[Ips-dsgr] IPS Daily Report - 16 October 10

rwc rwc at ips.gov.au
Sun Oct 17 10:41:07 EST 2010


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 16/2330Z OCTOBER 2010 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 16 OCTOBER AND FORECAST FOR 17 OCTOBER - 19 OCTOBER
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 16 Oct:  Moderate

Flares    Max     Fadeout    Freq.  Sectors
  M2.9    1912UT  possible   lower  East Pacific/

Observed 10.7 cm flux/Equivalent Sunspot Number for 16 Oct:  87/30

1B. SOLAR FORECAST
             17 Oct             18 Oct             19 Oct
Activity     Low to moderate    Low to moderate    Low to moderate
Fadeouts     Possible           Possible           Possible
10.7cm/SSN    88/32              88/32              88/32

COMMENT: Active region (AR) 1112 produced an M-class flare at 
16/1912UT. This flare was associated with a 1N H-alpha flare, 
observed at Holloman Solar observatory, and also had associated 
radio burst activity, reported by San Vito Solar Observatory, 
including a Tenflare and Type II sweep. AR 1112 continues to 
show a complex magnetic structure on the GONG magnetograms and 
has a moderate chance of producing C and/or M class xray flares 
over the next 24 hours. The solar wind veolcity ranged between 
380 and 310 over the UT day and is expected to remain in this 
range or slightly above for the next two days. The Bz component 
of the interplanetary magnetic field was between +4/-6 nT over 
the last 24 hours. On 19 October there is likely to be a increase 
in solar wind due to a coronal hole reaching its geoeffective 
location on the solar disc. There is also a possiblity of a slight 
increase in proton flux today, 17 October (inferred by Tenflare) 
and further geoeffective activity on 19 or 20 October due to 
the Type II sweep (inferred CME). 

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 16 Oct: Quiet 

Estimated Indices 16 Oct :  A   K           
   Australian Region       6   22112222
      Darwin               5   22101222
      Townsville          14   33323333
      Learmonth            6   22102322
      Canberra             4   11002222
      Hobart               4   11102222
      Casey(Ant)           8   33212222
    
Observed Regional daily pc3 Indices 16 Oct : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice_Springs        0   (Quiet)
      Gnangara             0   (Quiet)
      Canberra             0   (Quiet)
      Hobart               2   (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 16 Oct : A 
           Fredericksburg         4
           Planetary              5                         

Observed AFr/Ap Indices 15 Oct :  A   K
           Fredericksburg         3
           Planetary              5   0101 1131     

2B. MAGNETIC FORECAST 
Date      Ap    Conditions
17 Oct     6    Quiet 
18 Oct     6    Quiet 
19 Oct    12    Unsettled 

COMMENT: Geomagnetic activity was mostly Quiet at all latitudes. 
Expect this trend to continue for the next two days, On 19 October 
expect an increase in geomagnetic activity with mostly unsettled 
conditions and isolated cases of active to minor storm conditions 
at high latitudes due to increase speed in solar wind associated 
with coronal hole and CME (inferred by Type II sweep). 

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

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

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

Date   T index
16 Oct    31

Observed Australian Regional MUFs
   Niue Island Region:
      Near predicted monthly values during local day,
      Depressed by 15% during local night.
      Depressed by 25% after local dawn.
   Northern Australian Region:
      Near predicted monthly values during local day,
      Enhanced by 15% 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
17 Oct    30    Near predicted monthly values 
18 Oct    30    Near predicted monthly values 
19 Oct    30    Near predicted monthly values 

COMMENT: There is a slight possibility of a weak short wave fade 
at high latitudes due to an increase in proton flux that may 
occur today, 17 October, inferred by Tenflare burst occurring 
at 16/1916 UT. Otherwise, expect near predicted MUF values for 
the next three days. 

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 15 Oct
       Daily Proton Fluence >1 MeV:   4.1E+05
       Daily Proton Fluence >10 MeV:  1.4E+04
       Daily Electron Fluence >2 MeV: 1.60E+07   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 3%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A7.9

ACE Satellite Solar Wind Day Averaged Data for 15 Oct
Speed: 309 km/sec  Density:    5.3 p/cc  Temp:    25500 K  Bz:   1 nT

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