[Ips-dsgr] IPS Daily Report - 18 November 03

rwc rwc at ips.gov.au
Wed Nov 19 10:55:57 EST 2003


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 18/2330Z NOVEMBER 2003 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 18 NOVEMBER AND FORECAST FOR 19 NOVEMBER - 21 NOVEMBER
STATUS INDICATORS SOL:** YELLOW **   MAG:** RED **     ION: GREEN
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1A. SOLAR SUMMARY
Activity 18 Nov:  Moderate

Flares    Max     Fadeout    Freq.  Sectors
 M3/2N    0752UT  possible   lower  Mid East/Indian
 M4/--    1011UT  possible   lower  European

Observed 10.7 cm flux/Equivalent Sunspot Number for 18 Nov: 144/98


1B. SOLAR FORECAST
             19 Nov             20 Nov             21 Nov
Activity     Moderate           Moderate to high   Moderate to high
Fadeouts     Possible           Probable           Probable
10.7cm/SSN   160/114            190/143            220/170
COMMENT: Active region 501 produced an M1.8 level impulsive flare 
at 0130UT, and a long duration M3.2 level flare at 0730. The 
second flare was one of a complex series of M level activity 
lasting several hours. A Type II radio sweep was observed on 
the Culgoora radiospectrograph at 0750UT with an estimated shock 
speed of 420 km/s. There was an associated full halo CME first 
visible in LASCO imagery at 0840UT. An earth-directed shock from 
this event is expected on day two of the forecast period. Sacramento 
Peak Observatory reports intense Ca XV emission on the east limb 
associated with the expected return today of previous X-class 
flare producing regions 486 and 488. 



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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 18 Nov: Unsettled to Active 

Estimated Indices 18 Nov :  A   K           
   Australian Region      16   3333 4333
      Darwin               -   ---- ----
      Townsville          15   3333 3333
      Learmonth           15   3333 4322
      Culgoora            15   3323 4333
      Canberra            18   3333 4433
      Hobart              17   3433 4322
      Casey(Ant)          24   4--4 4433
    
Observed Regional daily pc3 Indices 18 NOV : 
      Townsville          32   (Quiet to unsettled)
      Learmonth           78   (Active)
      Culgoora           126   (Severe storm)
      Canberra           188   (Severe storm)
      Hobart             185   (Severe storm)
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 18 Nov : A 
           Fredericksburg        18
           Planetary             21                         

Observed AFr/Ap Indices 17 Nov :  A   K
           Fredericksburg        21
           Planetary             34   5445 5544     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
19 Nov    35    Active to Minor storm 
20 Nov    50    Storm levels 
21 Nov    30    Active to Minor storm 
COMMENT: Solar wind parameters remain elevated due to the persisting 
coronal hole wind stream. Solar wind velocity has declined steadily 
over the UT day as the coronal hole rotates out of geoeffective 
range. Coronal hole wind stream effects should decline to near 
normal levels over the next day. There is a possibility of increased 
geomagnetic activity today due to a glancing blow from the CME 
observed on Nov 17. There is a high probability of significant 
disturbance up to severe storm levels at times due to a strong 
shock from a full halo CME observed around 0830UT today. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
19 Nov      Fair           Fair           Fair-Poor
20 Nov      Poor           Poor           Poor
21 Nov      Fair           Fair           Fair-Poor
COMMENT: HF conditions returning to normal after a prolonged 
period of coronal hole wind stream induced disturbance. High 
latitudes can expect further isolated periods of disturbance 
today. There is a good possibility of further geomagnetic activity 
at all latitudes over the next few days due to shocks following 
recent solar flare activity. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
18 Nov    53

Observed Australian Regional MUFs
   Equatorial PNG Region:
      Enhanced by 15% during local day,
      Enhanced by 20% during local night.
   Northern Australian Region:
      Near predicted monthly values during local day,
      Enhanced by 30% during local night.
   Southern Australian and New Zealand Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Scott Base):
      Near predicted monthly values over the UT day,
      with extended local periods of disturbance.


Predicted Monthly T index for November:  52

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
19 Nov    50    near predicted monthly values/depressed 5 to 
                10% 
20 Nov    35    about 20% below predicted monthly values 
21 Nov    50    depressed 10 to 20%/near predicted monthly values 
COMMENT: Generally improving HF conditions observed at all latitudes 
as geomagnetic disturbance due to coronal hole wind stream subsides. 
Expect continuing periods of disturbance at high latitudes today. 
There is a good possibility of degraded conditions on day two 
due to anticipated geomagnetic disturbance associated with a 
full halo CME observed early today. 
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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 17 Nov
       Daily Proton Fluence >1 MeV:   7.9E+06
       Daily Proton Fluence >10 MeV:  1.1E+04
       Daily Electron Fluence >2 MeV: 5.70E+08 (high)
       X-ray background: B7.2
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.

ACE Satellite Solar Wind Day Averaged Data for 17 Nov
Speed: 759 km/sec  Density:    1.5 p/cc  Temp:   296000 K  Bz:  -3 nT

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