[Ips-dsgr] ASWFC Daily Report - 26 August 25 issued 2331 UT on 26 Aug 2025 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Wed Aug 27 09:31:00 AEST 2025


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/26 AUGUST 2025
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 26 AUGUST AND FORECAST FOR 27 AUGUST - 29 AUGUST
STATUS INDICATORS SOL:** RED **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 26 Aug:  R1

Flares    Max     Fadeout    Freq.  Sectors
  M3.3    0030UT  possible   lower  West Pacific
  M4.5    0525UT  possible   lower  E. Asia/Aust.
  M1.0    1407UT  possible   lower  South American/
                                    Atlantic

Observed 10.7 cm flux/Equivalent Sunspot Number for 26 Aug: 202/153


1B. SOLAR FORECAST
             27 Aug             28 Aug             29 Aug
Activity     R1-R2              R1-R2              R1-R2
Fadeouts     Probable           Probable           Probable
10.7cm/SSN   200/152            200/152            205/156

COMMENT: Solar activity on UT day 26-Aug was at the R1 level 
due to three M-class flares, the largest of which was an M4.5 
flare at 26/0525UT produced by AR4197 (S17E46, beta). There are 
currently thirteen numbered sunspot regions visible on the solar 
disk. AR4191 (N13E05, beta-gamma) has exhibited spot development 
over the UT day, particularly in its intermediate spots. AR4200 
(S08E01, beta-gamma) recently appeared on the solar disk and 
has shown spot growth. AR4197 has shown spot growth in both its 
leader and trailer spots but has overall become less compact, 
with a clear gap now separating the leader and trailer groups. 
This region has also become less magnetically complex over the 
UT day. AR4199 (N08E56, beta) has shown slight decay over the 
24-hour period. AR4190 (N20W20, beta), AR4198 (N11E24, beta) 
and AR4201 (S18E55, beta) have all shown slight growth. All other 
sunspot regions are either stable or in decay. Solar activity 
is expected at R1-R2 levels over 27-29 Aug. S1 solar proton conditions 
were observed on UT day 26-Aug. S0-S1 solar proton conditions 
are expected over 27-29 Aug due to ongoing effects from a farside 
eruption on 21-Aug. Several CMEs were observed, but none are 
considered geoeffective. A southeast-directed CME was observed, 
visible in STEREO-A coronagraph imagery from 26/0609UT. This 
CME is considered to be associated with the aforementioned M4.5 
flare from AR4197. Modelling indicates this low velocity CME 
does not contain a geoeffective component. A second southeast-directed 
CME was observed at 26/1348UT in LASCO C2 coronagraph imagery. 
Modelling indicates this CME is not Earth-directed. The solar 
wind speed on UT day 26-Aug decreased, ranging from 325 to 420 
km/s and is currently near 365 km/s. The peak total interplanetary 
magnetic field strength (IMF, Bt) was 8 nT and the north-south 
IMF component (Bz) range was -7 to +7 nT. The solar wind speed 
is expected to remain near background levels over 27-29 Aug.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 26 Aug: G0

Estimated Indices 26 Aug : A   K           
   Australian Region       4   22221001
      Cocos Island         3   22221000
      Darwin               7   33221112
      Townsville           7   23231022
      Learmonth            3   22121001
      Alice Springs        4   22221001
      Gingin               4   22221001
      Canberra             5   22230002
      Kennaook Cape Grim   4   12231001
      Hobart               5   22231002    

Estimated Antarctic Regional K Indices 26 Aug :
      Macquarie Island     8   13143001
      Casey                9   33331112
      Mawson              19   26432013

Observed Regional daily pc3 Indices 26 Aug : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin              12   (Quiet)
      Canberra            18   (Quiet)
      Hobart              30   (Quiet to unsettled)

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 26 Aug : A 
           Fredericksburg         9
           Planetary             10                         

Observed AFr/Ap Indices 25 Aug :  A   K
           Fredericksburg         8   0112 4221
           Planetary              8   1111 3322     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
27 Aug    10    G0
28 Aug     8    G0
29 Aug     6    G0

COMMENT: G0 geomagnetic conditions were observed in the Australian 
region on UT day 26-Aug. Mostly G0 geomagnetic conditions were 
observed in the Antarctic region, with an isolated period of 
G2 observed at Mawson. G0 geomagnetic conditions are expected 
over 27-29 Aug.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
26 Aug      Normal         Normal         Poor(PCA)      

PCA Event : 10MeV Proton/PCA Event Began 26 08 2025 2040UT and is in progress

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
27 Aug      Normal         Normal         Poor(PCA)
28 Aug      Normal         Normal         Poor(PCA)
29 Aug      Normal         Normal         Poor(PCA)

COMMENT: HF radio propagation conditions on UT day 26-Aug were 
mostly normal at low and mid latitudes. A polar cap absorption 
(PCA) event began on 26-Aug and is ongoing, affecting high latitude 
radio communication. HF radio propagation conditions are expected 
to be mostly normal over 27-29 Aug, with poor conditions at high 
latitudes due to an ongoing PCA event. Shortwave fadeouts are 
probable.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
26 Aug   101

Observed Australian Regional MUFs
   Cocos Island Region:
      No data available.
   Niue Island Region:
      Enhanced by 25% during local day.
      Enhanced by 15% during local night.
   Northern Australian Region:
      Enhanced by 15% during local day.
      Enhanced by 25% during local night.
   Southern Australian Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Davis/Mawson):
      Near predicted monthly values over the UT day.
      Proton event in progress, increased absorption observed.

Monthly T index:
Month  T index
Jul      88
Aug      96
Sep      93

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
27 Aug   100    Near predicted monthly values
28 Aug   100    Near predicted monthly values
29 Aug   100    Near predicted monthly values

COMMENT: ASWFC SWF HF Communications Warning 76 was issued on 
25 August and is current for 25-27 Aug. Maximum usable frequencies 
(MUFs) in the Australian region on UT day 26-Aug were near predicted 
monthly values to 25% enhanced. MUFs are expected to be near 
predicted monthly values over 27-29 Aug. Shortwave fadeouts are 
probable.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 25 Aug
       Daily Proton Fluence >1 MeV:   3.5E+06
       Daily Proton Fluence >10 MeV:  6.7E+05
       Daily Electron Fluence >2 MeV: 4.10E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 6%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C2.1

DSCOVR Satellite Solar Wind Day Averaged Data for 25 Aug
Speed: 409 km/sec  Density:    3.6 p/cc  Temp:   102000 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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