[Ips-dsgr] IPS Daily Report - 16 June 07

rwc rwc at ips.gov.au
Sun Jun 17 09:39:00 EST 2007


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 16/2330Z JUNE 2007 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 16 JUNE AND FORECAST FOR 17 JUNE - 19 JUNE
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 16 Jun:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 16 Jun:  68/2

1B. SOLAR FORECAST
             17 Jun             18 Jun             19 Jun
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 remained very low today. The effect 
of the coronal has further weakened. The solar wind speed 
gradaully decreased from 520 to 460 km/s over the UT day 
today. The north-south component of the interplanetary 
magnetic field (Bz) showed minor fluctuations between +/- 4 nT 
almost the whole day today. The effect of this coronal hole 
is expected to further weaken over the next 24 hours. A 
possible effect of another recurrent coronal hole may start 
to strengthen the solar wind stream from 19 June. Solar 
activity is expected to remain at very low levels for the 
next few days. 
-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 16 Jun: Quiet to Unsettled 

Estimated Indices 16 Jun :  A   K           
   Australian Region       7   13123211
      Darwin               5   22112212
      Townsville           8   23222222
      Learmonth            8   13223222
      Camden               5   12123110
      Canberra             4   12113110
      Hobart               6   13123111
      Casey(Ant)           8   23223221
    
Observed Regional daily pc3 Indices 16 Jun : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Camden              63   (Active)
      Canberra             4   (Quiet)
      Hobart              22   (Quiet to 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 16 Jun : A 
           Fredericksburg         7
           Planetary              7                         

Observed AFr/Ap Indices 15 Jun :  A   K
           Fredericksburg         7
           Planetary              8   2321 2212     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
17 Jun     5    Quiet 
18 Jun     4    Quiet 
19 Jun     8    Quiet to Unsettled 
COMMENT: Geomagnetic activity reamained mostly at quiet 
levels with some periods of unsettled levels recorded on 
16 June. Geomagnetic activity is expected to remain mostly 
at quiet levels on 17 and 18 June. Quiet to unsettled levels 
of geomagnetic activity may be expected on 19 June due the
possible effect of a recurrent coronal hole. 
-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
16 Jun      Normal-fair    Normal         Normal-fair    
PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
17 Jun      Normal         Normal         Normal
18 Jun      Normal         Normal         Normal
19 Jun      Normal         Normal         Normal-Fair
COMMENT: Minor to mild degradations in HF conditions and 
depressions in MUFs may be observed at high latitude on 
19 June due to some possibility of enhancement in geomagnetic 
activity levels on this day. HF conditions are expected to 
remain mostly normal on 17 and 18 June. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
16 Jun    10

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Depressed by 20% during local day with periods of 
      degradations,
      Near predicted monthly values during local night.
   Northern Australian Region:
      Near predicted monthly values.
   Southern Australian and New Zealand Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Enhanced by 15% over the UT day with periods of
      minor to significant depressions and degradations. .

Predicted Monthly T index for June:   9

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
17 Jun    12    Near predicted monthly values 
18 Jun    14    Near predicted monthly values 
19 Jun    14    Near predicted monthly values 
COMMENT: HF conditions are expected to remain mostly normal 
in most parts of Aus/NZ regions for the next three days with 
some possibility of minor degradations on some locations in 
the Southern Aus/NZ regions on 19 June due to some possibility 
of enhancement in geomagnetic activity levels on 19 June. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 15 Jun
       Daily Proton Fluence >1 MeV:   8.8E+05
       Daily Proton Fluence >10 MeV:  1.7E+04
       Daily Electron Fluence >2 MeV: 8.60E+06   (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 15 Jun
Speed: 574 km/sec  Density:    1.5 p/cc  Temp:   120000 K  Bz:   1 nT

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


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