[Ips-dsgr] IPS Daily Report - 11 July 08

rwc rwc at ips.gov.au
Sat Jul 12 09:43:53 EST 2008


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 11/2330Z JULY 2008 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 11 JULY AND FORECAST FOR 12 JULY - 14 JULY
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 11 Jul:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 11 Jul:  66/0


1B. SOLAR FORECAST
             12 Jul             13 Jul             14 Jul
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    66/0               66/0               66/0
COMMENT: Solar activity remained at very low levels over the 
last 24 hours as there is currently no active regions on disc. 
Solar wind parameters showed an increase in velocity, density 
and temperature with the arrival of the high speed solar wind 
stream from the recurrent coronal hole. Solar wind speed increased 
from 350km/s at 0000UT to be ~475km/s at the time of this report. 
The north-south component of the interplanetary magnetic field 
(Bz) ranged between +/-5nT for most of the UT day, but increased 
to 10nT at the time of this report and had few southward excursions. 
Solar wind velocity is expected further increase over the next 
24 hours. Solar activity is expected to remain at very low levels 
for the next 3 days. 




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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 11 Jul: Quiet to Unsettled 

Estimated Indices 11 Jul :  A   K           
   Australian Region       6   11223112
      Darwin               6   21223112
      Townsville           9   22323222
      Learmonth            7   11223113
      Camden               5   00223112
      Canberra             4   00223002
      Hobart               4   01123111
      Casey(Ant)           6   22222211
    
Observed Regional daily pc3 Indices 11 Jul : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice_Springs        0   (Quiet)
      Culgoora            10   (Quiet)
      Camden              10   (Quiet)
      Gnangara             0   (Quiet)
      Canberra             6   (Quiet)
      Hobart              11   (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 11 Jul : A 
           Fredericksburg         4
           Planetary             12                         

Observed AFr/Ap Indices 10 Jul :  A   K
           Fredericksburg         2
           Planetary              4   1001 1212     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
12 Jul    13    Unsettled to Active 
13 Jul    12    Unsettled 
14 Jul     9    Quiet to Unsettled 
COMMENT: Quiet to Unsettled geomagnetic conditions observed over 
the last 24 hours with the arrival of the high speed solar wind 
stream from the geoeffective coronal hole in the latter half 
of the UT day. Unsettled to Active conditions expected for 12Jul 
with possible isolated minor storm periods for mid to high latitudes. 
Unsettled conditions expected for 13Jul and Quiet to Unsettled 
for 14Jul. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
12 Jul      Normal-fair    Fair           Normal-fair   
13 Jul      Normal-fair    Normal-fair    Fair          
14 Jul      Normal-fair    Normal-fair    Fair          

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


Date   T index
11 Jul    -5

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Mostly 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 20% during local night.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Enhanced by 90% over the UT day.

Predicted Monthly T index for July:   4

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
12 Jul    -5    depressed 10 to 20%/near predicted monthly values 
13 Jul   -10    depressed 10 to 20%/near predicted monthly values 
14 Jul   -10    depressed 10 to 20%/near predicted monthly values 
COMMENT: Mostly normal HF conditions observed during the last 
24 hours for all regions. Southern AUS/NZ regions had continued 
enhanced conditions during local night and Antarctic regions 
over most of the UT day. With the continued rise in geomagnetic 
activity due to a high speed solar wind stream arrival over the 
next 24 hours, MUF depressions of 10%-20% possible for Northern 
AUS, Southern AUS/NZ regions and disturbed ionospheric conditions 
for Antarctic regions for 12Jul-14Jul. 
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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 10 Jul
       Daily Proton Fluence >1 MeV:   9.8E+05
       Daily Proton Fluence >10 MeV:  1.8E+04
       Daily Electron Fluence >2 MeV: 4.70E+06   (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 10 Jul
Speed: 337 km/sec  Density:    1.8 p/cc  Temp:    66300 K  Bz:   1 nT

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