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

rwc rwc at ips.gov.au
Tue May 11 09:51:34 EST 2010


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 10/2330Z MAY 2010 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 10 MAY AND FORECAST FOR 11 MAY - 13 MAY
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 10 May:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 10 May:  74/11

1B. SOLAR FORECAST
             11 May             12 May             13 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 during the UT day. One 
B-class flare was observed. Solar wind speed varied between 
320 and 370 km/s for most parts of the UT day today. The 
interplanetary magnetic field Bz component stayed close to 
the normal value almost the whole day today. Solar wind stream 
may remain strengthened for the next three days due to the 
presence of small sized coronal holes in geoeffective positions. 
Solar activity is expected to remain at very low levels for 
the next three days. 
-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 10 May: Quiet 

Estimated Indices 10 May :  A   K           
   Australian Region       3   1211110-
      Darwin               3   1211110-
      Townsville          12   -332----
      Learmonth            4   121-----
      Canberra             0   000010--
      Hobart               1   1100----
      Casey(Ant)           4   1220----
    
Observed Regional daily pc3 Indices 10 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 10 May : A 
           Fredericksburg         3
           Planetary              5                         

Observed AFr/Ap Indices 09 May :  A   K
           Fredericksburg         1
           Planetary              4   1001 1111     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
11 May     7    Quiet to unsettled 
12 May     7    Quiet to unsettled 
13 May     7    Quiet to unsettled 
COMMENT: Mostly Quiet conditions observed over the last 
24 hours. Mostly quiet to unsettled conditions with some 
possibility of isolated active periods may be expected for 
the next three days due to the presence of small coronal 
holes in geoeffective positions. 
-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
10 May      Normal         Normal         Normal         
PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
11 May      Normal         Normal         Normal-fair   
12 May      Normal         Normal         Normal-fair   
13 May      Normal         Normal         Normal-fair   
COMMENT: HF conditions were mostly normal today. Due to the
unavailability of some data due to a power failure, the whole 
day could not be analysed. Mostly normal conditions on low 
and mid latitudes are expected for the next three days and 
some MUF depressions and degradations in conditions may be 
possible on high latitude circuits due to a possible enhancement 
in geomagnetic activity levels during this period. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
10 May    14

Observed Australian Regional MUFs
   Cocos Island Region:
      No data available during local day,
      No data available during local night.
   Niue Island Region:
      Depressed by 20% during local day,
      Near predicted monthly values during local night.
      Depressed by 25% after local dawn.
   Northern Australian Region:
      Mostly near predicted monthly values,
   Southern Australian and New Zealand Region:
      Near predicted monthly values.
   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
11 May    22    near predicted monthly values 
12 May    22    near predicted monthly values 
13 May    22    near predicted monthly values 
COMMENT: Mostly normal HF conditions were observed in the Aus/NZ 
regions today. Due to the unavailability of some data due to 
a power failure, the whole day could not be analysed. Mostly 
normal HF conditions may be expected for the next three days 
in this region. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 09 May
       Daily Proton Fluence >1 MeV:   2.2E+05
       Daily Proton Fluence >10 MeV:  1.9E+04
       Daily Electron Fluence >2 MeV: 5.60E+08   (high fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability:24%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A3.8

ACE Satellite Solar Wind Day Averaged Data for 09 May
Speed: 405 km/sec  Density:    0.5 p/cc  Temp:    37300 K  Bz:   0 nT

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


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