[Ips-dsgr] IPS Daily Report - 14 June 09

rwc rwc at ips.gov.au
Mon Jun 15 09:49:24 EST 2009


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 14/2330Z JUNE 2009 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 14 JUNE AND FORECAST FOR 15 JUNE - 17 JUNE
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 14 Jun:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 14 Jun:  68/2


1B. SOLAR FORECAST
             15 Jun             16 Jun             17 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 disk is spotless. Solar wind speed Vsw was low
300-330km/sec. 
Stereo-B spacecraft shows similar levels so Vsw should remain 
in the low-average 300-350km/sec range for the next 2-3 days. 
IMF Bz had an extended southward period 05-21UT up to -7nT which 
was effective for merging with the geomagnetic field from ~17UT. 
SOHO spacecraft LASCO C2 and C3 imagers observed an east limb 
CME early on 13th June which is not expected to be geo-effective. 
However if the shock front is broad the edge may glance the
geomagnetic field in the next 1-2 days. 




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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 14 Jun: Quiet 

Estimated Indices 14 Jun :  A   K           
   Australian Region       3   21111111
      Darwin               3   21011111
      Townsville           7   22222222
      Learmonth            4   21012121
      Camden               2   11011111
      Canberra             1   10011001
      Hobart               2   10111111
      Casey(Ant)           4   21112121
    
Observed Regional daily pc3 Indices 14 Jun : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice_Springs        0   (Quiet)
      Camden               0   (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 14 Jun : A 
           Fredericksburg         5
           Planetary              5                         

Observed AFr/Ap Indices 13 Jun :  A   K
           Fredericksburg         3
           Planetary              4   1010 1122     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
15 Jun     4    Quiet 
16 Jun     4    Quiet 
17 Jun     4    Quiet 
COMMENT: The geomagnetic field was Quiet and mid and low latitudes 
due to low solar wind speed (Vsw). Stereo-B spacecraft shows 
similar levels so Vsw should remain in the low-average 300-350km/sec 
range for the next 2-3 days. IMF Bz had an extended southward 
period 05-21UT up to -7nT which was effective for merging with 
the geomagnetic field from ~17UT. The near auroral zone stations 
(Mawson, Davis) show Active to Minor Storm conditions near 2330UT. 
SOHO spacecraft LASCO C2 and C3 imagers observed an east limb 
CME early on 13th June which is not expected to be geo-effective. 
However if the shock front is broad the edge may glance the
geomagnetic field in the next 1-2 days causing sporadic Unsettled conditions. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
15 Jun      Normal         Normal         Normal
16 Jun      Normal         Normal         Normal
17 Jun      Normal         Normal         Normal

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


Date   T index
14 Jun    11

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Near predicted monthly values.
   Northern Australian Region:
      Near predicted monthly values.
   Southern Australian and New Zealand Region:
      Near predicted monthly values during local day,
      Enhanced by 60% 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
15 Jun     5    near predicted monthly values 
16 Jun     5    Near predicted monthly values 
17 Jun     5    Near predicted monthly values 
COMMENT: HF MUF conditions were at monthly averages except for 
southern stations (Canberra, Hobart, Christchurch) which showed 
very enhanced nighttime ionisation for reasons not readily apparent. 
Extensive spread-F at night at near-equatorial latitudes. MUFs 
are expected to remain mostly normal across Aust/NZ region for 
the next three days. Low possibility of slight disturbance in 
1-2 days if an east limb CME shock front glances the geomagnetic 
field. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 13 Jun
       Daily Proton Fluence >1 MeV:   7.1E+05
       Daily Proton Fluence >10 MeV:  1.9E+04
       Daily Electron Fluence >2 MeV: 5.10E+04   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.0

ACE Satellite Solar Wind Day Averaged Data for 13 Jun
Speed: 283 km/sec  Density:    0.3 p/cc  Temp: NA K  Bz:   0 nT

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