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

rwc rwc at ips.gov.au
Wed May 5 09:33:26 EST 2004


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 04/2330Z MAY 2004 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 04 MAY AND FORECAST FOR 05 MAY - 07 MAY
STATUS INDICATORS SOL:GREEN   MAG:** YELLOW **     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 04 May:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 04 May:  87/30

1B. SOLAR FORECAST
             05 May             06 May             07 May
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    95/41              95/41              90/34
COMMENT: Solar activity was  very low today. Only a few 
low B-class flares were  observed- the largest  being a 
B2.8 at 1609UT from region 601(S09W77).  The solar wind 
speed gradually increased from 350 to 450 km/s (approx.) 
during the first half of  the UT day and  then  remained 
between 400 km/s and 450 km/s during the rest of the day 
by the time of this report. The north-south component of 
the  interplanetary  magnetic field (Bz)  showed  minor  
fluctuations (+/- 5nT approx.) almost the whole day. The 
coronal hole, that is currently in a geoeffective position, 
may strengthen the solar wind stream during the next  two 
days. Region  601 may produce C-class activity. 

-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 04 May: Quiet to Unsettled 

Estimated Indices 04 May :  A   K           
   Australian Region       8   2331 3113
      Darwin               7   2--- ----
      Townsville           7   2231 3112
      Learmonth            8   2232 3123
      Culgoora             7   2231 3012
      Canberra             8   2331 3012
      Hobart               8   1331 3113
      Casey(Ant)          11   3332 3123
    
Observed Regional daily pc3 Indices 04 MAY : 
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Culgoora             0   (Quiet)
      Canberra             6   (Quiet)
      Hobart              26   (Quiet to 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 04 May : A 
           Fredericksburg         7
           Planetary             10                         

Observed AFr/Ap Indices 03 May :  A   K
           Fredericksburg         6
           Planetary              7   2122 2222     

2B. MAGNETIC FORECAST 
Date      Ap    Conditions
05 May    16    Mostly unsettled to active. 
06 May    16    Mostly unsettled to active. 
07 May    12    Quiet to unsettled 
COMMENT:  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 near the normal value. 
The geomagnetic activity  may remain enhanced during the 
next 2 days due to a coronal hole effect. 

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

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

Date   T index
04 May    52

Observed Australian Regional MUFs
   Equatorial PNG Region:
      Near predicted monthly values.
   Northern Australian Region:
      Near predicted monthly values.
   Southern Australian and New Zealand Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Scott Base):
      Near predicted monthly values over the UT day with
      periods of depressions and significant degradations. 


Predicted Monthly T index for May:  43

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
05 May    45    near predicted monthly values/depressed upto 
                10%. 
06 May    45    near predicted monthly values/depressed upto 
                10%. 
07 May    54    Near predicted monthly values 
COMMENT:  Minor to moderate  depressions  in MUFs  and 
degradations in HF conditions may be observed, especially 
in the southern Aus/NZ regions during the next 2 days. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 03 May
       Daily Proton Fluence >1 MeV:   1.7E+05
       Daily Proton Fluence >10 MeV:  1.3E+04
       Daily Electron Fluence >2 MeV: 2.50E+06 (normal)
       X-ray background: B1.0
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.

ACE Satellite Solar Wind Day Averaged Data for 03 May
Speed: 363 km/sec  Density:    9.0 p/cc  Temp:    39000 K  Bz:   1 nT

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


IPS Radio and Space Services      | email: asfc at ips.gov.au
PO Box 1386                       | WWW: http://www.ips.gov.au
Haymarket NSW 1240  AUSTRALIA     | FTP: ftp://ftp.ips.gov.au 
tel: +61 2 9213 8010              | fax: +61 2 9213 8060 

IMPORTANT: This e-mail, including any attachments, may contain,confidential
or copyright information.  The views expressed in this message are those of
the individual sender, unless specifically stated to be the views of IPS.
If you are not the intended recipient, please contact the sender immediately
and delete all copies of this e-mail and attachments.




More information about the ips-dsgr mailing list