[Ips-dsgr] IPS Daily Report - 02 June 09

rwc rwc at ips.gov.au
Wed Jun 3 09:24:04 EST 2009


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 02/2330Z JUNE 2009 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 02 JUNE AND FORECAST FOR 03 JUNE - 05 JUNE
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 02 Jun:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 02 Jun:  72/8


1B. SOLAR FORECAST
             03 Jun             04 Jun             05 Jun
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    72/8               72/8               72/8
COMMENT: Solar activity was very low over the last 24 hours. 
Region 1019(N28E15) produced a B-class flare. The solar wind 
speed stayed around 300 km/s for most parts of the UT day today. 
The Bz component of the interplanetary magnetic field stayed 
close to the normal value (between +/-2nT) for most parts of 
the UT day today. Solar activity is expected to stay at very 
low levels for the next 3 days. However, the solar wind stream 
may get strengthened on 3 and 4 June due to an anticipated 
recurrent coronal hole effect. 
-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 02 Jun: Quiet 

Estimated Indices 02 Jun :  A   K           
   Australian Region       1   11010001
      Darwin               2   12110001
      Townsville           7   22------
      Learmonth            0   10010000
      Camden               0   01000001
      Canberra             0   00------
      Hobart               0   00000000
      Casey(Ant)           3   11------
    
Observed Regional daily pc3 Indices 02 Jun : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice_Springs        0   (Quiet)
      Camden               2   (Quiet)
      Gnangara             0   (Quiet)
      Canberra             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 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 02 Jun : A 
           Fredericksburg         2
           Planetary              4                         

Observed AFr/Ap Indices 01 Jun :  A   K
           Fredericksburg         2
           Planetary              3   1110 1111     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
03 Jun     7    Quiet to Unsettled 
04 Jun     7    Quiet to Unsettled 
05 Jun     5    Quiet 
COMMENT: Geomagnetic activity remained at quiet levels 
today. Geomagnetic activity is expected to rise to quiet 
to unsettled levels on 03 and 04 June due to an anticipated 
strengthening in the solar wind stream due to the effect of 
a recurrent coronal hole. Activity level is expected to decline 
to quiet levels on 05 June. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
03 Jun      Normal         Normal-fair    Normal-fair   
04 Jun      Normal         Normal-fair    Normal-fair   
05 Jun      Normal         Normal         Normal        
COMMENT: HF conditions were mostly normal on most locations 
on 02 June although sporadic E-layers and spread F conditions 
were also observed at times. HF conditions may show minor 
degradations on high and some mid latitude locations on 03 
and 04 June due to an anticipated slight rise in geomagnetic 
activity levels on these days. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
Date   T index
02 Jun    -5

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Depressed by 15% during local day,
      Depressed by 45% during local night.
   Northern Australian Region:
      Near predicted monthly values.
   Southern Australian and New Zealand Region:
      Near predicted monthly values during local day,
      Enhanced by 30% during local night.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day.

Predicted Monthly T index for June:   5

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
03 Jun     0    near predicted monthly values/depressed 5 to 
                15% 
04 Jun     0    near predicted monthly values/depressed 5 to 
                15% 
05 Jun     2    near predicted monthly values 
COMMENT: HF conditions are expected to remain mostly normal 
on most locations across Aus/NZ regions for the next three 
days with the possibility of minor degradations in the Southern 
parts of this regions on 03 and 04 June due to an anticipated 
slight rise in geomagnetic activity on these days. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 01 Jun
       Daily Proton Fluence >1 MeV:   4.7E+05
       Daily Proton Fluence >10 MeV:  2.0E+04
       Daily Electron Fluence >2 MeV: 9.90E+04   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.3

ACE Satellite Solar Wind Day Averaged Data for 01 Jun
Speed: 320 km/sec  Density:    0.7 p/cc  Temp:    36400 K  Bz:   0 nT

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


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