[Ips-dsgr] IPS Daily Report - 19 April 05

rwc rwc at ips.gov.au
Wed Apr 20 09:53:40 EST 2005


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 19/2330Z APRIL 2005 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 19 APRIL AND FORECAST FOR 20 APRIL - 22 APRIL
STATUS INDICATORS SOL:GREEN   MAG:** YELLOW **     ION: GREEN
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1A. SOLAR SUMMARY
Activity 19 Apr:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 19 Apr:  78/17

1B. SOLAR FORECAST
             20 Apr             21 Apr             22 Apr
Activity     Very low to low    Very low to low    Very low to low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    80/20              80/20              80/20
COMMENT: Solar activity has been very low during the last 
24 hours. An interesting high B-class flare was observed 
around S12E56 near the region 755 at 2150UT today. The flare 
was associated to a Type II radio sweep and a partial halo 
CME with shock speed between 1000 and 1300 km/s. The flare 
seems to have originated from two parallel ribbons, which 
normally results in a proton event. But the X-ray flux level 
of the flare has been quite low. So a proton event may eventuate 
in the next 24 hours but it is not very clear at this stage due 
to the low X-ray flux of the flare. Solar wind speed decreased 
from 370 to 320 km/s by 2000UT today and then rose to 400 km/s by 
the time of this report. This rise may have been caused by 
the anticipated coronal hole effect. The north-south component 
of the interplanetary magnetic field (Bz) remained close to 
the normal value for most of the time today. Solar activity 
is expected to remain at very low to low levels during the 
next three days. The effect of another coronal hole, that is 
taking a geoeffective position, may further strengthen the 
solar wind stream from 22 April. 

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 19 Apr: Quiet 

Estimated Indices 19 Apr :  A   K           
   Australian Region       4   1221 2112
      Learmonth            5   1221 2222
      Culgoora             4   1121 2112
      Canberra             5   1231 2102
      Hobart               4   1221 2102
      Casey(Ant)           7   2232 2211
    
Observed Regional daily pc3 Indices 19 Apr : 
      Townsville          NA
      Learmonth           NA
      Culgoora            NA
      Canberra            NA
      Hobart              10   (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 19 Apr : A 
           Fredericksburg         8
           Planetary             10                         

Observed AFr/Ap Indices 18 Apr :  A   K
           Fredericksburg         5
           Planetary              8   1321 2222     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
20 Apr    12    Mostly unsettled, active periods possible. 
21 Apr    12    Mostly unsettled, active periods possible. 
22 Apr    16    Mostly unsettled, extended active periods possible. 
COMMENT: Due to the effect of a high speed solar wind 
stream from a coronal hole the geomagnetic activity may 
rise from quiet to unsettled levels with possibility of 
active periods during the next three days. Relatively 
longer active periods may be possible on day three of 
this period due to another coronal hole taking geoeffective 
position around that time. 

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
19 Apr      Normal         Normal         Poor-normal    
PCA Event : No event. (Caution: A proton event may be observed
in the next 24 hours from a parallel ribbon flare. But the flare
X-ray flux being low, it is not very clear at this stage if the 
proton event will actually eventuate or not.)

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
20 Apr      Normal         Normal         Normal-Fair
21 Apr      Normal         Normal         Normal-Fair
22 Apr      Normal         Normal-Fair    Fair
COMMENT: HF conditions are expected to remain mostly normal 
at low and mid latitude locations during the next two days. 
However, minor to moderate degradations in HF conditions may 
be observed on high latitudes during the next three days and 
on some mid-latitude locations on the third day of this period. 
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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
19 Apr    31

Observed Australian Regional MUFs
   Equatorial PNG Region:
      Enhanced by 15% during local day,
      Enhanced by 15% during local night.
   Northern Australian Region:
      Near predicted monthly values during local day,
      Depressed by 25% during local night.
   Southern Australian and New Zealand Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Scott Base):
      Near predicted monthly values with periods of
      minor to significant degradations.

Predicted Monthly T index for April:  29

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
20 Apr    25    near predicted monthly values/depressed 5%. 
21 Apr    25    near predicted monthly values/depressed 5%. 
22 Apr    23    near predicted monthly values/depressed 5 to 
                10%. 
COMMENT: HF conditions are expected to remain mostly normal 
in most northern Aus/NZ regions during the next three days. 
Minor to mild depressions in MUFs and degradations in HF 
conditions may be observed in Southern Aus/NZ regions during 
this period. 
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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 18 Apr
       Daily Proton Fluence >1 MeV:   6.4E+05
       Daily Proton Fluence >10 MeV:  1.5E+04
       Daily Electron Fluence >2 MeV: 4.20E+08 (moderate fluence)  
Electron Fluence Daily Deep Dielectric Discharge Probability:21%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A4.8

ACE Satellite Solar Wind Day Averaged Data for 18 Apr
Speed: 380 km/sec  Density:    3.2 p/cc  Temp:    51000 K  Bz:  -2 nT

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