[Ips-dsgr] IPS Daily Report - 22 July 04

rwc rwc at ips.gov.au
Fri Jul 23 09:57:08 EST 2004


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 22/2330Z JULY 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 22 JULY AND FORECAST FOR 23 JULY - 25 JULY
STATUS INDICATORS SOL:** YELLOW **   MAG:** YELLOW **     ION: GREEN
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1A. SOLAR SUMMARY
Activity 22 Jul:  High

Flares    Max     Fadeout    Freq.  Sectors
  M9.1    0032UT  probable   lower  West Pacific

Observed 10.7 cm flux/Equivalent Sunspot Number for 22 Jul: 173/127


1B. SOLAR FORECAST
             23 Jul             24 Jul             25 Jul
Activity     Low to moderate    Low to moderate    Low to moderate
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   170/124            160/114            160/114
COMMENT: Solar activity was moderate over the past 24 hours. 
Region 652 was the only active region, producing a M9.1 class 
flare at 0015UT, with an associated non-earth directed, southward 
projected CME as seen on the LASCO C3 imagery. Region 652 also 
produced some minor C-Class events, these being of the order 
of C5.3 and C5.8 at 0745UT and 1100UT respectively. The Culgoora 
Spectrograph continues to display a strong radio noise storm. 
Solar wind speed was steady at 400km/s from 0000UT to 1000UT 
upon which the sudden impulse from the expected arrival of the 
20July CME event caused solar wind parameters to increase, with 
the velocity rising to 500km/s and it then steadily rose to be 
at 700km/s of the time of this report. The north south component 
of the inter planetary magnetic field (Bz) also indicated the 
arrival of the CME as it began to oscilate between +/-10nT from 
1000UT, after which it then went southward at 1300UT with an 
avg. magitude of -10nT and a maximum of -20nT at 2000UT. The 
solar wind stream parameters are expected to be at elevated levels 
over the next 24hours. Region 652 did not undergo any change 
in its size or magnetic complexity, but still holds the potential 
for isolated flare activity. 
A moderate shock was observed in the solar wind at 0953UT on 
22 Jul. 
ACE EPAM data indicates an energetic ion enhancement event beginning 
22/0920UT, which can be a precursor to increased geomagnetic 
activity over next 24-36 hours. 

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 22 Jul: Quiet to Minor Storm 

Estimated Indices 22 Jul :  A   K           
   Australian Region      11   1113 3345
      Darwin              10   2113 3335
      Townsville          11   1113 4335
      Learmonth           12   1003 4346
      Culgoora             9   1013 3335
      Canberra            12   1033 3345
      Hobart               9   1003 3335
      Casey(Ant)          15   1213 3356
    
Observed Regional daily pc3 Indices 22 JUL : 
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Culgoora             0   (Quiet)
      Canberra            25   (Quiet to unsettled)
      Hobart               0   (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.

Estimated AFr/Ap Indices 22 Jul : A 
           Fredericksburg        10
           Planetary             12                         

Observed AFr/Ap Indices 21 Jul :  A   K
           Fredericksburg         5
           Planetary              6   2121 1322     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
23 Jul    22    active 
24 Jul    15    Unsettled to Active 
25 Jul    15    Unsettled to Active 
COMMENT: The geomagnetic activity was Active over the last 24 
hours with the arrival of the CME observed on 20 July. Unsettled 
to Active conditions are expected over the next 2 days with isolated 
periods of Minor Storm levels possible. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
23 Jul      Normal         Normal-Fair    Fair
24 Jul      Normal         Normal         Normal-Fair
25 Jul      Normal         Normal         Normal-Fair
COMMENT: Minor to moderate degradations of HF conditions are 
expected over the next 24 hours, especially at mid and high latitudes, 
with conditions returning to normal on day two and three of this 
outlook. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
22 Jul    64

Observed Australian Regional MUFs
   Equatorial PNG Region:
      Enhanced by 30% during local day,
      Enhanced by 65% during local night.
      Enhanced by 20% after local dawn.
   Northern Australian Region:
      Near predicted monthly values.
   Southern Australian and New Zealand Region:
      Enhanced by 15% during local day,
      Enhanced by 20% during local night.
      Enhanced by 30% after local dawn.
   Antarctic Region (Casey/Scott Base):
      Enhanced by 75% over the UT day.


Predicted Monthly T index for July:  39

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
23 Jul    55    near predicted monthly values/depressed 5 to 
                10% 
24 Jul    55    near predicted monthly values/depressed 5 to 
                10% 
25 Jul    55    Near predicted monthly values 
COMMENT: HF conditions are expected undergo isolated minor degradation 
periods in the southern regions of AUS/NZ over the next 24 hours, 
and return to normal on day two and three of this outlook. 
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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 21 Jul
       Daily Proton Fluence >1 MeV:   2.0E+05
       Daily Proton Fluence >10 MeV:  1.3E+04
       Daily Electron Fluence >2 MeV: 2.90E+07 (normal)
       X-ray background: B6.5
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.

ACE Satellite Solar Wind Day Averaged Data for 21 Jul
Speed: 461 km/sec  Density:    1.7 p/cc  Temp:   136000 K  Bz:   1 nT

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