[Ips-dsgr] ASWFC Daily Report - 17 January 26 issued 2330 UT on 17 Jan 2026 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Sun Jan 18 10:30:50 AEDT 2026


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/17 JANUARY 2026
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 17 JANUARY AND FORECAST FOR 18 JANUARY - 20 JANUARY
STATUS INDICATORS SOL:** YELLOW **   MAG:** YELLOW **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 17 Jan:  R1

Flares    Max     Fadeout    Freq.  Sectors
  M2.1    1029UT  possible   lower  European

Observed 10.7 cm flux/Equivalent Sunspot Number for 17 Jan: 159/113


1B. SOLAR FORECAST
             18 Jan             19 Jan             20 Jan
Activity     R1, chance of R2   R1, chance of R2   R1, chance of R2
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   160/114            160/114            165/119

COMMENT: Solar flare activity reached the R1 level on UT day 
17-Jan, with an M2.1 flare peaking at 17/1029UT from Active Region 
(AR) 4341 (S11E32, beta-gamma-delta). This region is the largest 
and most magnetically complex of seven regions on the visible 
disk, and has remained mostly stable over the last 24 hours. 
It has also produced numerous C-class flares during this period. 
Active regions 4342 (N18E39, beta-gamma) and 4343 (S10W18, beta-gamma) 
have also produced several low-level C-class flares over the 
past UT day and have remained stable. AR 4344 (N20E28, beta) 
has shown some growth over the last UT day, while all other regions 
have remained stable or in decay. Solar flare activity is forecast 
to remain at the R1 level, with a chance of R2 activity, based 
on the flare activity of active regions 4341, 4342, and 4343. 
S0 solar radiation storm conditions were observed over the past 
24 hours, with the proton flux at background levels. S0 conditions 
are expected to persist over the period 18-20 Jan. No Earth-directed 
coronal mass ejections were observed in the past 24 hours in 
the available coronagraph imagery. The solar wind speed was elevated 
across 17-Jan, ranging between 680-750 km/s for most of the UT 
day. A discrete jump was observed at 17/0215UT, likely coinciding 
with a connection to a coronal hole high-speed wind stream. A 
decrease in the interplanetary magnetic field strength (IMF, 
Bt) was also observed at this time, dropping from a peak value 
of 12 nT down to 8 nT. The north-south component (Bz) of the 
magnetic field ranged between -9 and +10 nT, but has ranged between 
-6 and +7 nT since the high-speed wind stream connection. Connection 
to the coronal hole high-speed wind stream was also observed 
in ACE EPAM data, with an ion enhancement occurring at 17/0535UT. 
The solar wind stream is forecast to remain at very strong levels 
over 18-20 Jan due to these coronal hole high-speed wind stream 
effects.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 17 Jan: G0

Estimated Indices 17 Jan : A   K           
   Australian Region      15   33423333
      Cocos Island        10   32322322
      Darwin              17   33423334
      Townsville          16   33433333
      Learmonth           17   43433332
      Alice Springs       14   33423323
      Gingin              18   43433333
      Canberra            14   33323333
      Kennaook Cape Grim  16   33433333
      Hobart              15   33423333    

Estimated Antarctic Regional K Indices 17 Jan :
      Macquarie Island    23   44444432
      Casey               51   57743333
      Mawson              38   45644454

Observed Regional daily pc3 Indices 17 Jan : 
      Darwin              16   (Quiet)
      Townsville           0   (Quiet)
      Learmonth           15   (Quiet)
      Alice Springs        4   (Quiet)
      Gingin              84   (Minor storm)
      Canberra           106   (Major storm)
      Hobart             129   (Severe storm)

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 17 Jan : A 
           Fredericksburg        22
           Planetary             28                         

Observed AFr/Ap Indices 16 Jan :  A   K
           Fredericksburg        17
           Planetary             26   3433 4545     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
18 Jan    24    G1, chance of G2
19 Jan    20    G1
20 Jan    17    G0, chance of G1

COMMENT: ASWFC Geomagnetic Warning 5 was issued on 17 January 
and is current for 17-19 Jan. Geomagnetic activity was at the 
G0 level in the Australian region on UT day 17-Jan, with periods 
of G1-G3 observed in the Antarctic region, and a weak (14 nT) 
impulse was observed at 0610UT. G1 activity was reported at the 
planetary level due to the influence of a coronal hole high speed 
wind stream. G1 geomagnetic conditions, with a chance of G2, 
are forecast for 18-Jan due to these wind stream effects. This 
will decline to G1 on 19-Jan, and decrease to G0 with a chance 
of G1 on 20-Jan as this coronal hole rotates across the solar 
disk.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
18 Jan      Fair-normal    Fair-normal    Fair
19 Jan      Normal-fair    Normal-fair    Fair
20 Jan      Normal-fair    Normal-fair    Fair

COMMENT: Global ionospheric conditions were Normal-Fair on 17-Jan, 
with some depressions seen in the South African region, as well 
as degradations in the polar regions. MUFs were near predicted 
values in the European region. Ionospheric conditions are expected 
to become Fair-Normal on 18-Jan due to ongoing geomagnetic activity, 
trending towards Normal-Fair on 19-20 Jan as geomagnetic conditions 
ease. Shortwave fadeouts are possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
17 Jan    87

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

Monthly T index:
Month  T index
Dec      110
Jan      89
Feb      88

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
18 Jan    75    Depressed 10 to 15%/near predicted monthly values
19 Jan    70    Depressed 10 to 15%/near predicted monthly values
20 Jan    87    Near predicted monthly values

COMMENT: Maximum Usable Frequencies (MUFs) on UT day 17-Jan were 
mostly near predicted monthly values, with some enhancements 
seen in Niue Island. Strong spread-F and sporadic-E were observed 
in the Southern Australian region. MUFs were depressed in the 
Antarctic region by up to 20%. MUFs in the Australian region 
are expected to be depressed by 10-15% on 18-19 Jan due to coronal 
hole high-speed wind streams effects. These will likely trend 
towards predicted values on 20-Jan as the wind stream effects 
subside. Shortwave fadeouts are possible, and sporadic-E may 
be observed during local night hours.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 16 Jan
       Daily Proton Fluence >1 MeV:   4.0E+06
       Daily Proton Fluence >10 MeV:  1.5E+04
       Daily Electron Fluence >2 MeV: 1.10E+08   (moderate fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability:11%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B9.3

DSCOVR Satellite Solar Wind Day Averaged Data for 16 Jan
Speed: 673 km/sec  Density:    2.3 p/cc  Temp:   347000 K  Bz:   2 nT

(Courtesy Space Weather Prediction Center, Boulder USA)
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Australian Space Weather Forecasting Centre
Bureau of Meteorology
ASWFC at bom.gov.au
www.bom.gov.au | www.sws.bom.gov.au



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