[Ips-dsgr] IPS Daily Report - 08 March 14 issued 2343 UT on 08 Mar 2014

rwc rwc at ips.gov.au
Sun Mar 9 10:43:12 EST 2014


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/08 MARCH 2014 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 08 MARCH AND FORECAST FOR 09 MARCH - 11 MARCH
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 08 Mar:  Low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 08 Mar: 142/96


1B. SOLAR FORECAST
             09 Mar             10 Mar             11 Mar
Activity     Low                Low                Low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN   140/94             135/89             135/89

COMMENT: Background x-ray flux remains at B levels during 8 March 
with only low level C-class flares from region 1991(S24W51) and 
new numbered region 2002(S19E64). There are currently 9 numbered 
regions on the visible disk, all are small with a simple magnetic 
configuration. Solar activity is expected to be Low for the next 
24 hours with only a slight chance of an M-class event. A small 
Disappearing Solar Filament (DSF) lifted off the SE Quadrant 
~~0300UT. SOHO observed 2 CMEs among which a CME first observed 
after 0330UT UT, most likely associated with the DSF and a second 
CME after 1836UT probably associated to a C2 flare from region 
2002 at 1800UT.The relevant period of imagery is not yet available 
to see whether they have an earth directed component. Further 
analysis will be given in tomorrow's report when imagery should 
be available. Solar wind speed was ~400km/s during the day and 
Bz component ranged in the neutral +/-4nT. A coronal hole high 
speed stream may mildly elevate solar wind speeds 09-10 March.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 08 Mar: Quiet

Estimated Indices 08 Mar : A   K           
   Australian Region       2   11101101
      Cocos Island         1   11001000
      Darwin               2   11101101
      Townsville           2   11101111
      Learmonth            2   21101101
      Alice Springs        2   11101101
      Norfolk Island       1   10000011
      Culgoora             1   01100101
      Gingin               1   20100000
      Camden               2   11101101
      Canberra             1   01100101
      Launceston           3   12110111
      Hobart               2   11110101    

Estimated Antarctic Regional K Indices 08 Mar :
      Macquarie Island     1   01110000
      Casey                9   24321112
      Mawson               8   31112114

Observed Regional daily pc3 Indices 08 Mar : 
      Darwin               2   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             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 International Center for Space Weather 
Science and Education, Japan.


Estimated AFr/Ap Indices 08 Mar : A 
           Fredericksburg         4
           Planetary              5                         

Observed AFr/Ap Indices 07 Mar :  A   K
           Fredericksburg         3
           Planetary              3   1000 1122     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
09 Mar    12    Unsettled with isolated Active periods.
10 Mar    10    Quiet to Unsettled
11 Mar     7    Quiet

COMMENT: Quiet conditions observed over the last 24 hours. Unsettled 
conditions, with possible Active periods may be expected over 
the next 24 hours,due to a minor coronal hole.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
08 Mar      Normal         Normal         Normal         

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
09 Mar      Normal         Normal-fair    Normal-fair
10 Mar      Normal         Normal-fair    Normal-fair
11 Mar      Normal         Normal-fair    Normal-fair


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


Date   T index
08 Mar   145

Observed Australian Regional MUFs
   Northern Australian Region:
      Near predicted monthly values during local day.
      Enhanced by 25% during local night.      
   Southern Australian and New Zealand Region:
      Enhanced by 20% during local day.
      Enhanced by 30% during local night.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Enhanced by 30% over the UT day.

Monthly T index:
Month  T index
Feb      121
Mar      79
Apr      79

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
09 Mar   130    Near to 15% above predicted monthly values
10 Mar   130    Near to 15% above predicted monthly values
11 Mar   130    Near to 15% above predicted monthly values

COMMENT: Observed MUFs were generally above predicted monthly 
values. There may be a slight lowering in MUFs values, however 
MUFs are expected to remain near predicted or slightly higher 
over the next 3 days.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 07 Mar
       Daily Proton Fluence >1 MeV:   1.4E+06
       Daily Proton Fluence >10 MeV:  2.2E+04
       Daily Electron Fluence >2 MeV: 6.60E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B5.4

ACE Satellite Solar Wind Day Averaged Data for 07 Mar
Speed: 429 km/sec  Density:    1.2 p/cc  Temp:    85700 K  Bz:   1 nT

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