[Ips-dsgr] IPS Daily Report - 17 January 08

rwc rwc at ips.gov.au
Fri Jan 18 10:42:55 EST 2008


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 17/2330Z JANUARY 2008 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 17 JANUARY AND FORECAST FOR 18 JANUARY - 20 JANUARY
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 17 Jan:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 17 Jan:  74/11


1B. SOLAR FORECAST
             18 Jan             19 Jan             20 Jan
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 disc currently spotless and solar activity expected 
to be very low. Solar disc dominated by recurrent coronal hole 
of extended longitude. The hole is still geoeffective and causing 
enhanced solar wind speeds (Vsw). From SOHO EIT195 and STEREO 
EUVI195 spacecraft images the hole appears to be weakening as 
well as the the more mid-latitude segments rotating beyond
geoeffective longitudes. The variations in hole latitude (inverted U) and 
its latitudinal narrowness appear to make Earth drift in and 
out of the higher speed stream as it rotates. Hence Vsw decreased 
from 620 to 560 km/sec but then increased to ~650km/sec over 
the UT day. 




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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 17 Jan: Quiet to Unsettled 

Estimated Indices 17 Jan :  A   K           
   Australian Region      10   23323222
      Darwin               8   22223222
      Townsville          10   23223322
      Learmonth           13   23324323
      Camden              10   23323222
      Canberra             -   --------
      Hobart               9   22323222
      Casey(Ant)          16   4-433232
    
Observed Regional daily pc3 Indices 17 Jan : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            2   (Quiet)
      Canberra             5   (Quiet)
      Hobart              31   (Quiet to unsettled)
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 17 Jan : A 
           Fredericksburg         8
           Planetary              8                         

Observed AFr/Ap Indices 16 Jan :  A   K
           Fredericksburg         9
           Planetary             11   3333 2223     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
18 Jan     6    Quiet 
19 Jan     6    Quiet 
20 Jan     4    Quiet 
COMMENT: Geomagnetic field was mostly Quiet with some Unsettled 
periods over the 24 hrs at mid and equatorial latitudes. Some 
activity is still due to coronal hole enhanced Vsw, but summer 
magnetic dipole orientation has dampened the magnetic fields 
response. The coronal hole is rotating out of geoeffective position 
and also waning so activity should be predominantly Quiet by 
19-20th. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
18 Jan      Normal         Normal         Normal
19 Jan      Normal         Normal         Normal
20 Jan      Normal         Normal         Normal
COMMENT: Extensive equatorial spread F observed at equatorial 
latitudes and pre-dawn sporadic E at mid-latitudes (in Australasian 
sector - take caution with extrapolation to other sectors). High 
latitudes still moderately disturbed, probably due to enhanced 
polar twin-cell convection caused by geomagnetic-IMF merging, 
although this has weakened compared with previous two days. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
17 Jan    -5

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Mostly near predicted monthly values,
      Depressed by 20% after local dawn.
   Northern Australian Region:
      Near predicted monthly values during local day,
      Depressed by 30% during local night.
   Southern Australian and New Zealand Region:
      Near predicted monthly values during local day,
      Depressed by 25% during local night.
      Enhanced by 70% after local dawn.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day.
      

Predicted Monthly T index for January:  12

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
18 Jan    -5    Below monthly values by (day/night); 5/10% for 
                northern Australia; 5/10% for southern Australia; 
                5/10% for equatorial; 0/5% for Antarctica. 
19 Jan     0    Below monthly values by (day/night); 5/10% for 
                northern Australia; 5/5% for southern Australia; 
                5/10% for equatorial; 0/0% for Antarctica. 
20 Jan     0    Near predicted monthly values 
COMMENT: At equatorial and sub-equatorial latitudes, extensive 
spread F was again observed, probably due to coronal hole induced 
geomagnetic disturbance which is now waning. At mid-latitudes 
strong pre-dawn sporadic (Es) which blanketed the F layer widespread. 
Night Es was common but often was not blanketing. Antarctic ionosphere
was still moderately disturbed due to ongoing but reduced enhanced 
geomagnetic conditions (Unsettled to Active) and polar twin-cell 
convection caused by geomagnetic-IMF merging. 
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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 16 Jan
       Daily Proton Fluence >1 MeV:   3.7E+06
       Daily Proton Fluence >10 MeV:  1.8E+04
       Daily Electron Fluence >2 MeV: 2.30E+08   (moderate fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability:16%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.0

ACE Satellite Solar Wind Day Averaged Data for 16 Jan
Speed: 661 km/sec  Density:    0.9 p/cc  Temp:   191000 K  Bz:  -1 nT

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