[Ips-dsgr] IPS Daily Report - 22 April 07

rwc rwc at ips.gov.au
Mon Apr 23 09:31:49 EST 2007


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 22/2330Z APRIL 2007 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 22 APRIL AND FORECAST FOR 23 APRIL - 25 APRIL
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 22 Apr:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 22 Apr:  69/3


1B. SOLAR FORECAST
             23 Apr             24 Apr             25 Apr
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    70/5               70/5               70/5

COMMENT: Solar activity was very low over the last 24 hours and 
is expected to remain very low over the next few days. There 
are no visible spots on the solar disk. The anticipated high 
speed coronal hole wind stream arrived at ~22/0020 UT with a 
small impulse and a subsequent increase in solar wind speed to 
elevated for the next 2 days. 

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 22 Apr: Quiet to Unsettled
with isolated Active periods. 

Estimated Indices 22 Apr :  A   K           
   Australian Region      10   33232222
      Darwin               9   32232222
      Townsville          11   33232322
      Learmonth           18   33253333
      Camden               9   3-232222
      Canberra             9   22232322
      Hobart               8   22232222
      Casey(Ant)          10   33232222
    
Observed Regional daily pc3 Indices 22 Apr : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            3   (Quiet)
      Camden               9   (Quiet)
      Canberra             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 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 22 Apr : A 
           Fredericksburg         8
           Planetary             12                         

Observed AFr/Ap Indices 21 Apr :  A   K
           Fredericksburg         2
           Planetary              2   1100 0111     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
23 Apr    11    Quiet to unsettled 
24 Apr     8    Quiet to unsettled 
25 Apr     6    Quiet 

COMMENT: IPS Geomagnetic Warning 6 was issued on 22 April and 
is current for interval 22-23 April. Geomagnetic conditions over 
the UT day ranged from Quiet to Unsettled with isolated Active 
periods, particularly at high latitudes. The increased geomagnetic 
activity is in response to the arrival of a high speed coronal 
hole wind stream at ~22/0020UT (time at the ACE satellite). 
Geomagnetic conditions are expected to remain mostly Unsettled 
today (23 April) gradually returning to Quiet by 25 April. 

-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
22 Apr      Normal         Normal         Fair           
PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
23 Apr      Normal         Normal         Fair          
24 Apr      Normal         Normal         Normal-fair   
25 Apr      Normal         Normal         Normal-fair   

COMMENT: HF conditions were mostly normal over the UT day, with 
the exception of the Equatorial and Low latitude regions which 
experienced some MUF depressions late in the local day / early 
evening. Unsettled geomagnetic conditions may result in degraded 
HF at high latitudes and variable HF conditions at low latitudes 
today (23 April) and some minor MUF depressions, particularly 
at the higher latitudes. 

-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
22 Apr    10

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      No data available during local day,
      Depressed by 30% during local night.
   Northern Australian Region:
      Depressed by 20% during local day,
      Near predicted monthly values during local night.
   Southern Australian and New Zealand Region:
      Near predicted monthly values during local day,
      Enhanced by 20% during local night.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Enhanced by 15% over the UT day.

Predicted Monthly T index for April:   9

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
23 Apr     5    about 10% above predicted monthly values 
24 Apr     9    near predicted monthly values 
25 Apr    12    near predicted monthly values 

COMMENT: The ionosphere in the Australian region was mostly normal 
over the UT day, with the exception of the N.Aus/PNG regions 
which experienced MUF depressions of up to 30% near local
afternoon/early evening. More widespread MUF depressions are 
possible in the Australian region today (23 April) in response to 
yesterday's elevated geomagnetic activity, however they are only 
expected to be mild. 

-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 21 Apr
       Daily Proton Fluence >1 MeV:   5.5E+05
       Daily Proton Fluence >10 MeV:  1.9E+04
       Daily Electron Fluence >2 MeV: 8.50E+06   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 2%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.0

ACE Satellite Solar Wind Day Averaged Data for 21 Apr
Speed: 299 km/sec  Density:    6.2 p/cc  Temp:    23100 K  Bz:   0 nT

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