[Ips-dsgr] IPS Daily Report - 28 February 07

rwc rwc at ips.gov.au
Thu Mar 1 10:33:26 EST 2007


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 28/2330Z FEBRUARY 2007 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 28 FEBRUARY AND FORECAST FOR 01 MARCH - 03 MARCH
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 28 Feb:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 28 Feb:  76/14


1B. SOLAR FORECAST
             01 Mar             02 Mar             03 Mar
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    75/13              75/13              75/13

COMMENT: Solar activity is expected to remain at very low levels 
over the next several days. The Bz component of the interplanetary 
magnetic field has mostly fluctuated between +/-5nT for the last 
24 hours. The solar wind speed ranged bewteen 600-700km/s over 
the period, elevated due to a recurrent solar coronal hole. Solar 
wind speeds are expected to remain elevated but slowly decline 
over the next 3 days. 

-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 28 Feb: Unsettled to Active 

Estimated Indices 28 Feb :  A   K           
   Australian Region      18   34433333
      Darwin              12   33333222
      Townsville          15   33343233
      Learmonth           21   44443333
      Canberra            15   34433222
      Casey(Ant)          19   34433433
    
Observed Regional daily pc3 Indices 28 Feb : 
      Darwin               0   (Quiet)
      Townsville           2   (Quiet)
      Learmonth            0   (Quiet)
      Camden               0   (Quiet)
      Canberra            54   (Unsettled)
      Hobart              63   (Active)
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 Feb : A 
           Fredericksburg        15
           Planetary             20                         

Observed AFr/Ap Indices 27 Feb :  A   K
           Fredericksburg         7
           Planetary             12   0032 1343     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
01 Mar    10    Quiet to Unsettled. Active periods at high latitudes 
02 Mar     6    Quiet 
03 Mar     5    Quiet 

COMMENT: A recurrent coronal hole remains in geoeffective position 
producing yesterday's (28 Feb) unsettled geomagnetic conditions. 
Minor storm conditions were observed at high latitudes. Expect 
geomagnetic activity to return to Quiet to Unsettled levels with 
isolated Active periods at high latitudes today (29 Feb) and 
tomorrow. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
01 Mar      Normal         Normal         Normal-Fair
02 Mar      Normal         Normal         Normal
03 Mar      Normal         Normal         Normal

COMMENT: Despite increased geomagnetic activity, ionospheric 
conditions remained mostly normal. Strong enhancements occurred 
in the equatorial/PNG and Northern Australian regions, particularly 
over the local night. Minor depressions occurred over the Antarctic 
regions. Expect mostly normal HF conditions to prevail in the 
Australian region with further equatorial enhancements likely. 

-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
28 Feb    39

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Near predicted monthly values during local day,
      Enhanced by 30% during local night.
   Northern Australian Region:
      Near predicted monthly values during local day,
      Enhanced by 25% during local night.
   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 February:  11

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
01 Mar    25    Mostly near predicted monthly values / variably 
                enhanced at equatorial latitudes 
02 Mar    20    Near predicted monthly values / enhanced 10% 
03 Mar    20    Near predicted monthly values / enhanced 10% 

COMMENT: HF conditions remain mostly normal. Some strong enhancements 
occurred at low latitudes, particularly over the local night. 
Minor depressions occurred at high latitudes due to enhanced 
geomagnetic activity. Expect mostly normal HF conditions to prevail 
with further equatorial enhancements and isolated high latitude 
depressions likely. 

-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 27 Feb
       Daily Proton Fluence >1 MeV:   2.0E+06
       Daily Proton Fluence >10 MeV:  1.6E+04
       Daily Electron Fluence >2 MeV: 2.90E+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 27 Feb
Speed: 397 km/sec  Density:    4.2 p/cc  Temp:   124000 K  Bz:   0 nT

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