[Ips-dsgr] IPS Daily Report - 25 February 14 issued 2330 UT on 25 Feb 2014

Regional Warning Centre rwc at ips.gov.au
Wed Feb 26 10:30:18 EST 2014


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/25 FEBRUARY 2014 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 25 FEBRUARY AND FORECAST FOR 26 FEBRUARY - 28 FEBRUARY
STATUS INDICATORS SOL:** RED **   MAG:GREEN     ION: ** YELLOW **
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1A. SOLAR SUMMARY
Activity 25 Feb:  High

Flares    Max     Fadeout    Freq.  Sectors
 X4/--    0049UT  probable   all    West Pacific

Observed 10.7 cm flux/Equivalent Sunspot Number for 25 Feb: 174/128


1B. SOLAR FORECAST
             26 Feb             27 Feb             28 Feb
Activity     Moderate to high   Moderate to high   Moderate to high
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   180/133            180/133            180/133

COMMENT: Solar activity over the last 24 hours was High due to 
an X4.9 flare from AR1990, newly rotated onto the solar disc 
and is returning region AR1967/1944. There were also mid C level 
flares from ARs 1986 and 1989. A large CME was issued with the 
X4.9 flare but it is directed towards the east as the source 
in AR1990 was at 82 deg E, and hence unlikely to be geoeffective. 
However SOHO LASCO observations assessed the CME to be an asymmetric 
partial halo and the GEOSTAT countdown has been initiated. Solar 
protons reached Earth a few hours later and the flux is currently 
at the low S1 level, unlikely to be a threat to spacecraft. AR1990 
has potential for further X class flares and other spot groups 
such as AR1981/82 have potential for M flares. Solar wind speed 
(Vsw) gradually decreased from 450km/s to 380km/s over the UT 
day. A latitudinally spread but longitudinally narrow coronal 
hole CH605, is near central meridian and should enhance speeds 
in 3-4 days time for less than 24 hours. The north-south component 
of the interplanetary magnetic field (IMF Bz) ranged between 
+/-5nT not effective for geomagnetic merging.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 25 Feb: Quiet to Unsettled

Estimated Indices 25 Feb : A   K           
   Australian Region       3   31001101
      Cocos Island         1   21000100
      Darwin               3   31100101
      Townsville           4   40000111
      Learmonth            5   41001102
      Alice Springs        4   40000101
      Norfolk Island       1   20001001
      Culgoora             3   30001011
      Gingin               5   41001102
      Camden               2   30001001
      Canberra             2   30001001
      Launceston           4   31012102
      Hobart               4   31012101    

Estimated Antarctic Regional K Indices 25 Feb :
      Macquarie Island     1   10011001
      Casey               10   43321212
      Mawson              13   21012126
      Davis                6   22112213

Observed Regional daily pc3 Indices 25 Feb : 
      Darwin               2   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               2   (Quiet)
      Canberra             7   (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 25 Feb : A 
           Fredericksburg         5
           Planetary              5                         

Observed AFr/Ap Indices 24 Feb :  A   K
           Fredericksburg         5
           Planetary              5   1112 1221     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
26 Feb     6    Quiet
27 Feb     6    Quiet
28 Feb     6    Quiet

COMMENT: Quiet conditions mostly observed at mid and low latitudes 
over the last 24 hours after an initial Unsettled 3 hours. Unsettled 
at high-latitudes ~13-15UT probably due to a weak shock in the 
solar wind observed at the L1 point by the ACE spacecraft ~1215UT. 
Expect mostly Quiet conditions for 26Feb-28Feb in the absence 
of prolonged IMF Bz southwards or CME activity from AR1982 which 
is in a geoeffective position.

-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
25 Feb      Normal         Normal         Normal         

PCA Event : 10MeV Proton/PCA Event Began 21 02 2014 0015UT and is in progress

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
26 Feb      Normal         Normal         Poor(PCA)
27 Feb      Normal         Normal         Normal
28 Feb      Normal         Normal         Normal


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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
25 Feb   116

Observed Australian Regional MUFs
  Northern Australian Region:
      Near predicted monthly values during local day.
      Enhanced by 30% during local night.
      Enhanced by 20% after local dawn.
   Southern Australian and New Zealand Region:
      Near predicted monthly values during local day.
      Enhanced by 15% during local night.
      Enhanced by 20% after local dawn.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Enhanced by 25% over the UT day.
      Proton event in progress, increased absorption observed.

Monthly T index:
Month  T index
Jan      119
Feb      75
Mar      75

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
26 Feb   110    Near to 15% above predicted monthly values
27 Feb   110    Near to 15% above predicted monthly values
28 Feb   110    Near to 15% above predicted monthly values

COMMENT: A strong short wave fadeout was observed across the 
region early in the UT day (~0050UT) for a couple of hours due 
to an X4.9 flare from sunspot group AR1990 newly rotated onto 
the disc (see Solar section). The SWF epicentre was NE of Australia 
and models indicated ALF for the east coast over 1500km path 
to be elevated from 5 to 20MHz. Many ionosondes showed 100% absorption 
across the HF band. AR1990 appears to hold further potential for 
X or at least M class flares and further SWFs should be expected. 
Observed MUF's for most of Australasia were near monthly median 
values during the day but enhanced 15-30% at night. This is possibly 
due to wind transport at night of enhanced ionisation from the 
daylight hemisphere due to increased ionising EUV/X-ray enhanced 
by numerous active regions on the disc. Geomagnetic activity 
expected to be Quiet for 26-28th Feb so ionosphere not expected 
to be too variable. 

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 24 Feb
       Daily Proton Fluence >1 MeV:   1.1E+05
       Daily Proton Fluence >10 MeV:  1.0E+04
       Daily Electron Fluence >2 MeV: 4.90E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B9.1

ACE Satellite Solar Wind Day Averaged Data for 24 Feb
Speed: 488 km/sec  Density:    1.5 p/cc  Temp:   121000 K  Bz:   2 nT

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