[Ips-dsgr] IPS Daily Report - 02 July 03

rwc rwc at ips.gov.au
Thu Jul 3 08:48:15 EST 2003


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 02/2330Z JULY 2003 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 02 JULY AND FORECAST FOR 03 JULY - 05 JULY
STATUS INDICATORS SOL:** YELLOW **   MAG:** RED **     ION: **YELLOW**
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 02 Jul:  Moderate

Flares    Max     Fadeout    Freq.  Sectors
 M3/1F    0728UT  possible   lower  Mid East/Indian

Observed 10.7 cm flux/Equivalent Sunspot Number for 02 Jul: 135/89


1B. SOLAR FORECAST
             03 Jul             04 Jul             05 Jul
Activity     Low to moderate    Low to moderate    Low to moderate
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   140/94             145/99             150/105
COMMENT: Solar wind speed initially continued to decline from 550 to 
450km/sec and then began a rise back to 550km/sec toward end of the UT 
day. This rise may be an early than expected entry into a coronal 
hole wind stream that was expected to be entered 03/04 July. 
This coronal hole is visible as a south-polar extension hole 
in SEC SXI imagery. The north south component of the IMF was 
southward 5nT after about 6UT. Large solar region 397 in the 
north-east solar quadrant produced the M3 event. 397 region evolution 
has been mixed, with some growth reported in trailer spots, whilst 
decay has been reported in middle spots. A weak radio noise storm 
has been observed so far this morning on the Culgoora Spectrograph. 
Isolated M class activity probable. 

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

Geomagnetic field for Australian Region 02 Jul: Quiet to Unsettled 

Estimated Indices 02 Jul :  A   K           
   Australian Region       8   2223 2131
      Darwin               9   2223 2231
      Townsville           7   1123 2132
      Learmonth            8   2223 2131
      Canberra             8   2223 2131
      Hobart               7   1223 2221
      Casey(Ant)           9   2333 2121
    
Observed Regional daily pc3 Indices 02 JUL : 
      Townsville           0   (Quiet)
      Learmonth           15   (Quiet)
      Canberra            31   (Quiet to unsettled)
      Hobart              42   (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 02 Jul : A 
           Fredericksburg        12
           Planetary             14                         

Observed AFr/Ap Indices 01 Jul :  A   K
           Fredericksburg        14
           Planetary             13   3432 3333     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
03 Jul    15    Unsettled to active 
04 Jul    20    Active, chance of isolated minor storm periods. 
05 Jul    20    Active, chance of isolated minor storm periods. 
COMMENT: IPS Geomagnetic Warning 28 was issued on 2 July and 
is current for interval 3-6 July. Geomagnetic activity is expected 
to be initially unsettled today then becoming active later in UT 
day. Active conditions are then expected 4-5 July with chance 
for isolated minor storm periods. 
-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
02 Jul      Normal         Fair-normal    Fair           
PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
03 Jul      Normal         Normal         Normal-Fair
04 Jul      Normal         Normal-Fair    Fair
05 Jul      Normal         Normal-Fair    Fair
COMMENT: A gradual return to degraded conditions is expected 
at mid to high latitudes over coming days. Mid to Low latitudes 
are expected to remain near normal. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
02 Jul    72

Observed Australian Regional MUFs
   Equatorial PNG Region:
      Near predicted monthly values during local day,
      Enhanced by 35% during local night.
   Northern Australian Region:
      Mostly near predicted monthly values,
   Southern Australian and New Zealand Region:
      Mostly near predicted monthly values,
   Antarctic Region (Casey/Scott Base):
      Near predicted monthly values over the UT day.


Predicted Monthly T index for July:  62

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
03 Jul    75    near predicted monthly values 
04 Jul    75    near predicted monthly values 
05 Jul    75    Near predicted monthly values 
COMMENT: Southern region conditions may deteriorate again, particularly 
local night hours, and after local dawn, from 04 July due to 
activity induced by another coronal hole wind stream. Chance 
of an isolated shortwave fadeouts on daylight circuits. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 01 Jul
       Daily Proton Fluence >1 MeV:   3.4E+05
       Daily Proton Fluence >10 MeV:  1.1E+04
       Daily Electron Fluence >2 MeV: 2.80E+08 (moderate)
       X-ray background: B3.8
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.

ACE Satellite Solar Wind Day Averaged Data for 01 Jul
Speed: 647 km/sec  Density:    1.0 p/cc  Temp:   181000 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