[Ips-dsgr] IPS Daily Report - 02 May 04

rwc rwc at ips.gov.au
Mon May 3 09:45:38 EST 2004


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 02/2330Z MAY 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 02 MAY AND FORECAST FOR 03 MAY - 05 MAY
STATUS INDICATORS SOL:GREEN   MAG:** YELLOW **     ION: GREEN
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1A. SOLAR SUMMARY
Activity 02 May:  Low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 02 May:  98/45

1B. SOLAR FORECAST
             03 May             04 May             05 May
Activity     Low                Low                Low
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   100/48             100/48              95/41
COMMENT: Solar activity was low today. Several B- and 
C-class flares were recorded from region 601(S10W48)- 
the largest being a C8.3 at 1119UT. Region 601 remained 
quite active for the second consecutive day. The solar 
wind speed gradually decreased from 410 km/s to 370 km/s 
(approx.) by the time of this report. The north-south 
component of the interplanetary magnetic field (Bz) 
remained mostly moderately positive. A high speed solar 
wind stream from a coronal hole, is expected to keep the 
solar wind stream strengthened during the next three days. 
Also a faint CME has been reported associated with the 
C9-flare observed on 01 May. This CME is expected to cause 
some strengthening in the solar wind stream on 05 May. Due
to unavailability of LASCO images for the required period, 
no further comment can be made about this CME at this stage. 
Region 601 holds potential for isolated M-class activity. 

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 02 May: Quiet 

Estimated Indices 02 May :  A   K           
   Australian Region       4   2112 1112
      Darwin               5   2113 2112
      Townsville           6   2113 2122
      Learmonth            5   2113 1122
      Culgoora             4   2112 1112
      Canberra             3   2012 1111
      Hobart               3   2112 1011
      Casey(Ant)           3   2211 0111
    
Observed Regional daily pc3 Indices 02 MAY : 
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Culgoora            18   (Quiet)
      Canberra            52   (Unsettled)
      Hobart              71   (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 02 May : A 
           Fredericksburg         8
           Planetary              8                         

Observed AFr/Ap Indices 01 May :  A   K
           Fredericksburg         8
           Planetary             13   3333 3333     

2B. MAGNETIC FORECAST 
Date      Ap    Conditions
03 May    20    Unsettled to active, isolated minor storm periods 
                possible. 
04 May    20    Unsettled to active, isolated minor storm periods 
                possible. 
05 May    20    Unsettled to active, isolated minor storm periods 
                possible. 
COMMENT: IPS Geomagnetic Warning 16 was issued on 2 May and 
is current for interval 3-4 May. The geomagnetic activity 
remained lower than expected during the last 24 hours. The 
possible reasons for this seem to be a weaker than expected 
solar wind stream and also Bz remaining mostly positive. The 
geomagnetic activity may remain enhanced during the next 
3 days due to a coronal hole effect and a possible arrival 
of a faint CME that was associated to the C9 flare observed 
on 01 May. 

-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
02 May      Fair-normal    Normal         Normal-poor    
PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
03 May      Normal-fair    Fair           Fair-poor     
04 May      Normal-fair    Fair           Fair-poor     
05 May      Normal-fair    Fair           Fair-poor     
COMMENT: Moderate degradations in HF conditions are 
possible at mid and high latitudes during the next 3 days. 
Minor degradations may also be recorded at low latitudes 
during this period. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
02 May    49

Observed Australian Regional MUFs
   Equatorial PNG Region:
      Mostly near predicted monthly values,
      Enhanced by 20% after local dawn.
   Northern Australian Region:
      Near predicted monthly values during local day,
      Depressed by 15% during local night.
      Enhanced by 20% after local dawn.
   Southern Australian and New Zealand Region:
      Mostly near predicted monthly values,
   Antarctic Region (Casey/Scott Base):
      Enhanced by 15% over the UT day with periods of 
      significant depressions and degradations.


Predicted Monthly T index for May:  43

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
03 May    45    near predicted monthly values/depressed upto 
                15%. 
04 May    45    near predicted monthly values/depressed upto 
                15%. 
05 May    45    near predicted monthly values/depressed upto 
                15%. 
COMMENT: IPS HF Communications Warning 23 was issued on 
2 May and is current for interval 3-4 May. Minor to moderate 
depressions in MUFs and degradations in HF conditions may be 
observed, especially in the southern Aus/NZ regions during 
the next 3 days. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 01 May
       Daily Proton Fluence >1 MeV:   1.8E+05
       Daily Proton Fluence >10 MeV:  1.3E+04
       Daily Electron Fluence >2 MeV: 8.30E+05 (normal)
       X-ray background: A9.1
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.

ACE Satellite Solar Wind Day Averaged Data for 01 May
Speed: 425 km/sec  Density:    7.1 p/cc  Temp:    29700 K  Bz:   3 nT

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