[Ips-dsgr] IPS Daily Report - 23 April 02

rwc rwc at ips.gov.au
Wed Apr 24 09:52:19 EST 2002


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 23/2330Z APRIL 2002 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 23 APRIL AND FORECAST FOR 24 APRIL - 26 APRIL
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: ** YELLOW **
http://www.ips.gov.au/asfc/current
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1A. SOLAR SUMMARY
Activity 23 Apr:  Low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 23 Apr: 175/129

http://www.ips.gov.au/learmonth/solar     http://www.ips.gov.au/culgoora

1B. SOLAR FORECAST
             24 Apr             25 Apr             26 Apr
Activity     Low to moderate    Low to moderate    Low to moderate
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   180/133            180/133            180/133
COMMENT: Regions 9915(N11E28), 9916(S18E47) and 9914(N04E18) 
are showing minor growth. Region 9912(N11W38) is showing a slow 
decay in spots. After arrival of the shock, associated to the 
CME observed on 21 April, the solar wind speed went upto nearly 
680km/s. The solar wind speed remained nearly constant at 600km/s 
for nearly 14 hours. It is showing a decline now. 
A strong shock was observed in the solar wind at 0414UT on 23 
Apr. 

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2A. MAGNETIC SUMMARY
http://www.ips.gov.au/asfc/aus_geomag

Geomagnetic field for Australian Region 23 Apr: Quiet to Minor Storm 

Estimated Indices 23 Apr :  A   K           
   Australian Region      23   2553 3423
      Townsville          23   1553 3423
      Learmonth           26   1553 3523
      Canberra            21   1553 3322
      Hobart              21   1553 3322
      Casey(Ant)          30   3654 3333
      Davis(Ant)          34   3564 443-
    
Observed Regional daily pc3 Indices 23 APR : 
      Darwin              NA
      Townsville           3   (Quiet)
      Learmonth           19   (Quiet)
      Canberra            46   (Unsettled)
      Hobart              52   (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 23 Apr : A 
           Fredericksburg        18
           Planetary             22                         

Observed AFr/Ap Indices 22 Apr :  A   K
           Fredericksburg         8
           Planetary             12   3423 3322     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
24 Apr    15    Unsettled to active 
25 Apr    10    Quiet to unsettled. 
26 Apr     6    Mostly quiet. 
COMMENT: IPS Geomagnetic Warning 14 was issued on 23 April and 
is current for interval 23-24 April. A shock(0414UT/23April), 
followed by a sudden impulse (64nT, 0449UT/23April), arrived 
due to the CME obsrved on 21 April from region 9906.It raised 
the geomagnetic activity to minor storm level. After the arrival 
of this shock, Bz fluctuated between north and south for nearly 
14 hours and it now seems to be settling northwards. The geomagnetic 
activity is expected to decline from active to unsettled to quiet 
level over the next 3 days (i.e. 24, 25 and 26 April). The solar 
wind speed is also declining towards the more nominal levels. 
A moderate (64nT) impulse was observed in the IPS magnetomter 
data at 0449UT on 23 Apr. 
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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
23 Apr      Normal-fair    Normal-fair    Fair           
PCA Event : 10Mev Proton/PCA Event Began 21 04 2002 0235UT and is in progress

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
24 Apr      Normal         Normal         Poor-fair     
25 Apr      Normal         Normal         Fair-normal   
26 Apr      Normal         Normal         Normal        
COMMENT: Shock arrived at 0414UT/23April due to the partial halo 
CME observed on 21 April. It was followed by a moderate sudden 
impulse at 0450/23 April. The geomagnetic activity rose to minor 
storm level. Mild degradations were observed in the HF conditions 
at low and mid-latitudes. The >100MeV proton event ended at 2335UT/22April 
but the >10MeV proton event is still in progress. Polar circuits 
may be expected to show degradations due to the proton event 
on 24 April. 
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

http://www.ips.gov.au/asfc/aus_hf

Date   T index
23 Apr   121

Observed Australian Regional MUFs
   Equatorial PNG Region:
      Mostly near predicted monthly values,
      Enhanced by 30% after local dawn.
   Northern Australian Region:
      Near predicted monthly values during local day,
      Depressed by 15% during local night.
      Enhanced by 15% after local dawn.
   Southern Australian and New Zealand Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Scott Base):
      Proton event in progress, increased absorption observed.


Predicted Monthly T index for April: 113

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
24 Apr   140    Near predicted monthly values to enchanced upto 
                10%. 
25 Apr   150    10 to 20% above predicted monthly values 
26 Apr   155    10 to 20% above predicted monthly values 
COMMENT: IPS HF Communications Warning 18 was issued on 23 April 
and is current for interval 23-24 April. Due to the partial halo 
CME, observed on 21 April, the geomagnetic activity rose upto 
minor storm level on 23 April. The HF conditions are expected 
to remain mostly normal in Australian region over the next
3 days as the geomagnetic activity is declinig. 
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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 22 Apr
       Daily Proton Fluence >1 MeV:   3.3E+08
       Daily Proton Fluence >10 MeV:  8.0E+07
       Daily Electron Fluence >2 MeV: 5.60E+07 (normal)
       X-ray background: C1.0
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.

ACE Satellite Solar Wind Day Averaged Data for 22 Apr
Speed: 281 km/sec  Density:    1.7 p/cc  Temp:    77500 K  Bz:  -2 nT
http://sec.noaa.gov/ace/MAG_SWEPAM_24h.html

(Courtesy Space Environment Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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IPS Radio and Space Services      | email: asfc at ips.gov.au
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