[Ips-dsgr] IPS Daily Report - 09 June 03

rwc rwc at ips.gov.au
Tue Jun 10 09:53:26 EST 2003


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 09/2330Z JUNE 2003 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 09 JUNE AND FORECAST FOR 10 JUNE - 12 JUNE
STATUS INDICATORS SOL:* YELLOW *   MAG:** RED **     ION: GREEN
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1A. SOLAR SUMMARY
Activity 09 Jun:  Moderate

Flares    Max     Fadeout    Freq.  Sectors
 M4/1N    1128UT  possible   lower  European

Observed 10.7 cm flux/Equivalent Sunspot Number for 09 Jun: 158/112


1B. SOLAR FORECAST
             10 Jun             11 Jun             12 Jun
Activity     Moderate           Low to moderate    Low to moderate
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   155/109            155/109            150/105
COMMENT: Due to continued growth in regions 375 and 380 there 
has been a general increase in background X-ray flux levels. 
Superimposed flare activity has resulted in a number of high 
C-class flares recorded over the past 24 hours. Region 375 produced 
an impulsive M4 level flare at 1120UT with an associated Type 
II radio sweep reported. LASCO C3 imagery showed an northeast 
directed CME from this event, which does not appear earth-directed. 
An X1 level flare occured at 2140UT. Culgoora radiospectrograph 
recorded a strong Type II sweep in association with this event. 
The flare was impulsive in nature, and no optical correlation 
was possible. Further M- to X- class activity is possible today 
from the currently visible active regions. 



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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 09 Jun: Unsettled to Minor Storm 

Estimated Indices 09 Jun :  A   K           
   Australian Region      16   3333 4335
      Darwin              15   3333 3334
      Townsville          16   3333 4335
      Learmonth           16   3333 4335
      Canberra            16   3333 4335
      Hobart              15   3333 4234
      Casey(Ant)          15   3433 3236
    
Observed Regional daily pc3 Indices 09 JUN : 
      Townsville           2   (Quiet)
      Learmonth           59   (Unsettled)
      Canberra           117   (Major storm)
      Hobart             155   (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 09 Jun : A 
           Fredericksburg        20
           Planetary             20                         

Observed AFr/Ap Indices 08 Jun :  A   K
           Fredericksburg        21
           Planetary             27   4543 3444     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
10 Jun    25    active 
11 Jun    20    active 
12 Jun    15    Unsettled to Active 
COMMENT: There was a general decline in solar wind speed over 
the first half of the UT day, followed by an increasing trend 
over the second half. Interplanetary magnetic field Bz has shown 
mild polarity fluctuations about an average neutral value, but 
trended moderately southward late in the UT day. There was a 
significant increase in solar wind proton and electron fluxes 
at the time of wind speed inflection, suggesting a further period 
of coronal hole induced disturbance today. These effects are 
expected to decline after tomorrow. At the time of report issue 
there is a major to minor magnetic storm period in progress. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
10 Jun      Fair           Fair           Fair-Poor
11 Jun      Normal         Normal-Fair    Fair
12 Jun      Normal         Normal         Normal-Fair
COMMENT: Moderate overnight depressions observed S Aus region. 
Extended periods of disturbance observed at high latitudes. HF 
conditions expected to be degraded at mid to high latitudes over 
next few days due to coronal hole high speed wind stream. 
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
09 Jun    84

Observed Australian Regional MUFs
   Equatorial PNG Region:
      Near predicted monthly values during local day,
      Enhanced by 50% during local night.
      Enhanced by 20% after local dawn.
   Northern Australian Region:
      Enhanced by 15% during local day,
      Near predicted monthly values during local night.
   Southern Australian and New Zealand Region:
      Near predicted monthly values during local day,
      Depressed by 25% during local night.
   Antarctic Region (Casey/Scott Base):
      Exteneded periods of disturbance. Widespread spread-F
      conditions observed. Absorption around local dawn.


Predicted Monthly T index for June:  68

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
10 Jun    70    Near predicted values/enhanced equatorial/PNG 
                region. Near predicted monthly values with mild 
                overnight or post-dawn depressions Aus/NZ regions. 
                Generally poor conditions in Antarctic regions. 
11 Jun    80    near predicted monthly values 
12 Jun    85    Near predicted monthly values 
COMMENT: Moderate overnight depressions observed S Aus regions. 
Extensive and occasionally intense sporadic-E and spread-F conditions 
observed S Ocean/Antarctic regions with absorption observed around 
local dawn. Expect similar localised conditions today. Degraded 
HF conditions expected next few days due to further coronal hole 
induced geomagnetic activity. 
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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 08 Jun
       Daily Proton Fluence >1 MeV:   9.7E+05
       Daily Proton Fluence >10 MeV:  1.0E+04
       Daily Electron Fluence >2 MeV: 2.50E+07 (normal)
       X-ray background: B7.9
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.

ACE Satellite Solar Wind Day Averaged Data for 08 Jun
Speed: 756 km/sec  Density:    2.6 p/cc  Temp:   280000 K  Bz:   0 nT

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