[Ips-dsgr] IPS Daily Report - 20 September 08

rwc rwc at ips.gov.au
Sun Sep 21 09:46:04 EST 2008


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 20/2330Z SEPTEMBER 2008 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 20 SEPTEMBER AND FORECAST FOR 21 SEPTEMBER - 23 SEPTEMBER
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 20 Sep:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 20 Sep:  68/2


1B. SOLAR FORECAST
             21 Sep             22 Sep             23 Sep
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    67/0               67/0               67/0
COMMENT: Solar activity remained very low on 20 September. 
The disc remains spotless. The solar wind speed remained 
between around 300 km/s and 340 km/s for most parts of the 
UT day today. The north-south component of the interplanetary 
magnetic field (BZ) varied mostly between +/-3nT today. Solar 
activity is expected to remain at very low levels for the 
next 3 days. 
-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 20 Sep: Quiet 

Estimated Indices 20 Sep :  A   K           
   Australian Region       3   12111101
      Darwin               -   --------
      Townsville           -   --------
      Learmonth            -   --------
      Camden               1   12001000
      Canberra             1   12001000
      Hobart               4   12121102
      Casey(Ant)           5   23211111
    
Observed Regional daily pc3 Indices 20 Sep : 
      Darwin              NA
      Townsville          NA
      Learmonth           NA
      Alice_Springs       NA
      Camden               0   (Quiet)
      Gnangara            NA
      Canberra            NA
      Hobart               4   (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 20 Sep : A 
           Fredericksburg         3
           Planetary              5                         

Observed AFr/Ap Indices 19 Sep :  A   K
           Fredericksburg         3
           Planetary              5   0122 2112     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
21 Sep     3    Quiet 
22 Sep     3    Quiet 
23 Sep     3    Quiet 
COMMENT: The geomagnetic activity remained at mostly quite 
levels today and similar conditions can be expected for the 
next three days. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
21 Sep      Normal-fair    Normal         Normal-fair   
22 Sep      Normal-fair    Normal         Normal-fair   
23 Sep      Normal-fair    Normal         Normal-fair   
COMMENT: Minor to mild degradations in HF conditions at
low latitudes and minor to significant degradations at 
high latitudes were observed today. Poor ionisation in 
the ionosphere due to continued very low levels of solar 
activity seems to be the reason for these degradations 
in HF conditions and depressions in MUFs. Mid-latitude 
locations remained less affected by this phenomenon. 
Similar HF conditions may be expected for the next three 
days. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
20 Sep   -11

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Depressed by 20% during local day,
      Depressed by 35% during local night.
      Depressed by 20% after local dawn.
   Northern Australian Region:
      Depressed by 20% during local day,
      Depressed by 15% during local night.
      Depressed by 30% after local dawn.
   Southern Australian and New Zealand Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Irregular periods of enhancements and depressions in
      MUFs and degradations in HF conditions observed. 

Predicted Monthly T index for September:   2

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
21 Sep    -8    near predicted monthly values/depressed 5 to 
                15% 
22 Sep    -8    near predicted monthly values/depressed 5 to 
                15% 
23 Sep    -8    near predicted monthly values/depressed 5 to 
                15% 
COMMENT: Degradations in HF conditions and depressions in 
MUFs were observed today, especially at low and high latitudes. 
Poor ionisation due to continued very low levels of solar 
activity seems to be the reason for this. Mid latitudes were 
less affected by this phenomenon. Similar HF conditions may 
be expected across Auz/NZ regions for the next three days. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 19 Sep
       Daily Proton Fluence >1 MeV:   7.4E+05
       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: A1.0

ACE Satellite Solar Wind Day Averaged Data for 19 Sep
Speed: 349 km/sec  Density:    1.2 p/cc  Temp:    45700 K  Bz:  -1 nT

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


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