[Ips-dsgr] IPS Daily Report - 27 February 10

rwc rwc at ips.gov.au
Sun Feb 28 10:20:58 EST 2010


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 27/2330Z FEBRUARY 2010 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 27 FEBRUARY AND FORECAST FOR 28 FEBRUARY - 02 MARCH
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 27 Feb:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 27 Feb:  79/19

1B. SOLAR FORECAST
             28 Feb             01 Mar             02 Mar
Activity     Very low           Very low           Low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    84/26              84/26              84/26

COMMENT: Solar activity was Very Low over the the last 24 hours. 
Active regions 1050 and 1051 have simple magnetic structure and 
are not expected to produce any significant activity over the 
next three days, however the return of active region 1045 late 
in the UT day on 28 February may increase activity to Low. The 
solar wind speed was at nominal levels of 300 to 360 km/s. Expect 
the solar wind to remain in this range until mid UT day on 28 
February when a recurrent coronal hole is expected to be geo-effective. 
The Bz component of the interplanetary magnetic field ranged between 
+/-4nT over the last 24 hrs. 

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 27 Feb: Quiet 

Estimated Indices 27 Feb :  A   K           
   Australian Region       2   11100121
      Darwin               2   11100012
      Townsville           3   21110121
      Learmonth            2   11000120
      Canberra             0   00000010
      Hobart               2   11100121
      Casey(Ant)           4   12210121
    
Observed Regional daily pc3 Indices 27 Feb : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            2   (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 Feb : A 
           Fredericksburg         5
           Planetary              5                         

Observed AFr/Ap Indices 26 Feb :  A   K
           Fredericksburg         1
           Planetary              2   1000 0001     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
28 Feb     8    Quiet to Unsettled 
01 Mar    10    Quiet to Unsettled 
02 Mar    10    Quiet to Unsettled 

COMMENT: Geomagnetic activity was predominantly Quiet at low 
to mid latitudes with isolated periods of Unsettled to Active 
levels in the Antarctic region. This trend is expected to continue 
until mid UT day today, 28 February, when the solar wind speed 
is expected to increase resulting in Quiet conditions at low 
latitudes, Quiet to Unsettled conditions at mid latitudes and 
Quiet to Active conditions at High latitudes with isolated cases 
of Minor Storm levels. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
28 Feb      Normal         Normal         Normal-Fair
01 Mar      Normal         Normal         Normal-Fair
02 Mar      Normal         Normal         Normal-Fair

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

Date   T index
27 Feb    32

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values during local day,
      Enhanced by 20% during local night.
      Enhanced by 25% after local dawn.
   Niue Island Region:
      Enhanced by 35% during local day,
      Enhanced by 25% during local night.
      Enhanced by 30% after local dawn.
   Northern Australian Region:
      Near predicted monthly values during local day,
      Variable conditions during local night.
   Southern Australian and New Zealand Region:
      Near predicted monthly values during local day,
      Enhanced by 15% during local night.
      Enhanced by 35% after local dawn.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day.

Predicted Monthly T index for February:   4

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
28 Feb    30    Near predicted monthly values to enhanced 10 
                to 30%. 
01 Mar    30    Near predicted monthly values to enhanced 10 
                to 30%. 
02 Mar    30    Near predicted monthly values to enhanced 10 
                to 30%. 

COMMENT: Ionospheric conditions in the Australian/NZ region were 
elevated compared with predicted monthly values due to strong 
EUV from the sunspot regions on the disc. Expect similar conditions 
over the next three days. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 26 Feb
       Daily Proton Fluence >1 MeV:   2.3E+05
       Daily Proton Fluence >10 MeV:  2.1E+04
       Daily Electron Fluence >2 MeV: 4.90E+05   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A3.8

ACE Satellite Solar Wind Day Averaged Data for 26 Feb
Speed: 381 km/sec  Density:    1.9 p/cc  Temp:    67300 K  Bz:   1 nT

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