturbed 
conditions than yesterday. The coronal hole is likely to produce 
further Unsettled conditions over the next two days (11-12 March) 
with possible Active periods at mid/low latitudes and Minor Storm 
conditions at high latitudes especially if prolonged Bz southwards 
occurs after IMF fluctuations settle. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
11 Mar      Normal         Normal         Normal-Fair
12 Mar      Normal         Normal         Normal-Fair
13 Mar      Normal         Normal         Normal-Fair

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
10 Mar   -16

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Near predicted monthly values.
   Northern Australian Region:
      Depressed by 15% during local day,
      Near predicted monthly values during local night.
   Southern Australian and New Zealand Region:
      Depressed by 30% during local day,
      Near predicted monthly values during local night.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day.

Predicted Monthly T index for March:   6

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
11 Mar   -15    10 to 20% below predicted monthly values 
12 Mar   -10    5 to 15% below predicted monthly values 
13 Mar     0    0 to 5% below predicted monthly values 
COMMENT: IPS HF Communications Warning 9 was issued on 10 March 
and is current for interval 10-11 March. MUFs were up to 30% 
depressed compared with monthly values over the UT day due to 
geomagnetic activity from the recurrent solar coronal hole high-speed 
solar-wind stream. Large enhancement and depressions at equatorial 
latitudes. Expect further but less deep MUF depressions 11-12 
March but otherwise mostly normal HF conditions. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 09 Mar
       Daily Proton Fluence >1 MeV:   1.2E+06
       Daily Proton Fluence >10 MeV:  1.7E+04
       Daily Electron Fluence >2 MeV: 1.80E+06   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 0%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.0

ACE Satellite Solar Wind Day Averaged Data for 09 Mar
Speed: 592 km/sec  Density:    7.5 p/cc  Temp:   234000 K  Bz:   1 nT

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