[Ips-dsgr] IPS Daily Report - 14 October 03

rwc rwc at ips.gov.au
Wed Oct 15 08:45:38 EST 2003


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 14/2330Z OCTOBER 2003 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 14 OCTOBER AND FORECAST FOR 15 OCTOBER - 17 OCTOBER
STATUS INDICATORS SOL:GREEN   MAG:** RED **     ION: ** RED **
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1A. SOLAR SUMMARY
Activity 14 Oct:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 14 Oct:  92/37


1B. SOLAR FORECAST
             15 Oct             16 Oct             17 Oct
Activity     Low                Low                Low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN   100/48             100/48             105/54
COMMENT: Solar wind speed continued to rise starting the day 
at 500km/sec and increasing to 600km/sec toward end of UT day. 
Rise in solar wind speed due to solar coronal hole wind stream. 
The north-south component of the interplanetary magnetic field 
was southward by about 5nT for most of the UT day, increasing 
toward 10nT south 17-21UT. The coronal hole wind stream from 
this hole has a southward Bz orientation and further elevated 
wind speeds and southward orientation of Bz expected today. Elevated 
wind speed conditions expected until about 19 Oct. The Sun was 
flare quiet over past 24 hours. 

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 14 Oct: Unsettled to Minor Storm 

Estimated Indices 14 Oct :  A   K           
   Australian Region      24   3343 4455
      Darwin               -   ---- ----
      Townsville          20   2233 4455
      Learmonth           28   2333 5555
      Culgoora            26   3333 5455
      Canberra            25   2243 5455
      Hobart              24   2354 -4-5
      Casey(Ant)          17   4-33 333-
    
Observed Regional daily pc3 Indices 14 OCT : 
      Townsville           0   (Quiet)
      Learmonth            7   (Quiet)
      Culgoora            48   (Unsettled)
      Canberra            33   (Quiet to unsettled)
      Hobart              34   (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.

Estimated AFr/Ap Indices 14 Oct : A 
           Fredericksburg        25
           Planetary             40                         

Observed AFr/Ap Indices 13 Oct :  A   K
           Fredericksburg        12
           Planetary             13   3222 3334     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
15 Oct    25    Active to minor storm 
16 Oct    20    Active to minor storm 
17 Oct    18    Active 
COMMENT: IPS Geomagnetic Warning 46 was issued on 12 October 
and is current for interval 14-16 October. Geomagnetic activity 
forecast increased due to southward magnetic orientation of high 
speed wind stream from coronal hole now passing solar central 
meridian. Southward interplanetary magnetic field orientation 
is associated with stronger geomagnetic activity. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
15 Oct      Fair           Fair           Fair-Poor
16 Oct      Normal         Normal-Fair    Poor-Fair
17 Oct      Normal         Normal-Fair    Fair
COMMENT: Degradation in HF conditions stronger than expected. 
Degradation associated with coronal hole high speed wind stream. 
Continued degradation expected today, then possibly slightly 
easing but remaining somewhat degraded over next 3 to 4 days 
at mid to high latitudes. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
14 Oct    71

Observed Australian Regional MUFs
   Equatorial PNG Region:
      Near predicted monthly values during local day,
      Enhanced by 50% during local night.
   Northern Australian Region:
      Enhanced by 20% during local day,
      Enhanced by 45% during local night.
   Southern Australian and New Zealand Region:
      Near predicted monthly values during local day,
      Enhanced by 15% during local night.
      Depressed by 30% after local dawn.
   Antarctic Region (Casey/Scott Base):
      Near predicted monthly values, depressed 15-20%
      late in UT day. Spread F observed.


Predicted Monthly T index for October:  55

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
15 Oct    20    depressed 10 to 25% (southern Aus/NZ region)
15 Oct    50    near predicted monthly values (northern Aus)
16 Oct    30    depressed 10 to 15%/near predicted monthly values 
17 Oct    40    depressed 10 to 15%/near predicted monthly values 
COMMENT: IPS HF Communications Warning 67 was issued on 12 October 
and is current for interval 15-16 October. Depressed conditions 
observed after local dawn this morning southern Aus/NZ region. 
Northern Aus region MUFs (north of Brisbane) are showing a much 
less depression response to overnight geomagnetic activity, induced 
by a solar coronal hole high speed wind stream, hence there are 
two T indices forecast for today with a T index of 50 for northern 
Aus region, and a Tindex of 20 for southern Aus/NZ region. If 
you are communicating from one region to another it is suggested 
to use the lower of the two indices. Coronal hole induced geomagnetic 
activity expected next few days which will probably keep southern 
Aus/NZ region MUfs lower than normal possibly until 18 Oct. 
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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 13 Oct
       Daily Proton Fluence >1 MeV:   3.8E+05
       Daily Proton Fluence >10 MeV:  1.2E+04
       Daily Electron Fluence >2 MeV: 1.90E+06 (normal)
       X-ray background: B1.7
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.

ACE Satellite Solar Wind Day Averaged Data for 13 Oct
Speed: 367 km/sec  Density:    5.7 p/cc  Temp:    53200 K  Bz:  -2 nT

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