[Ips-dsgr] ASWFC Daily Report - 22 January 26 issued 2330 UT on 22 Jan 2026 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Fri Jan 23 10:30:51 AEDT 2026


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/22 JANUARY 2026
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 22 JANUARY AND FORECAST FOR 23 JANUARY - 25 JANUARY
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 22 Jan:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 22 Jan: 194/146


1B. SOLAR FORECAST
             23 Jan             24 Jan             25 Jan
Activity     R1-R2              R1-R2              R1-R2   
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   192/144            192/144            190/143

COMMENT: Solar flare activity was at the R0 level on UT day 22-Jan, 
with a C9.5 flare from Active Region (AR) 4350 (N20E20, alpha) 
at 22/1954UT being the largest observed. There are currently 
nine numbered active regions on the disk, with AR 4345 (S16W25, 
beta) being the largest and most magnetically complex. This region 
has exhibited some minor growth over the previous UT day, with 
regions 4350, 4351 (S04E11, beta), and 4354 (S13E14, beta) also 
showing growth over the last 24 hours. A new unnumbered region 
has rotated over the eastern limb at (S11E80). While this region 
is coincident with a possible return of previously flare-active 
region 4325, this new region appears small and magnetically simple. 
All other regions on the disk are either stable or in decay. 
Solar flare activity is expected to reach R1-R2 levels over the 
period 23-25 Jan. Solar radiation storm conditions briefly reached 
the S1 level at 22/0500UT, with the proton flux ranging between 
2.16-10.6 pfu throughout the day. The solar proton flux is expected 
to decline over 23-Jan, with S0 solar radiation storm conditions 
are forecast, with a chance of reaching S1. S0 conditions are 
forecast over Jan 24-25, as the proton flux continues to trend 
toward background levels. No Earth-directed Coronal Mass Ejections 
(CMEs) were observed over the past 24 hours. A small, narrow 
CME associated with a filament eruption was observed in SOHO 
coronagraph imagery at 22/0224UT. Subsequent modelling has determined 
this event will not impact the Earth. The solar wind continued 
to decline on UT day 22-Jan, with the wind speed declining from 
600-630 km/s early in the UT day to 500-530 km/s over the last 
six hours. The interplanetary magnetic field strength (IMF, Bt) 
peaked at 11 nT during 22-Jan, with the North-South component 
(Bz) ranging between -7 and +8 nT during this time. An extended 
period of southward Bz began at 22/2045UT and is ongoing. The 
solar wind is expected to slowly trend towards background levels 
over 23-25 Jan as the effects of a previous CME that impacted 
Earth on 19-Jan continue to subside, and a coronal high speed 
wind stream moves out of a geoeffective position.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 22 Jan: G0

Estimated Indices 22 Jan : A   K           
   Australian Region      10   32232223
      Cocos Island         6   22222212
      Darwin              10   32232223
      Townsville          11   32233223
      Learmonth           11   32233313
      Alice Springs        9   32232213
      Gingin               9   32322222
      Canberra            11   33332113
      Kennaook Cape Grim  12   33332223
      Hobart              12   33332223    

Estimated Antarctic Regional K Indices 22 Jan :
      Macquarie Island     8   22322213
      Casey               31   45653233
      Mawson              32   55433336

Observed Regional daily pc3 Indices 22 Jan : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               4   (Quiet)
      Canberra            38   (Quiet to unsettled)
      Hobart              83   (Minor 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 22 Jan : A 
           Fredericksburg        12
           Planetary             13                         

Observed AFr/Ap Indices 21 Jan :  A   K
           Fredericksburg        45
           Planetary             73   7776 4433     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
23 Jan     9    G0
24 Jan    10    G0
25 Jan     9    G0

COMMENT: Geomagnetic conditions in the Australian region were 
at G0 levels on UT day 22-Jan, as the effects of a previous coronal 
mass ejection impact continue to ease. G0 conditions were also 
observed at the planetary level, with some intervals of G1-G2 
activity reported in the Antarctic region. G0 conditions are 
forecast for 23-25 Jan, as geomagnetic effects from both the 
previously mentioned CME, and a coronal hole high speed wind 
stream both continue to subside.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
22 Jan      Fair-normal    Fair-normal    Fair-normal    

PCA Event : 10MeV Proton/PCA Event Began at 2240UT 18/01, Ended at 1640UT 21/01

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
23 Jan      Normal-fair    Normal-fair    Fair-normal
24 Jan      Normal         Normal         Normal-fair
25 Jan      Normal         Normal         Normal-fair

COMMENT: Global ionospheric conditions continued to improve over 
UT day 22-Jan following geomagnetic activity from a coronal mass 
ejection impact on 19-Jan. Conditions were observed to be Fair 
at many sites across the globe at the beginning of the UT day, 
but improved towards Normal conditions by the end of the UT day. 
MUFs in the European region were depressed 20% during local night, 
but recovered towards predicted values during local daytime. 
Ionospheric conditions are forecast to continue to recover, improving 
to Normal-Fair on 23-Jan, trending towards Normal conditions 
on 24-25 Jan. Shortwave fadeouts are possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
22 Jan    85

Observed Australian Regional MUFs
   Cocos Island Region:
      Depressed by 35% during local day.
      Depressed by 25% during local night.
      Depressed by 20% after local dawn.
   Niue Island Region:
      Enhanced by 35% during local day.
      Enhanced by 55% during local night.
      Enhanced by 30% after local dawn.
   Northern Australian Region:
      Enhanced by 20% during local day.
      Near predicted monthly values during local night.
   Southern Australian Region:
      Depressed by 20% during local day.
      Near predicted monthly values during local night.
   Antarctic Region (Casey/Davis/Mawson):
      Near predicted monthly values 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
23 Jan    70    Near predicted monthly values
24 Jan    80    Near predicted monthly values
25 Jan    81    Near predicted monthly values

COMMENT: ASWFC SWF HF Communications Warning 14 was issued on 
21 January and is current for 21-23 Jan. Ionospheric conditions 
continued to recover in the Australian region on UT day 22-Jan 
following the coronal mass ejection impact with Earth on 19-Jan. 
Maximum Usable Frequencies (MUFs) in the Australian region trended 
towards near predicted monthly values over the UT day, with some 
enhancements seen in northern Australia and Niue Island. Strong 
sporadic E was visible during night hours in southern Australia, 
and spread F was observed in Hobart. MUFs will continue to trend 
towards predicted monthly values over 23-25 Jan, with some enhancements 
possible. Sporadic E may be observed during local night hours, 
and shortwave fadeouts are possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 21 Jan
       Daily Proton Fluence >1 MeV:   4.7E+07
       Daily Proton Fluence >10 MeV:  1.3E+06
       Daily Electron Fluence >2 MeV: 7.00E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 8%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C1.1

DSCOVR Satellite Solar Wind Day Averaged Data for 21 Jan
Speed: 660 km/sec  Density:    0.4 p/cc  Temp:    80200 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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