[Ips-dsgr] SWS Daily Report - 16 February 17 issued 2330 UT on 16 Feb 2017 [SEC=UNCLASSIFIED]

Regional Warning Centre rwc at sws.bom.gov.au
Fri Feb 17 10:30:39 EST 2017


SUBJ: SWS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/16 FEBRUARY 2017 BY Space Weather Services
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 16 FEBRUARY AND FORECAST FOR 17 FEBRUARY - 19 FEBRUARY
STATUS INDICATORS SOL:GREEN   MAG:** YELLOW **     ION: ** YELLOW **
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1A. SOLAR SUMMARY
Activity 16 Feb:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 16 Feb:  74/11


1B. SOLAR FORECAST
             17 Feb             18 Feb             19 Feb
Activity     Very low to low    Very low to low    Very low to low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    74/11              74/11              74/11

COMMENT: The solar activity was at very low levels during the 
UT day 16 February, with no flares. There are currently three 
numbered sunspot regions on the visible solar disk. Very low 
levels of solar activity are expected for the next 3 days (17-19 
February) with a slight chance of C-class flares. No Earth directed 
CMEs were observed in available LASCO imagery on UT day 16 February. 
The solar wind speeds increased gradually from the nominal levels 
of ~300 km/s at the beginning of the UT to ~450 km/s by the end 
of the UT day. This was in response to the high speed streams 
emanating from a recurrent positive polarity coronal hole now 
taking geoeffective location on the solar disk. The IMF Bt fluctuated 
between 4 nT and 11 nT. The Bz component varied between -8 nT 
and +6 nT, with a significant southward component between 16/1200 
UT and 16/1400 UT. The two day outlook (17-18 February) is for 
the solar winds to enhance further since the high speed streams 
from the coronal is expected to persist for few days.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 16 Feb: Quiet to Unsettled

Estimated Indices 16 Feb : A   K           
   Australian Region       8   12213331
      Cocos Island         8   12213331
      Darwin               6   12202231
      Townsville           8   12213331
      Learmonth            9   12213332
      Alice Springs        6   02203231
      Norfolk Island       7   12203321
      Culgoora             7   02203331
      Gingin               7   11213232
      Canberra             5   02203220
      Launceston          11   02314332    

Estimated Antarctic Regional K Indices 16 Feb :
      Macquarie Island    18   02205620
      Casey               11   34312222
      Mawson              20   23324435

Observed Regional daily pc3 Indices 16 Feb : 
      Darwin               0   (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 16 Feb : A 
           Fredericksburg         8
           Planetary             10                         

Observed AFr/Ap Indices 15 Feb :  A   K
           Fredericksburg         2
           Planetary              3   1010 1011     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
17 Feb    16    Active
18 Feb    10    Quiet to Unsettled
19 Feb    10    Quiet to Unsettled

COMMENT: SWS Geomagnetic Warning 7 was issued on 16 February 
and is current for 17 Feb only. Magnetic activity were mostly 
between quiet and unsettled levels across the Australian region 
on UT day 16 February. Active geomagnetic conditions were observed 
in high latitude regions. The Australia DST index dipped to minimum 
of -34 nT at 16/1500 UT following the period of significant southward 
IMF Bz. The unsettled conditions were caused by the arrival of 
co-rotating interaction region associated with the coronal hole. 
The outlook for today 17 February for geomagnetic conditions 
to be mostly between unsettled and active levels, occasionally 
reaching minor storm levels associated with the high speed solar 
wind streams emanating from the coronal hole. There is some chance 
that auroras may be visible on the local night of 17 February 
in Tasmania and possibly from the coastline of Victoria.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
17 Feb      Normal         Normal-fair    Fair
18 Feb      Normal         Normal         Normal-fair
19 Feb      Normal         Normal         Normal-fair

COMMENT: Minor to mild depressions in MUFs were observed on UT 
day 16 February in the high southern hemisphere regions. Other 
regions were near monthly predicted levels. Slightly poor HF 
conditions are expected today, 17 February, with the high latitude 
depressions possibly extending into the mid-latitude regions. 
This is response to the current disturbed conditions associated 
with the coronal hole.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
16 Feb    13

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

Monthly T index:
Month  T index
Jan      0
Feb      18
Mar      16

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
17 Feb    -3    Depressed 15%/near predicted monthly values
18 Feb    -5    Depressed 15%/near predicted monthly values
19 Feb    -3    Depressed 15%/near predicted monthly values

COMMENT: SWS HF Communications Warning 14 was issued on 16 February 
and is current for 17-19 Feb. MUFs were near monthly predicted 
values in the mid- and low-latitude regions of Australia on UT 
day 16 February. Minor depressions were observed in the high-latitude 
Australian regions during the latter part of the UT day. Over 
the next two days (17-18 February), the high latitude depressions 
are expected to extend into the mid latitude regions as disturbed 
geomagnetic conditions associated with the coronal hole persist. 
HF users are advised to use lower than the monthly predicted 
frequencies.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 15 Feb
       Daily Proton Fluence >1 MeV:   1.0E+06
       Daily Proton Fluence >10 MeV:  1.5E+04
       Daily Electron Fluence >2 MeV: 3.90E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 6%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A5.9

ACE Satellite Solar Wind Day Averaged Data for 15 Feb
Speed: 306 km/sec  Density:   11.1 p/cc  Temp:    17900 K  Bz:   0 nT

(Courtesy Space Weather Prediction Center, Boulder USA)
ACE data can be incorrect during strong proton events.
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Space Weather Services              email: asfc at bom.gov.au
Bureau of Meteorology
PO Box 1386                         WWW: http://www.sws.bom.gov.au
Haymarket NSW 1240  AUSTRALIA       FTP: ftp://ftp-out.sws.bom.gov.au
tel: +61 2 9213 8010                fax: +61 2 9213 8060 

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