[Ips-dsgr] IPS Daily Report - 05 February 12 issued 2331 UT on 05 Feb 2012

rwc rwc at ips.gov.au
Mon Feb 6 10:31:12 EST 2012


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 04/2330Z FEBRUARY 2012 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 04 FEBRUARY AND FORECAST FOR 05 FEBRUARY - 07 FEBRUARY
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 04 Feb:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 04 Feb: 107/57


1B. SOLAR FORECAST
             05 Feb             06 Feb             07 Feb
Activity     Very Low           Very Low           Very Low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN   105/54             105/54             105/54

COMMENT: Solar activity remained Very Low over the last 24 hours. 
The X-ray flares were two B-class from the largest region AR1410 
which has now stopped growing and is stable. It's partner region 
AR1413 is declining in size, and the only other active region 
on the disc AR1414 is small and not growing. The solar wind speed 
remained at mildly elevated levels ~450 km/s but was very steady 
at this level over the UT day. In contrast the IMF Bz north-south 
component fluctuated rapidly with timescales less than an hour 
between relatively low values of +/- 4nT but these fluctuations 
were likely to cause some geomagnetic disturbance. Solar activity 
is expected to remain Very Low for the next 3 days as the few 
currently visible sunspot regions are small, stable and magnetically 
simple (Beta). The STEREO-B spacecraft shows no significant active 
regions likely to rotate onto the Earth facing disc in the next three days.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 04 Feb: Quiet to Unsettled

Estimated Indices 04 Feb : A   K           
   Australian Region       8   22223222
      Darwin               8   22223222
      Townsville          10   22233322
      Learmonth           10   22224322
      Norfolk Island       6   12222222
      Camden               8   22223222
      Canberra             8   22223222
      Hobart               8   22223312    

Estimated Antarctic Regional K Indices 04 Feb :
      Macquarie Island    13   12244412
      Casey               21   35434323
      Mawson              25   44334345
      Davis               20   34444422

Observed Regional daily pc3 Indices 04 Feb : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gnangara             4   (Quiet)
      Canberra             2   (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 04 Feb : A 
           Fredericksburg         7
           Planetary              8                         

Observed AFr/Ap Indices 03 Feb :  A   K
           Fredericksburg         4
           Planetary              6   2111 3212     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
05 Feb     5    Quiet
06 Feb     5    Quiet
07 Feb     5    Quiet

COMMENT: Magnetic conditions in the Australian region were mainly 
Quiet with some isolated Unsettled periods, probably due the 
rapid, although low amplitude, fluctuations in IMF Bz north-south 
component throughout the day together with a moderately elevated 
solar wind speed. Antarctic regions, particularly around the 
auroral oval and sub-Antarctic (inner magnetosphere Plasmapause) 
saw some Active and Minor storms levels of activity. The polar 
cap was less affected suggesting strong field aligned current 
activity driven by the rapidly fluctuating IMF Bz. Conditions 
are expected to remain Quiet for the next 3 days, in the absence 
of prolonged IMF Bz southwards, as no CMEs or high speed solar 
wind streams are expected.


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

B
3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
05 Feb      Normal         Normal         Normal
06 Feb      Normal         Normal         Normal
07 Feb      Normal         Normal         Normal

COMMENT: HF conditions generally stable at mid and Equatorial 
latitudes. Polar latitudes moderately disturbed at auroral and 
sub-auroral regions, and a little less inside the polar cap, 
by geomagnetic activity from rapidly fluctuating IMF Bz north-south 
component augmented by moderately elevated solar wind speed.

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


Date   T index
04 Feb    77

Observed Australian Regional MUFs
   Niue Island Region:
      Mostly near predicted monthly values.
      Enhanced by 20% after local dawn.
   Northern Australian Region:
      Depressed by 15% during local day.
      Near predicted monthly values during local night.
   Southern Australian and New Zealand Region:
      Depressed by 15% during local day.
      Near predicted monthly values during local night.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day.

Predicted Monthly T index for February:  80

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
05 Feb    75    Near predicted monthly values
06 Feb    75    Near predicted monthly values
07 Feb    70    0 to 5% below predicted monthly values

COMMENT: MUFs were depressed ~15% at Mid-latitudes during the 
daytime, probably from the decreased EUV and X-ray ionising flux 
from the low number of sunspots which are all fairly small and 
low activity. However in an opposite trend, Equatorial latitudes 
had enhanced MUFs near local noon, probably due to transport 
of ionisation by thermospheric neutral winds into the region. 
Nighttime values were close to monthly medians and Mid-latitudes.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 03 Feb
       Daily Proton Fluence >1 MeV:   4.1E+05
       Daily Proton Fluence >10 MeV:  3.7E+04
       Daily Electron Fluence >2 MeV: 4.80E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B2.1

ACE Satellite Solar Wind Day Averaged Data for 03 Feb
Speed: 418 km/sec  Density:    4.0 p/cc  Temp:   100000 K  Bz:  -1 nT

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

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