[Ips-dsgr] IPS Daily Report - 27 March 07

rwc rwc at ips.gov.au
Wed Mar 28 09:30:15 EST 2007


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 27/2330Z MARCH 2007 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 27 MARCH AND FORECAST FOR 28 MARCH - 30 MARCH
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 27 Mar:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 27 Mar:  73/9

1B. SOLAR FORECAST
             28 Mar             29 Mar             30 Mar
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    74/11              74/11              72/8
COMMENT: The solar activity remained very low on 27 March 
UT day. The effect of the coronal hole kept the solar wind 
stream strengthened. The solar wind speed remained between 
420 and 450 km/s until 1700UT and then showed a rise to 580 
km/s by 1900UT. The solar wind speed then showed a gradual 
decrease until the time of this report and it is around 550 
km/s at 2300UT. The north-south component of the interplanetary 
magnetic field (Bz) showed minor to moderate (mostly around 
+/-6 nT) fluctuations on both sides of the normal value almost 
the whole day. The effect of this coronal hole is expected to 
keep the solar wind stream strengthened on 28 March and then 
show a gradual decline. Solar activity is expected to remain 
at very low levels for the next few days. 

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

Geomagnetic field for Australian Region 27 Mar: Moslty quiet to
unsettled. 

Estimated Indices 27 Mar :  A   K           
   Australian Region       9   23232222
      Darwin              11   23233--2
      Townsville          12   23333--2
      Learmonth            9   232-----
      Camden               7   -2231122
      Canberra             8   23231222
      Hobart               7   22231222
      Casey(Ant)          14   34332233
    
Observed Regional daily pc3 Indices 27 Mar : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Camden              41   (Unsettled)
      Canberra            51   (Unsettled)
      Hobart              51   (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 and have been shown to be
well correlated with rejection of high resolution aeromagnetic
survey flight-line data. 

NOTE: Indices may have been generated from data obtained in 
cooperation with the following organisations: Geoscience Australia, 
University of Newcastle Space Physics Group, Australian Government 
Antarctic Division and Space Environment Research Center, Japan.


Estimated AFr/Ap Indices 27 Mar : A 
           Fredericksburg        12
           Planetary             15                         

Observed AFr/Ap Indices 26 Mar :  A   K
           Fredericksburg         7
           Planetary             11   1121 2433     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
28 Mar     8    Mostly quiet to unsettled, isolated active 
		periods possible. 
29 Mar     5    Quiet 
30 Mar     5    Quiet 
COMMENT: The effect of a high speed solar wind stream from 
a coronal hole may raise the geomagnetic activity levels to 
unsettled and sometimes to active levels on 28 March. The 
effect of the coronal hole is expected to gradually diminish 
thereafter. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
28 Mar      Normal         Normal         Normal-Fair
29 Mar      Normal         Normal         Normal
30 Mar      Normal         Normal         Normal
COMMENT: Mild to moderate degradations in HF conditions and
depressions in MUFs are possible on high latitude circuits 
on 28 March due to the possibility of an enhancement in 
geomagnetic activity levels on this day. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
27 Mar    17

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

Predicted Monthly T index for March:  10

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
28 Mar    16    Near predicted monthly values 
29 Mar    18    Near predicted monthly values 
30 Mar    18    Near predicted monthly values 
COMMENT: HF conditions are expected to remain mostly normal 
for most parts of the Aus/NZ region for the next three days 
with some possibility of minor degrdations and MUF depressions 
in the Southern Aus/NZ regions at times on 28 March. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 26 Mar
       Daily Proton Fluence >1 MeV:   2.3E+06
       Daily Proton Fluence >10 MeV:  1.7E+04
       Daily Electron Fluence >2 MeV: 5.40E+06   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.0

ACE Satellite Solar Wind Day Averaged Data for 26 Mar
Speed: 472 km/sec  Density:    5.2 p/cc  Temp:   139000 K  Bz:   0 nT

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