[Ips-dsgr] ASWFC Daily Report - 07 January 26 issued 2331 UT on 07 Jan 2026 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Thu Jan 8 10:31:00 AEDT 2026


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/07 JANUARY 2026
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 07 JANUARY AND FORECAST FOR 08 JANUARY - 10 JANUARY
STATUS INDICATORS SOL:** YELLOW **   MAG:** RED **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 07 Jan:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 07 Jan: 135/89


1B. SOLAR FORECAST
             08 Jan             09 Jan             10 Jan
Activity     R1                 R1                 R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   132/86             130/84             130/84

COMMENT: Solar activity was at the R0 level throughout UT day 
07-Jan, with a C7.4 flare from Active Region (AR) 4334 (S15E08, 
beta) being the largest observed over the past 24 hours. This 
region is one of six numbered regions on the visible solar disk, 
with nearby AR 4336 (S09E41, beta) the largest and most magnetically 
complex. Both of these regions have remained mostly stable over 
the past UT day, with a redistribution of minor spots in both 
regions observed. A new active region emerged at N30W35, and 
appears to have a beta magnetic classification. All other regions 
appear stable or in decay, with four regions expected to rotate 
off the solar disk over the next UT day. Solar conditions are 
expected to reach R1 levels over 08-10 Jan. S0 solar radiation 
storm conditions were observed throughout 07-Jan, and are forecast 
to continue at the S0 level over the period 08-10 Jan. Two faint 
Coronal Mass Ejections (CMEs) were observed over the last 24 
hours. The first occurred at 07/0423UT in the southeast, appearing 
coincident with a low C-class flare in AR 4334. The second occurred 
at 07/1100UT, also appearing to originate from AR 4334. While 
these are both expected to miss the Earth, a small component 
of these CMEs may impact the Earth on 09-Jan. However, any effects 
from these CMEs will likely be secondary to high-speed wind stream 
effects from an equatorial coronal hole expected to connect with 
the Earth during this time. The solar wind speed was light over 
the last UT day, consistently ranging between 320-360 km/s. The 
interplanetary magnetic field strength (IMF, Bt) peaked at 10 
nT during 07-Jan, with the North-South component (Bz) ranging 
between -8 and +7 nT, and a prolonged period of southward Bz 
observed since 07/2030UT. The solar wind speed is expected to 
remain mostly light during 08-Jan, with a potential increase 
late in the UT day due to an equatorial coronal hole that will 
move into a geoeffective position by 09-Jan. The solar wind speed 
will then increase over 09-10 Jan due the high-speed wind stream 
effects of this coronal hole.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 07 Jan: G0

Estimated Indices 07 Jan : A   K           
   Australian Region       3   21001122
      Cocos Island         2   11011012
      Darwin               4   22101022
      Townsville           3   21001122
      Learmonth            3   21001122
      Alice Springs        3   22001022
      Gingin               4   21101122
      Canberra             3   11001122
      Kennaook Cape Grim   3   11001122
      Hobart               3   11001122    

Estimated Antarctic Regional K Indices 07 Jan :
      Macquarie Island     2   11000021
      Casey               15   44432222
      Mawson              10   23112243

Observed Regional daily pc3 Indices 07 Jan : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             0   (Quiet)
      Hobart               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 07 Jan : A 
           Fredericksburg         3
           Planetary              5                         

Observed AFr/Ap Indices 06 Jan :  A   K
           Fredericksburg         3
           Planetary              4   1012 2111     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
08 Jan    10    G0
09 Jan    30    G1
10 Jan    30    G1

COMMENT: G0 geomagnetic conditions were observed across the Australian 
and Antarctic regions during UT day 07-Jan. This was also observed 
at the planetary level. G0 conditions are expected for 08-Jan, 
rising to G1 on 09-10 Jan due to an equatorial coronal hole high-speed 
wind stream connecting with Earth, as well as effects from a 
possible glancing coronal mass ejection impact.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
08 Jan      Normal         Normal         Normal-fair
09 Jan      Fair-normal    Fair-normal    Fair
10 Jan      Fair-normal    Fair-normal    Fair

COMMENT: Ionospheric conditions were Normal-Fair during 07-Jan, 
with largely normal conditions reported at most sites. Some depressions 
were seen during local dawn hours in the South American and Asian 
regions. Depressions were also observed during local evening 
hours in the North American and European regions, with MUFs depressed 
up to 15% during local night in the European region, particularly 
at high latitudes. Conditions are forecast to be Normal over 
08-Jan, before becoming Fair-Normal over 09-10 Jan due to coronal 
hole high-speed wind stream effects. Shortwave fadeouts are possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
07 Jan   144

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values during local day.
      Enhanced by 25% during local night.
   Niue Island Region:
      Near predicted monthly values during local day.
      Enhanced by 15% during local night.
   Northern Australian Region:
      Enhanced by 15% during local day.
      Enhanced by 30% during local night.
   Southern Australian Region:
      Enhanced by 20% during local day.
      Enhanced by 20% 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
08 Jan   105    10 to 20% above predicted monthly values
09 Jan    80    Depressed 10 to 15% /near predicted monthly values
10 Jan    80    Depressed 10 to 15% /near predicted monthly values

COMMENT: Maximum useable frequencies (MUFs) in the Australian 
region were enhanced by 15-20% during UT day 07-Jan, with enhancements 
of up to 30% reported in the Northern Australian region. The 
Antarctic and Niue Island regions were near predicted monthly 
values. Strong sporadic-E affected mid- and polar latitudes during 
local night hours. 10-20% enhancements in MUFs are expected on 
08-Jan, then declining to be 10% depressed during 09-10 Jan due 
to coronal hole high-speed wind stream effects. Sporadic-E is 
possible during local night hours. Shortwave fadeouts are possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 06 Jan
       Daily Proton Fluence >1 MeV:   3.4E+05
       Daily Proton Fluence >10 MeV:  1.5E+04
       Daily Electron Fluence >2 MeV: 4.60E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 6%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C1.1

DSCOVR Satellite Solar Wind Day Averaged Data for 06 Jan
Speed: 369 km/sec  Density:    2.2 p/cc  Temp:    33500 K  Bz:   0 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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