[Ips-dsgr] IPS Daily Report - 30 May 08

rwc rwc at ips.gov.au
Sat May 31 09:42:34 EST 2008


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 30/2330Z MAY 2008 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 30 MAY AND FORECAST FOR 31 MAY - 02 JUNE
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 30 May:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 30 May:  67/0


1B. SOLAR FORECAST
             31 May             01 Jun             02 Jun
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    68/2               68/2               68/2
COMMENT: The visible disk is presently spotless. Solar wind speeds 
ranged from approximately 470 km/s up to 670 km/s during the 
past 24 hours under the influence of a coronal hole wind stream 
and are presently approximately 550 km/s. Solar wind speeds are 
expected to remain mildly elevated over the next couple of days. 




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

Geomagnetic field for Australian Region 30 May: Quiet to Unsettled 

Estimated Indices 30 May :  A   K           
   Australian Region       8   32222321
      Darwin               7   22212321
      Townsville           9   32222322
      Learmonth           10   31223332
      Camden               6   21112321
      Canberra             7   31112321
      Hobart               6   -1122321
      Casey(Ant)          14   33323342
    
Observed Regional daily pc3 Indices 30 May : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            4   (Quiet)
      Alice_Springs        0   (Quiet)
      Culgoora            14   (Quiet)
      Camden              39   (Quiet to unsettled)
      Gnangara            62   (Active)
      Canberra            27   (Quiet to unsettled)
      Hobart              54   (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 30 May : A 
           Fredericksburg         8
           Planetary              8                         

Observed AFr/Ap Indices 29 May :  A   K
           Fredericksburg         7
           Planetary              9   3321 2222     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
31 May    12    Mostly quiet to unsettled with the small chance 
                of isolated active periods and storm levels at 
                high latitudes. 
01 Jun    10    Mostly quiet to unsettled with the small chance 
                of isolated active periods and storm levels at 
                high latitudes. 
02 Jun     8    Quiet to unsettled 
COMMENT: Mostly quiet to unsettled levels have been observed 
across the Australian region during the past 24 hours with isolated 
active to storm levels at high latitudes. Mostly quiet to unsettled 
levels are expected for the next few days with isolated active 
and storm levels possible at high latitudes for 31 May - 1 June 
due to the influence of a coronal hole solar wind stream. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
31 May      Normal         Normal         Normal-Fair
01 Jun      Normal         Normal         Normal-Fair
02 Jun      Normal         Normal         Normal-Fair

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


Date   T index
30 May     5

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Depressed by 15% during local day,
      Near predicted monthly values 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):
      Mostly near predicted monthly values.

Predicted Monthly T index for May:   6

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
31 May     0    near predicted monthly values/depressed 5 to 
                15% 
01 Jun     0    near predicted monthly values/depressed 5 to 
                15% 
02 Jun     5    Near predicted monthly values 
COMMENT: Depressions of 5-15% were observed at times across the 
Aus/NZ region, otherwise MUFs were mostly near predicted monthly 
values during the past 24 hours. Mostly normal conditions are 
expected for the next few days with isolated depressions of 5-15% 
possible at times. Spread-F and Sporadic-E conditions were observed 
at times at most stations across the Aus/NZ region during 30 
May and are possible at times during the next few days. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 29 May
       Daily Proton Fluence >1 MeV:   7.5E+05
       Daily Proton Fluence >10 MeV:  1.7E+04
       Daily Electron Fluence >2 MeV: 1.10E+07   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 2%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.0

ACE Satellite Solar Wind Day Averaged Data for 29 May
Speed: 474 km/sec  Density:    4.3 p/cc  Temp:   100000 K  Bz:   1 nT

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