[Ips-dsgr] IPS Daily Report - 23 November 07

rwc rwc at ips.gov.au
Sat Nov 24 10:20:33 EST 2007


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 23/2330Z NOVEMBER 2007 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 23 NOVEMBER AND FORECAST FOR 24 NOVEMBER - 26 NOVEMBER
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: ** RED **
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1A. SOLAR SUMMARY
Activity 23 Nov:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 23 Nov:  70/5

1B. SOLAR FORECAST
             24 Nov             25 Nov             26 Nov
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    70/5               70/5               70/5
COMMENT: The solar disk remains spotless and solar activity 
continued to remain at very low levels today as well. The 
currrently going on coronal hole effect seems to be weakening 
now as the solar wind speed showed a gradual decrease from 
600 km/s to 540 km/s during the UT day today and the 
north-south component of the interplanetary magnetic field 
(Bz) also seems to have settled close to the normal value. 
The effect of this coronal hole is expected to further weaken 
over the next two days. Solar activity is expected to remain 
at very low levels for the next few days. 

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 23 Nov: Quiet to active. 

Estimated Indices 23 Nov :  A   K           
   Australian Region       9   32323122
      Darwin               7   22223112
      Townsville           9   23223222
      Learmonth            9   32323122
      Camden              10   42322122
      Canberra             8   22323212
      Hobart               6   22322111
      Casey(Ant)          15   4-433222
    
Observed Regional daily pc3 Indices 23 Nov : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Canberra             9   (Quiet)
      Hobart              14   (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 23 Nov : A 
           Fredericksburg        10
           Planetary             10                         

Observed AFr/Ap Indices 22 Nov :  A   K
           Fredericksburg         6
           Planetary             13   1321 2444     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
24 Nov    10    Quiet to Unsettled 
25 Nov     7    Quiet 
26 Nov     6    Quiet 
COMMENT: The effect of the coronal hole, that is currently 
in geoeffective position, seems to be weakening now. The 
geomagnetic activity is expected to stay mostly at quiet to 
unsettled levels on 24 November and then mostly at quiet 
levels on 25 and 26 November. 

-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
23 Nov      Poor-normal    Poor-normal    Poor-fair      
PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
24 Nov      Normal-fair    Normal-fair    Fair          
25 Nov      Normal-fair    Normal-fair    Normal-fair   
26 Nov      Normal         Normal         Normal-fair   
COMMENT: HF conditions may show minor to significant
degradations on 24 and at times on 25 November especially 
at mid and high latitude locations due to weak ionisation 
in the ionosphere and some left over effect of a coronal 
hole. Periods of minor to moderate depressions MUFs and 
degradations in HF conditions may also be observed on low 
latitudes during this period. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
23 Nov   -44

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Depressed by 15% during local day,
      Depressed by 30% during local night.
   Northern Australian Region:
      Depressed by 35% during local day,
      Depressed by 25% during local night.
      Depressed by 25% after local dawn.
   Southern Australian and New Zealand Region:
      Depressed by 25% during local day,
      Depressed by 25% during local night.
      Depressed by 25% after local dawn.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Depressed by 10 to 40 % with periods of degradations.

Predicted Monthly T index for November:  11

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
24 Nov   -42    15 to 30% below predicted monthly values 
25 Nov   -38    10 to 20% below predicted monthly values 
26 Nov   -35    5 to 15% below predicted monthly values 
COMMENT: IPS HF Communications Warning 34 was issued on 
23 November and is current for interval 24-25 November. 
Minor to significant degradations in HF conditions and 
depressions in MUFs may be expected across Aus/NZ regions 
for the next two days. Some improvements in conditions 
may be possible on 26 November. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 22 Nov
       Daily Proton Fluence >1 MeV:   2.0E+06
       Daily Proton Fluence >10 MeV:  1.6E+04
       Daily Electron Fluence >2 MeV: 1.50E+08   (moderate fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability:13%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.0

ACE Satellite Solar Wind Day Averaged Data for 22 Nov
Speed: 518 km/sec  Density:    4.0 p/cc  Temp:   102000 K  Bz:   0 nT

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