[Ips-dsgr] IPS Daily Report - 27 December 11 issued 2350 UT on 27 Dec 2011

rwc rwc at ips.gov.au
Wed Dec 28 10:50:05 EST 2011


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 27/2330Z DECEMBER 2011 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 27 DECEMBER AND FORECAST FOR 28 DECEMBER - 30 DECEMBER
STATUS INDICATORS SOL:GREEN   MAG:** RED **     ION: GREEN
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1A. SOLAR SUMMARY
Activity 27 Dec:  Low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 27 Dec: 140/94


1B. SOLAR FORECAST
             28 Dec             29 Dec             30 Dec
Activity     Moderate           Moderate           Moderate
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   140/94             140/94             140/94

COMMENT: Region 1386(S18E22) and region 1387(S21W57) produced 
several C-class flares, the largest being a C8.9 flare from region 
1386 at 0422UT. This was accompanied by a type II radio burst 
seen in the Culgoora solar radio telescope. A CME was associated 
with this event, it is not expected to be geoeffective. Regions 
1386 and 1387, the most active on the disk, are expected to continue 
producing C-class flares, with a chance of isolated M-class activity 
over the next 3 days. The solar wind conditions were normal over 
the last 24 hours. The multiple impact of the CMEs observed on 
25 and 26 December is likely to cause disturbance to the solar 
wind parameters from late on 28 December. A southern polar coronal 
hole might elevate the solar wind speed again on day 3.





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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 27 Dec: Quiet

Estimated Indices 27 Dec : A   K           
   Australian Region       1   11100011
      Darwin               4   22111112
      Townsville           5   12211122
      Learmonth            2   22100001
      Norfolk Island       2   11100112
      Camden               2   11200001
      Canberra             1   01100001
      Hobart               1   11100000    

Estimated Antarctic Regional K Indices 27 Dec :
      Macquarie Island     0   00100000
      Casey                6   33300011
      Mawson               2   22200000
      Davis                3   --211111

Observed Regional daily pc3 Indices 27 Dec : 
      Darwin               0   (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 27 Dec : A 
           Fredericksburg         0
           Planetary              0                         

Observed AFr/Ap Indices 26 Dec :  A   K
           Fredericksburg         2
           Planetary              0   0000 0000     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
28 Dec    25    Quiet to Active
29 Dec    20    Quiet to Active
30 Dec    20    Quiet to active

COMMENT: Mostly Quiet conditions observed over the last 24 hours. 
Quiet to Active conditions with Storm periods in Antarctica may 
be expected for the next 3 days due to the expected arrival of 
CMEs and that of a coronal hole.


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

B
3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
28 Dec      Normal         Normal         Fair
29 Dec      Normal-fair    Normal-fair    Fair
30 Dec      Normal-fair    Normal-fair    Fair



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


Date   T index
27 Dec   128

Observed Australian Regional MUFs
   Cocos Island Region:
      No data available during local day.
      No data available during local night.
   Niue Island Region:
      Enhanced by 30% during local day.
      Enhanced by 30% during local night.
   Northern Australian Region:
      Near predicted monthly values during local day.
      Enhanced by 20% during local night.
   Southern Australian and New Zealand Region:
      Enhanced by 20% during local day.
      Enhanced by 20% during local night.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Enhanced by 30% over the UT day.

Predicted Monthly T index for December:  71

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
28 Dec    90    Near predicted monthly values
29 Dec    90    Near predicted monthly values
30 Dec    90    Near predicted monthly values

COMMENT: Enhanced MUFs ranging from 10 to 30% observed over the 
last 24 hours. MUFs are expected to be near monthly values for 
low and mid latitudes for the next 3 days. Possible depressed 
periods for high latitudes due to the increased geomagnetic activity 
for 28-30 December.

-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 26 Dec
       Daily Proton Fluence >1 MeV:   3.9E+05
       Daily Proton Fluence >10 MeV:  8.3E+04
       Daily Electron Fluence >2 MeV: 9.90E+05   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B6.5

ACE Satellite Solar Wind Day Averaged Data for 26 Dec
Speed:NA km/sec  Density: NA p/cc  Temp: NA K  Bz: NA nT

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