[Ips-dsgr] IPS Daily Report - 13 June 07

rwc rwc at ips.gov.au
Thu Jun 14 09:48:53 EST 2007


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 13/2330Z JUNE 2007 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 13 JUNE AND FORECAST FOR 14 JUNE - 16 JUNE
STATUS INDICATORS SOL:GREEN   MAG:** YELLOW **     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 13 Jun:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 13 Jun:  71/6

1B. SOLAR FORECAST
             14 Jun             15 Jun             16 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 
anticipated effect of the coronal hole seems to have 
started as the solar wind speed showed a gradual increase 
from 300 km/s to 440 km/s after 1400UT until around 2300UT. 
The north-south component of the interplanetary magnetic 
field (Bz) remained close to the normal value for most 
part of the UT day today with some fluctuations (between 
+8/-7 nT) recorded in the last few hours of the day. The 
effect of this coronal hole is expected to keep the solar 
wind stream strengthened on 14 and 15 June. 

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

Geomagnetic field for Australian Region 13 Jun: Quiet 

Estimated Indices 13 Jun :  A   K           
   Australian Region       5   11122221
      Darwin               4   11111221
      Townsville           7   22222222
      Learmonth            8   12222331
      Camden               4   01122121
      Canberra             3   00022221
      Hobart               5   10023221
      Casey(Ant)           5   11221221
    
Observed Regional daily pc3 Indices 13 Jun : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Camden               2   (Quiet)
      Canberra             0   (Quiet)
      Hobart              10   (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 13 Jun : A 
           Fredericksburg         4
           Planetary              5                         

Observed AFr/Ap Indices 12 Jun :  A   K
           Fredericksburg         3
           Planetary              4   1110 1112     

2B. MAGNETIC FORECAST 
Date      Ap    Conditions
14 Jun    16    Mostly unsettled to active. Isolated minor storm 
                possible on high latitudes. 
15 Jun    12    Mostly unsettled to active. 
16 Jun     8    Quiet to unsettled 
COMMENT: Due to the effect of a recurrent corohal hole, 
geomagnetic activity is expected to remain mostly at 
unsettled to active levels on 14 and 15 June with some 
possibility of isolated minor storm periods at high 
latitudes on 14 June. A gradual decline in the geomagnetive 
activity level is expected thereafter. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
14 Jun      Normal         Normal-fair    Fair          
15 Jun      Normal         Normal         Normal-fair   
16 Jun      Normal         Normal         Normal        
COMMENT: Minor to mild degradations in HF conditions and 
depressions in MUFs may be observed at high latitude and 
some mid latitude locations on 14 and possibly 15 June due 
to an anticipated enhancement in geomagnetic activity levels 
during this period. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
13 Jun    10

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Depressed by 15% to near predicted monthly values during local
day,
      Depressed by 25% to 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):
      Near predicted monthly values to enhanced by 25% over the UT day
      with periods of degradations in HF condtions.

Predicted Monthly T index for June:   9

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
14 Jun    10    near predicted monthly values 
15 Jun    12    near predicted monthly values 
16 Jun    15    Near predicted monthly values 
COMMENT: HF conditions are expected to remain mostly normal 
in most parts of Aus/NZ regions with some possibility of minor
degradations on some locations in the Southern Aus/NZ regions 
on 14 and 15 June due to an anticipated enhancement in 
geomagnetic activity levels on these days. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 12 Jun
       Daily Proton Fluence >1 MeV:   1.0E+06
       Daily Proton Fluence >10 MeV:  1.9E+04
       Daily Electron Fluence >2 MeV: 1.40E+07   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 3%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.6

ACE Satellite Solar Wind Day Averaged Data for 12 Jun
Speed: 317 km/sec  Density:    0.5 p/cc  Temp:    17200 K  Bz:  -1 nT

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


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