[Ips-dsgr] SWS Daily Report - 03 January 19 issued 2330 UT on 03 Jan 2019 [SEC=UNCLASSIFIED]

Regional Warning Centre rwc at ips.gov.au
Fri Jan 4 10:30:20 EST 2019


SUBJ: SWS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/03 JANUARY 2019 BY Space Weather Services
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 03 JANUARY AND FORECAST FOR 04 JANUARY - 06 JANUARY
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 03 Jan:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 03 Jan:  73/9


1B. SOLAR FORECAST
             04 Jan             05 Jan             06 Jan
Activity     Very low to low    Very low to low    Very low to low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    72/8               72/8               70/5

COMMENT: Solar activity was very low on UT day 3 January. There 
is currently one active region on the visible solar disc, AR 
2732. During the next three UT days, 4-6 January, solar activity 
is expected to remain mostly very low with a small chance for 
C-class flares. A 52 deg long disappearing solar filament was 
observed from 3/1804 UT to 3/1948 UT. No Earth directed CMEs 
were observed in the available coronagraph imagery. The solar 
wind speed during the last 24 hours varied in the range 290-330 
km/s, currently at 310 km/s. During this period the total IMF 
(Bt) varied in the range 2-5 nT and the north-south component 
of IMF (Bz) fluctuated between -3 nT and +2 nT. On 4 January, 
the solar wind speed may increase up to moderate levels due to 
expected arrival of the corotating interaction region and high 
speed solar wind streams associated with a recurrent coronal 
hole.

-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 03 Jan: Quiet

Estimated Indices 03 Jan : A   K           
   Australian Region       1   11110001
      Cocos Island         1   11100000
      Darwin               2   21010001
      Townsville           1   11010001
      Learmonth            0   11000000
      Alice Springs        1   11000001
      Culgoora             1   00110001
      Gingin               1   11110000
      Canberra             0   00010001
      Launceston           2   11111001
      Hobart               1   10111000    

Estimated Antarctic Regional K Indices 03 Jan :
      Casey                4   22221001
      Mawson               4   31011012
      Davis                4   12121111

Observed Regional daily pc3 Indices 03 Jan : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             0   (Quiet)
      Melbourne           NA

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 03 Jan : A 
           Fredericksburg         2
           Planetary              3                         

Observed AFr/Ap Indices 02 Jan :  A   K
           Fredericksburg         1
           Planetary              2   0000 1100     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
04 Jan    10    Quiet to Unsettled
05 Jan    10    Quiet to Unsettled
06 Jan    10    Quiet to Unsettled

COMMENT: Quiet geomagnetic conditions were observed in the Australian 
region on UT day 3 January. Mostly quiet conditions were observed 
in Antarctica. During the next 3 UT days, 4-6 January, the global 
geomagnetic activity is expected to vary mostly between quiet 
and unsettled levels. The predicted increase in geomagnetic activity 
is due to expected arrival of the corotating interaction region 
and high speed solar wind streams associated with a recurrent 
coronal hole.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
04 Jan      Normal-fair    Normal-fair    Normal-fair
05 Jan      Normal-fair    Normal-fair    Normal-fair
06 Jan      Normal-fair    Normal-fair    Normal-fair

COMMENT: Mild MUF depressions are possible on 4 January as a 
consequence of the continued very low levels of ionising radiation 
from the Sun.

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


Date   T index
03 Jan   -33

Observed Australian Regional MUFs
   Cocos Island Region:
      No data available during local day.
      No data available 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.
   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
Dec      -32
Jan      -12
Feb      -13

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
04 Jan   -30    Near predicted monthly values/depressed 10 to 
                30%
05 Jan   -30    Near predicted monthly values/depressed 10 to 
                30%
06 Jan   -30    Near predicted monthly values/depressed 10 to 
                30%

COMMENT: SWS HF Communications Warning 2 was issued on 3 January 
and is current for 4 Jan only. Mostly near predicted monthly 
MUFs were observed on 3 January across the Australian region; 
mild MUF depressions were also seen, mostly in the Northern Australian 
region. Strong Sporadic E layers were seen across the Australian 
region and in Antarctica. Similar levels of ionospheric support 
are expected for the next 3 UT days, 4-6 January, with mild depressions 
being likely due to continued very low levels of ionising radiation 
from the Sun and predicted increase in geomagnetic activity.

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

GOES satellite data for 02 Jan
       Daily Proton Fluence >1 MeV:   6.5E+05
       Daily Proton Fluence >10 MeV:  1.7E+04
       Daily Electron Fluence >2 MeV: 3.40E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 5%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.9

DSCOVR Satellite Solar Wind Day Averaged Data for 02 Jan
Speed: 355 km/sec  Density:    2.4 p/cc  Temp:    29300 K  Bz:   0 nT

(Courtesy Space Weather Prediction Center, Boulder USA)
-----------------------------------------------------------

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 

IMPORTANT: This e-mail, including any attachments, may contain,
confidential or copyright information.  The views expressed in 
this message are those of the individual sender, unless 
specifically stated to be the views of SWS.  If you are not 
the intended recipient, please contact the sender immediately 
and delete all copies of this e-mail and attachments. 
To unsubscribe from an IPS mail list either send an email to 
"MAIL_LIST"-leave at ips.gov.au or go to
http://www.sws.bom.gov.au/mailman/listinfo/"MAIL_LIST".
Information about training can be obtained from
http://www.sws.bom.gov.au/mailman/listinfo/ips-training.
General information is available from
http://www.sws.bom.gov.au/mailman/listinfo/ips-info.




More information about the ips-dsgr mailing list