[Ips-dsgr] IPS Daily Report - 14 May 10

rwc rwc at ips.gov.au
Sat May 15 09:51:20 EST 2010


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 14/2330Z MAY 2010 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 14 MAY AND FORECAST FOR 15 MAY - 17 MAY
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 14 May:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 14 May:  70/5

1B. SOLAR FORECAST
             15 May             16 May             17 May
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 during the UT day today. 
Solar wind speed varied between 320 and 380 km/s during the 
UT day. The Bz component of the IMF stayed between +/-4 nT 
for most parts of the day. Solar wind stream may gain some 
strength on 15 and 16 May due to a coronal hole. Solar activity 
is expected to remain at very low levels for the next three days. 
-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 14 May: Quiet 

Estimated Indices 14 May :  A   K           
   Australian Region       3   12110211
      Darwin               2   11100111
      Townsville          12   23322333
      Learmonth            2   11110210
      Canberra             0   00000100
      Hobart               1   01000110
      Casey(Ant)           6   23210221
    
Observed Regional daily pc3 Indices 14 May : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice_Springs        0   (Quiet)
      Gnangara             0   (Quiet)
      Canberra             0   (Quiet)
      Hobart               0   (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 14 May : A 
           Fredericksburg         3
           Planetary              5                         

Observed AFr/Ap Indices 13 May :  A   K
           Fredericksburg         2
           Planetary              4   1011 1111     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
15 May     8    Quiet to Unsettled 
16 May     8    Quiet to Unsettled 
17 May     6    Quiet 
COMMENT: Mostly quiet conditions were observed over the last 
24 hours. Mostly quiet to unsettled on 15 and 16 May and mostly 
quiet conditions on 17 May may be expected. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
15 May      Normal         Normal         Normal-Fair
16 May      Normal         Normal         Normal-Fair
17 May      Normal         Normal         Normal
COMMENT: HF conditions were mostly normal today. Appearance of 
sporadic E-layers affected communications conditions on low and 
some mid latitude locations. Minor to mild degradations in HF 
conditions may be possible on high latitude circuits on 15 
and 16 May due to possible enhancements in geomagnetic activity 
levels on these days. Otherwise HF conditions are expected to 
remain mostly normal on most other locations for the next three 
days. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
14 May     5

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values to depressed by
      20% during local day,
      Depressed by 15% during local night.
   Niue Island Region:
      Near predicted monthly values to depressed 
      by 25% during local day,
      Depressed by 20% during local night.
      Depressed by 30% after local dawn.
   Northern Australian Region:
      Near predicted monthly values during local day,
      Depressed by 20% during local night.
      Depressed by 20% after local dawn.
   Southern Australian and New Zealand Region:
      Depressed by 15% during local day,
      Near predicted monthly values during local night.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day.

Predicted Monthly T index for May:  24

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
15 May     8    Near predicted monthly values to depressed 10%. 
16 May     8    Near predicted monthly values to depressed 10%. 
17 May    10    Near predicted monthly values to depressed 10%. 
COMMENT: Mostly normal HF conditions were observed in the 
Aus/NZ regions today with some periods of minor to mild 
depressions in MUFs. Nearly similar HF conditions may be 
expected in this region on 15 and 16 May. Mostly normal HF 
conditions may be expected on 17 May in the region. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 13 May
       Daily Proton Fluence >1 MeV:   5.3E+05
       Daily Proton Fluence >10 MeV:  2.0E+04
       Daily Electron Fluence >2 MeV: 1.60E+08   (moderate fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability:14%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.6

ACE Satellite Solar Wind Day Averaged Data for 13 May
Speed: 419 km/sec  Density:    0.2 p/cc  Temp:    88100 K  Bz:   1 nT

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


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