[Ips-dsgr] IPS Daily Report - 20 May 07

rwc rwc at ips.gov.au
Mon May 21 09:50:18 EST 2007


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 20/2330Z MAY 2007 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 20 MAY AND FORECAST FOR 21 MAY - 23 MAY
STATUS INDICATORS SOL:GREEN   MAG:** YELLOW **     ION: GREEN
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1A. SOLAR SUMMARY
Activity 20 May:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 20 May:  74/11


1B. SOLAR FORECAST
             21 May             22 May             23 May
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    75/13              75/13              75/13

COMMENT: Solar activity was very low over the past 24 hours. 
Spot region 956 (N02W19) again produced some B-class Xray flares, 
the most significant of which was a B6.7 at 20/0556UT. Due to 
the unavailability of SOHO LASCO imagery it remains unclear whether 
the solar events that occurred on 19 May were associated with 
a CME. The estimated arrival time of any shocks associated with 
this activity is the second half of 21 May although the magnitude 
of the shock would be expected to be small. Solar wind speeds 
remain elevated (currently 550km/s) but in decline. 

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 20 May: Quiet 

Estimated Indices 20 May :  A   K           
   Australian Region       5   22121112
      Darwin               5   22121112
      Townsville           8   32222222
      Learmonth            7   32122122
      Camden               4   21121111
      Canberra             4   21120112
      Hobart               5   21131111
      Casey(Ant)           8   3-321222
    
Observed Regional daily pc3 Indices 20 May : 
      Darwin               0   (Quiet)
      Townsville           7   (Quiet)
      Learmonth            0   (Quiet)
      Camden              17   (Quiet)
      Canberra             9   (Quiet)
      Hobart              15   (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 20 May : A 
           Fredericksburg         6
           Planetary             10                         

Observed AFr/Ap Indices 19 May :  A   K
           Fredericksburg        10
           Planetary             12   2332 2333     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
21 May    18    active 
22 May     8    Quiet to Unsettled 
23 May     5    Quiet 

COMMENT: The geomagnetic field was generally Quiet to Unsettled 
over the UT day. Isolated Active periods were observed at high 
latitude stations. There is the chance of a shock arrival in 
the solar wind sometime in the second half of the UT day which 
may produce geomagnetic activity to Active levels. This is related 
to solar flare activity on 19 May. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
21 May      Normal         Normal-Fair    Fair
22 May      Normal         Normal         Normal-Fair
23 May      Normal         Normal         Normal

COMMENT: Frequencies were generally near predicted monthly values 
20 May, apart from some minor MUF depressions in the PNG/Niue 
region overnight. Spread-F was observed in some S.Aus/NZ/Antarctic 
stations likely in response to elevated geomagnetic activity. 
These conditions are expected to continue 21-22 May. MUF depressions 
possible 23 May if the expected geomagnetic activity eventuates 
21-22 May. 

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


Date   T index
20 May    16

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Enhanced by 30% during local day,
      Depressed by 35% 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 35% during local night.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day.

Predicted Monthly T index for May:   9

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
21 May    14    near predicted monthly values 
22 May    12    near predicted monthly values 
23 May     6    Near predicted monthly values / Depressed by 
                10%. 
COMMENT: HF conditions were mostly normal 20 May. Periods of 
Spread-F were again observed at mid-high latitude stations. 
Equatorial stations suffered some MUF depressions overnight. 
HF conditions are expected to be much the same 21 May with 
minor MUF depressions at low latitudes and further Spread-F 
possible at mid-high latitudes. Expect mostly normal HF 
conditions 22 May. MUF depressions possible 23 May. 

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

GOES satellite data for 19 May
       Daily Proton Fluence >1 MeV:   8.8E+05
       Daily Proton Fluence >10 MeV:  1.7E+04
       Daily Electron Fluence >2 MeV: 3.10E+06   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.7

ACE Satellite Solar Wind Day Averaged Data for 19 May
Speed: 604 km/sec  Density:    1.6 p/cc  Temp:   185000 K  Bz:   1 nT

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