[Ips-dsgr] IPS Daily Report - 31 May 06

rwc rwc at ips.gov.au
Thu Jun 1 09:37:40 EST 2006


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 31/2330Z MAY 2006 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 31 MAY AND FORECAST FOR 01 JUNE - 03 JUNE
STATUS INDICATORS SOL:GREEN   MAG:** YELLOW **     ION: GREEN
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1A. SOLAR SUMMARY
Activity 31 May:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 31 May:  78/17


1B. SOLAR FORECAST
             01 Jun             02 Jun             03 Jun
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    80/20              75/13              80/20
COMMENT: A recurrent coronal hole is expected to become  
geoeffective about 1 June. A step change in solar wind speed 
occurred ~05UT from ~300km/sec to 400km/sec and it has slowly 
risen since. IMF Bz has been slightly north and south over the 
UT day and it currently ~+5nT so reconnection is not occurring 
with the geomagnetic field. 




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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 31 May: Quiet 

Estimated Indices 31 May :  A   K           
   Australian Region       3   21111111
      Darwin               3   21111111
      Learmonth            4   21221101
      Culgoora             2   11111100
      Camden               5   22112121
      Canberra             2   11111101
      Hobart               2   11111100
      Casey(Ant)           8   23222222
    
Observed Regional daily pc3 Indices 31 May : 
      Canberra             2   (Quiet)
      Learmonth            0   (Quiet)
      Culgoora             2   (Quiet)
      Hobart               6   (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 31 May : A 
           Fredericksburg         6
           Planetary             12                         

Observed AFr/Ap Indices 30 May :  A   K
           Fredericksburg         7
           Planetary              9   2202 3232     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
01 Jun    17    active 
02 Jun    18    active 
03 Jun    17    active 
COMMENT: IPS Geomagnetic Warning 6 was issued on 30 May and is 
current for interval 31 May to 2 June. A recurrent coronal hole 
is expected to become geoeffective about 1 June. Solar wind speed 
is already increasing and geomagnetic activity should increase 
over the UT day. IMF Bz is northwards and not expected to contribute 
to the increase in activity intially. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
01 Jun      Normal         Normal-Fair    Fair
02 Jun      Normal         Normal-Fair    Fair
03 Jun      Normal         Normal-Fair    Fair
COMMENT: Spread F prevalent at night at low/equatorial latitides 
and also observed at selected mid-latitude stations either all 
local night or pre-dawn. Strong sporadic E also observed at selected 
mid-near high latitudes (NLK,HBT). Expect conditions to degrade 
somewhat as the geomagnetic activity rises in response to the 
coronal hole solar wind speed increase. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
31 May    28

Observed Australian Regional MUFs
slightly above predicted monthly values

Predicted Monthly T index for May:  15

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
01 Jun    23    about 15% below predicted monthly values 
02 Jun    17    about 15% below predicted monthly values 
03 Jun    15    about 20% below predicted monthly values 
COMMENT: IPS HF Communications Warning 8 was issued on 31 May 
and is current for interval 1 June only. As the effects of the 
coronal hole solar wind speed increase take effect on the geomagnetic 
field, it will supress the ionosphere in the next 2-3 days. Depressions 
of up to 30% are possible and likely to average 15-20%. Spread 
F is already occurring at most tropical and some mid-latitude 
stations, particularly night and pre-dawn. This is likely to 
continue and degrade night time communications at all latitudes 
over the next 2-3 days together with reduced MUFs. 
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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 30 May
       Daily Proton Fluence >1 MeV:   3.5E+05
       Daily Proton Fluence >10 MeV:  1.7E+04
       Daily Electron Fluence >2 MeV: 1.60E+06 (normal fluence)  
Electron Fluence Daily Deep Dielectric Discharge Probability: 0%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A3.0

ACE Satellite Solar Wind Day Averaged Data for 30 May
Speed: 315 km/sec  Density:    2.2 p/cc  Temp:    23800 K  Bz:   1 nT

(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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Haymarket NSW 1240  AUSTRALIA       FTP: ftp://ftp.ips.gov.au 
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