[Ips-dsgr] IPS Daily Report - 26 April 03

rwc rwc at ips.gov.au
Sun Apr 27 09:56:50 EST 2003


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 26/2330Z APRIL 2003 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 26 APRIL AND FORECAST FOR 27 APRIL - 29 APRIL
STATUS INDICATORS SOL:** YELLOW **   MAG:** RED **     ION: GREEN
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1A. SOLAR SUMMARY
Activity 26 Apr:  High

Flares    Max     Fadeout    Freq.  Sectors
  M7.0    0807UT  probable   lower  Mid East/Indian
M2.1/1F    0058UT  possible   lower  West Pacific
M2.1/SN    0306UT  possible   lower  E. Asia/Aust.

Observed 10.7 cm flux/Equivalent Sunspot Number for 26 Apr: 144/98


1B. SOLAR FORECAST
             27 Apr             28 Apr             29 Apr
Activity     Low to moderate    Low to moderate    Low to moderate
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   150/105            145/99             140/94
COMMENT: Solar activity was high today. Three M-class flares 
were observed from region 338 (N18W71) These were M2.1/0058UT, 
M2.1/0306UT and M7.0/0807UT. No type II was associated to these 
flares. Because of un-availability of lasco images for this 
period, it could not be confirmed at this stage if any CME 
activity could be related to any of these flare. However, the 
absence of any Type II and Type IV around the time of these 
flares implies that it is less likely that there would have 
been any CME activity associated with these flare. It would 
be confirmed when the lasco images become available. 
Region 338 is still complex and holds potetial for M-class 
flare. Region 334(N16E13) also holds potential for M-class 
activity. The wind speed showed a gradual decrease from 
approximately 480 km/s to approximately 420 km/s during the 
UT day against an expected rise due to expected coronal hole 
activity which did not eventuate as yet. The solar wind 
stream may be strengthened due to the expected coronal hole 
activity in the next 2 days. The north-south component of the 
interplanetary magnetic field continued to show minor fluctuations 
between the north and south directions almost the whole day. 

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 26 Apr: Mostly quiet to unsettled with
occasional active periods. 

Estimated Indices 26 Apr :  A   K           
   Australian Region      13   2333 3333
      Darwin              11   2322 3333
      Townsville          12   2233 3333
      Learmonth           10   2222 3333
      Canberra            14   2233 4333
      Hobart              14   2233 4333
      Casey(Ant)          15   3432 3333
    
Observed Regional daily pc3 Indices 26 APR : 
      Townsville           0   (Quiet)
      Learmonth            3   (Quiet)
      Canberra            58   (Unsettled)
      Hobart              77   (Active)
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 26 Apr : A 
           Fredericksburg        10
           Planetary             15                         

Observed AFr/Ap Indices 25 Apr :  A   K
           Fredericksburg        19
           Planetary             32   4555 3435     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
27 Apr    25    Mostly active to minor storm. Isolated major 
                storm periods possible. 
28 Apr    23    Mostly active. Minor storm periods possible. 
29 Apr    20    Mostly unsettled to active. 
COMMENT: IPS Geomagnetic Warning 14 was issued on 26 April and 
is current for interval 26-28 April. The geomagnetic activity 
did not rise as per expectations as the expected coronal hole 
effect did not eventuate. The activity may rise during the next 
2 days due to the coronal hole effect. The CME activity, associated 
with the M3 flare observed on 24 April, may also have weak glancing 
effect on the geomagnetic activity on 27 April. The geomagnetic 
activity is expected to rise to active to minor storm levels 
with possibility of isolated major storm periods due to this 
coronal hole effect during the next 2 days. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
27 Apr      Fair           Fair           Fair-Poor
28 Apr      Normal         Normal-Fair    Fair
29 Apr      Normal         Normal-Fair    Fair
COMMENT: Mild to moderate depressions are possible over the next 
few days,especially at mid and high latitudes, due to anticipated 
elevated geomagnetic activity. 
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
26 Apr    78

Observed Australian Regional MUFs
   Equatorial PNG Region:
      Enhanced by 15% during local day,
      Near predicted monthly values during local night.
   Northern Australian Region:
      Enhanced by 15% during local day,
      Enhanced by 15% 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.


Predicted Monthly T index for April:  77

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
27 Apr    70    Depressed 5-10%. 
28 Apr    73    Depressed 5-10%. 
29 Apr    80    Near predicted monthly values 
COMMENT: IPS HF Communications Warning 30 was issued on 26 April 
and is current for interval 26-28 April. Mild to moderate depressions 
are possible at times over the next few days due to anticipated 
elevated geomagnetic activity. 
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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 25 Apr
       Daily Proton Fluence >1 MeV:   3.0E+06
       Daily Proton Fluence >10 MeV:  1.3E+04
       Daily Electron Fluence >2 MeV: 2.20E+08 (moderate)
       X-ray background: B6.4
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.

ACE Satellite Solar Wind Day Averaged Data for 25 Apr
Speed: 550 km/sec  Density:    3.3 p/cc  Temp:   208000 K  Bz:  -2 nT

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