[Ips-dsgr] IPS Daily Report - 15 October 09

rwc rwc at ips.gov.au
Fri Oct 16 10:25:15 EST 2009


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 15/2330Z OCTOBER 2009 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 15 OCTOBER AND FORECAST FOR 16 OCTOBER - 18 OCTOBER
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 15 Oct:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 15 Oct:  70/5


1B. SOLAR FORECAST
             16 Oct             17 Oct             18 Oct
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    72/8               72/8               72/8
COMMENT: Solar wind speed Vsw picked up from 300km/sec at 05UT 
to 450km/sec by 16UT and has remained there. This was accompanied 
by increases in solar wind density and temperature. This unexpected 
rise is possibly due to a corotating interaction region (CIR) 
ahead of either, the very weak coronal hole now near the cente 
of the disc in the southern hemisphere, or the stronger extension 
of the polar coronal hole that is visible now in STEREO-B images 
and approaching the limb. An IMF sector boundary crossing is 
expected in the next day or two, probably related to this event. 
IMF Bz was mostly north or weakly south apart from a -5nT southward 
excursion 15-17UT which was geoeffective (see geomagnetic). The 
solar disc continues to remain spotless although an active region 
is in transit mid-eastern limb in the SOHO spacecraft EIT imagery. 
Magnetograms still indicate simple bipolar magnetic configuration 
so flaring likelihood is low. No type II/III radio events from 
this region were observed by Learmonth observatory and the ARBIS 
software. Solar activity is expected to stay at very low levels 
for the next three days. STEREO-B shows the returning AR1027 
at 24N, due to return on the 15th and just becoming visible on 
the limb in SOHO EIT images. 




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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 15 Oct: Quiet 

Estimated Indices 15 Oct :  A   K           
   Australian Region       5   11222122
      Darwin               5   11222122
      Townsville           7   22222222
      Learmonth            5   11222221
      Canberra             3   01221021
      Hobart               6   11322121
      Casey(Ant)          10   32322232
    
Observed Regional daily pc3 Indices 15 Oct : 
      Darwin               2   (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 15 Oct : A 
           Fredericksburg         5
           Planetary              7                         

Observed AFr/Ap Indices 14 Oct :  A   K
           Fredericksburg         0
           Planetary              2   0000 1121     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
16 Oct     5    Quiet 
17 Oct     3    Quiet 
18 Oct     2    Quiet 
COMMENT: Geomagnetic conditions were Quiet at mid to low-latitudes 
despite the rise in Vsw to 450km/sec (see solar) at 16UT. Possible 
Unsettled conditions expected in the next 24 hours due to elevated 
Vsw. Polar conditions were mostly Unsettled with a brief high 
K at 19UT near the auroral oval from the IMF Bz southward excursion 
15-17UT. A weak coronal hole in the southern hemisphere will 
be in geoeffective position in one day although the current Vsw 
increase from the leading CIR may be it's main effect. STEREO-B 
shows another thin vertical coronal hole, an extension of the 
northern polar crown, approacing the limb, about 3-4 days from 
geoeffective position. 

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

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

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


Date   T index
15 Oct    -8

Observed Australian Regional MUFs
   Cocos Island/Niue Island Region:
      Depressed by 15% during local day,
      Depressed by 20% during local night.
   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:   1

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
16 Oct    -2    near predicted monthly values/depressed 5 to 
                20% 
17 Oct    -2    near predicted monthly values/depressed 5 to 
                20% 
18 Oct    -3    near predicted monthly values/depressed 5 to 
                10% 
COMMENT: HF frequencies are expected to remain mostly at normal 
to reduced levels during daytime across Aus/NZ for the next 3 
days with greated reductions in the north. Near-Equatorial regions 
show higher variability than mid-latitudes. Lack of significant 
magnetic activity indicates much of the low and mid latitude 
variability from monthly medians is being driven by neutral winds. 
Slightly enhanced geomagnetic activity in the day from increased 
Vsw may lift ionisation and frequencies. Similarly in 4-5 days 
when a coronal hole will probably take effect.effect. Extensive 
strong Es was observed across the region at Nuie 04-05UT, Learmonth 
12-13UT, Darwin 1230-14UT, Townsville 03-05UT, Brisbane 14-18UT, 
Norfolk Is 10-12UT, Hobart 17-21UT. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 14 Oct
       Daily Proton Fluence >1 MeV:   3.8E+05
       Daily Proton Fluence >10 MeV:  2.0E+04
       Daily Electron Fluence >2 MeV: 3.80E+04   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.0

ACE Satellite Solar Wind Day Averaged Data for 14 Oct
Speed: 353 km/sec  Density:    1.4 p/cc  Temp:    36000 K  Bz:   2 nT

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