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

rwc rwc at ips.gov.au
Tue Aug 17 09:43:42 EST 2010


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

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 16 Aug:  85/27

1B. SOLAR FORECAST
             17 Aug             18 Aug             19 Aug
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    85/27              85/27              85/27
COMMENT: Active region (AR) 1099(N17W85) produced several 
B and one C class x-ray flare during the UT day, 16 August. 
Solar wind speed ranged from 360 to 400 km/s over the UT day. 
The Bz component of the interplanetary magnetic field ranged 
between +/-4 nT over the last 24 hours. Solar wind stream 
is expected to stay stronger on 17 and 18 August due to the 
anticipations of arrivals of two CMEs that were observed 
on 14 and 15 August. Solar activity is expected to remain at 
very low levels for the next 3 days with some possibility of 
C-class flares. 

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 16 Aug: Quiet 

Estimated Indices 16 Aug :  A   K           
   Australian Region       5   22211221
      Darwin               5   22211121
      Townsville           6   12222222
      Learmonth            5   22211221
      Canberra             4   22110121
      Hobart               6   12222221
      Casey(Ant)           5   22211221
    
Observed Regional daily pc3 Indices 16 Aug : 
      Darwin               0   (Quiet)
      Townsville          NA
      Learmonth            0   (Quiet)
      Alice_Springs        0   (Quiet)
      Gnangara             5   (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 16 Aug : A 
           Fredericksburg         8
           Planetary              8                         

Observed AFr/Ap Indices 15 Aug :  A   K
           Fredericksburg         5
           Planetary              5   2201 1112     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
17 Aug    15    Unsettled to Active 
18 Aug    15    Unsettled to Active 
19 Aug     7    Quiet 
COMMENT: Geomagnetic activity may rise to usettled levels 
with the possibility of some active periods on 17 and 18 
August due to the anticipated arrival of two CMEs that were 
observed on 14 and 15 August. Geomagnetic activity is expected 
to return to mostly quiet levels on 19 August. 
-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
16 Aug      Normal         Normal         Normal         
PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
17 Aug      Normal         Normal-fair    Normal-fair   
18 Aug      Normal         Normal-fair    Normal-fair   
19 Aug      Normal         Normal         Normal        
COMMENT: Mostly normal HF conditions were observed on most 
locations on 16 August. Minor to moderated degradations in 
HF conditions may be expected, especially on mid and high 
latitude locations, on 17 and 18 August due an expected rise 
in geomagnetic activity levels on these days. HF conditions 
are expected to return to mostly normal levels on 19 August. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
16 Aug    36

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

Predicted Monthly T index for August:  27

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
17 Aug    25    near predicted monthly values/depressed 5 to 
                15% 
18 Aug    25    near predicted monthly values/depressed 5 to 
                20% 
19 Aug    30    near predicted monthly values 
COMMENT: Mostly normal HF conditions were observed on 16 
August on most locations in the Aus/NZ region. Minor to 
moderate degradations in HF conditions may be expected on 
17 and 18 August mainly in the southern Aus/NZ regions 
due an anticipated rise in geomagnetic conditions on these 
days. HF conditions are expectected to return to mostly normal 
levels on 19 August. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 15 Aug
       Daily Proton Fluence >1 MeV:   3.7E+06
       Daily Proton Fluence >10 MeV:  6.5E+04
       Daily Electron Fluence >2 MeV: 7.30E+07   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 9%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B1.5

ACE Satellite Solar Wind Day Averaged Data for 15 Aug
Speed: 386 km/sec  Density:    2.3 p/cc  Temp:    62000 K  Bz:   0 nT

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