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

rwc rwc at ips.gov.au
Fri Oct 15 10:10:30 EST 2010


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

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 14 Oct:  80/20


1B. SOLAR FORECAST
             15 Oct             16 Oct             17 Oct
Activity     Low                Low                Low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    80/20              80/20              82/23
COMMENT: Regions 1112 and 1113 each produced B-class flares. 
1113 has low chance (<5%) of producing C or M flares. New Region 
1114 was numbered today but it is small with simple magnetic 
configuration. IMF Bz was slightly north for much of the UT day, 
not conducive to merging with the geomagnetic field. The solar 
wind veolcity Vsw further steadily declined to 280 km/s. A CME 
observed early on the 11th Oct has an estimated velocity of 400km/sec 
suggesting it will pass Earth early in the UT day on the 15th. 
Spacecraft observations suggest the CME front edge may strike 
a glancing blow but as there is no Forbush decrease in cosmic 
ray flux the CME is not strongly Earth directed. The filament 
near AR1112 may be a source of further CMEs. A small coronal 
hole on the limb just ahead of AR1113 may be geoeffective in 




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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 14 Oct: Quiet 

Estimated Indices 14 Oct :  A   K           
   Australian Region       4   22111112
      Darwin               2   12100002
      Townsville          12   33332223
      Learmonth            5   221-----
      Canberra             1   100-----
      Hobart               1   11100001
      Casey(Ant)           9   232-----
    
Observed Regional daily pc3 Indices 14 Oct : 
      Darwin               0   (Quiet)
      Townsville           2   (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 Oct : A 
           Fredericksburg         2
           Planetary              5                         

Observed AFr/Ap Indices 13 Oct :  A   K
           Fredericksburg         3
           Planetary              4   2121 1111     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
15 Oct     9    Quiet to Unsettled 
16 Oct     7    Quiet 
17 Oct     7    Quiet 
COMMENT: Geomagnetic activity was mostly Quiet at all latitudes 
as IMF Bz was slightly north for much of the UT day and solar 
wind veolcity Vsw steadily declined to 280 km/s. A CME in flight 
has an estimated velocity of 400km/sec suggesting it will reach 
Earth distance early in the UT day on the 15th. Spacecraft
observations 
suggest the CME front edge may strike a glancing blow, but as 
there is no Forbush decrease in cosmic ray flux the CME is not 
strongly Earth directed. A small coronal hole on the limb just 
ahead of AR1113 may be geoeffective in ~6 days. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
15 Oct      Normal         Normal         Normal-Fair
16 Oct      Normal         Normal         Normal
17 Oct      Normal         Normal         Normal

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
14 Oct     8

Observed Australian Regional MUFs
   Cocos Island Region:
      Depressed by 15% during local day,
      No data available during local night.
   Niue Island Region:
      Depressed by 15% during local day,
      Depressed by 25% during local night.
   Northern Australian Region:
      Depressed by 15% during local day,
      Near predicted monthly values during local night.
   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 October:  30

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
15 Oct    20    about 5% below predicted monthly values 
16 Oct    15    5 to 10% below predicted monthly values 
17 Oct    15    5 to 10% below predicted monthly values 
COMMENT: MUFs at mid and low latitudes continued to be slow recovering

from the CME induced geomagnetic disturbance on the 12th. Recovery 
to slightly monthly values should be helped by low geomagnetic 
activity and three active regions on the solar disc with more 
ionising radiation. Another CME may strike a glancing blow during 
local day on the 15th with possible ionospheric depressions. 
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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 13 Oct
       Daily Proton Fluence >1 MeV:   3.4E+05
       Daily Proton Fluence >10 MeV:  1.5E+04
       Daily Electron Fluence >2 MeV: 3.10E+07   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 5%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A6.7

ACE Satellite Solar Wind Day Averaged Data for 13 Oct
Speed: 357 km/sec  Density:    6.9 p/cc  Temp:    21600 K  Bz:   0 nT

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