[Ips-dsgr] ASWFC Daily Report - 05 September 25 issued 2330 UT on 05 Sep 2025 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Sat Sep 6 09:30:57 AEST 2025


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/05 SEPTEMBER 2025
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 05 SEPTEMBER AND FORECAST FOR 06 SEPTEMBER - 08 SEPTEMBER
STATUS INDICATORS SOL:** YELLOW **   MAG:** YELLOW **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 05 Sep:  R1

Flares    Max     Fadeout    Freq.  Sectors
  M1.4    0116UT  possible   lower  West Pacific

Observed 10.7 cm flux/Equivalent Sunspot Number for 05 Sep: 149/104


1B. SOLAR FORECAST
             06 Sep             07 Sep             08 Sep
Activity     R0-R1              R0-R1              R0-R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   140/94             140/94             138/92

COMMENT: Solar activity on UT day 05-Sep was at the R1 level 
due to an M1.4 flare from AR4207 (N31E01, beta-gamma). This medium 
sized solar region is currently the largest and most magnetically 
complex region on the solar disk and is showing decay in its 
trailer spots. Solar region AR4197 (S18W87, beta) which was a 
recent region of interest showed decay as it rotated off the 
visible solar disk. Most of the on disk solar regions are relatively 
small. There are currently nine numbered sunspot regions visible 
on the solar disk. All other sunspot regions are either stable 
or in decay. Solar activity is expected to be at the R0-R1 level 
over 06-08 Sep. S0 solar radiation storm conditions were observed 
on UT day 05-Sep. S0 solar radiation storm conditions are expected 
over 06-08 Sep. Two solar filament eruptions have recently been 
observed. A small north south orientated 8 degree long filament 
located at N10W05 erupted at 04/1912 with narrow southward and 
later southeast directed plasma motion visible in SDO304 imagery 
from 04/1937UT. A minor southwest CME was observed in LASCO C2 
first visible from 04/1812UT. As this CME precedes the time of 
the small filament eruption it has not been paired to this event. 
A very faint CME was observed in LASCO C2 to the southeast from 
04/1948UT and a narrow south directed CME was observed from 04/2200UT. 
These CMEs match the dark southward and partial east directed 
plasma motion visible in SDO304 imagery and have been paired 
to the small filament eruption. The narrow southward CME is not 
considered to be significantly Earth directed as it is predominately 
directed southward out of the ecliptic plane and is too narrow 
to model. The very faint southeast component of the CME has been 
modelled and may arrive at the Earth on 07-Sep at 1000UT +/- 
12 hours, though modelling indicates most of the CME will pass 
behind the Earth. A 22 degree long east west orientated solar 
filament with centre located at N18E25 partially lifted off from 
05/0434UT visible in GONG H-alpha imagery. No significant CME 
appeared to follow this larger slower partial filament eruption 
on 05-Sep. A north-northwest CME was also observed from 05/0136UT, 
directed northward out of the ecliptic plane. A broad coronal 
hole spans across the solar disk in the southern solar hemisphere. 
The solar wind speed on UT day 05-Sep was steady and slightly 
elevated, ranging from 387 to 488 km/s and is currently near 
405 km/s. The peak total interplanetary magnetic field strength 
(IMF, Bt) was 10 nT and the north-south IMF component (Bz) range 
was -7 to +7 nT. The solar wind speed is expected to increase 
over 06-07 due to the wind stream from the coronal hole located 
in the southern solar hemisphere.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 05 Sep: G0

Estimated Indices 05 Sep : A   K           
   Australian Region       4   11121122
      Cocos Island         4   11121022
      Darwin               5   11121123
      Townsville           5   11121123
      Learmonth            6   21121132
      Alice Springs        4   11121022
      Gingin               5   21120132
      Canberra             4   10121122
      Kennaook Cape Grim   4   11121122
      Hobart               4   11121122    

Estimated Antarctic Regional K Indices 05 Sep :
      Macquarie Island     4   00041111
      Casey               11   33322133
      Mawson              34   32223276

Observed Regional daily pc3 Indices 05 Sep : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             8   (Quiet)
      Hobart               7   (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 05 Sep : A 
           Fredericksburg        11
           Planetary             14                         

Observed AFr/Ap Indices 04 Sep :  A   K
           Fredericksburg        10
           Planetary             10   2123 2323     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
06 Sep    15    G0-G1
07 Sep    20    G1
08 Sep    15    G0-G1

COMMENT: ASWFC Geomagnetic Warning 64 was issued on 5 September 
and is current for 6-7 Sep. G0 geomagnetic conditions were observed 
in the Australian region on UT day 05-Sep. In the Antarctic region 
G0 geomagnetic conditions were observed at Macquarie Island and 
Casey with an isolated G3 period at Mawson. G0-G1 geomagnetic 
conditions are generally expected on 06-08 Sep due to a solar 
coronal hole wind stream, with G1 periods expected for the second 
half of the UT day on 07-Sep due to a CME glancing blow from 
a recent small solar filament eruption.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
05 Sep      Normal         Fair-normal    Fair           

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
06 Sep      Normal         Fair-normal    Fair
07 Sep      Normal         Fair-normal    Fair
08 Sep      Normal         Fair-normal    Fair

COMMENT: HF radio propagation conditions on UT day 05-Sep were 
fair to normal. HF radio propagation conditions are generally 
expected to be mildly degraded at middle to high latitudes over 
06-08 Sep. HF conditions may be moderately degraded at middle 
to high latitudes from the second half of the UT day 07-Sep due 
to a possible weak CME arrival. Isolated minor shortwave fadeouts 
are possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
05 Sep   114

Observed Australian Regional MUFs
   Cocos Island Region:
      No data available.
   Niue Island Region:
      Enhanced by 15% during local day.
      Enhanced by 30% during local night.
      Enhanced by 20% after local dawn.
   Northern Australian Region:
      Near predicted monthly values during local day.
      Enhanced by 25% during local night.
   Southern Australian Region:
      Near predicted monthly values during local day.
      Enhanced by 15% during local night.
   Antarctic Region (Casey/Davis/Mawson):
      Near predicted monthly values over the UT day.

Monthly T index:
Month  T index
Aug      96
Sep      92
Oct      90

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
06 Sep   100    Near predicted monthly values
07 Sep   100    Near predicted monthly values
08 Sep    80    15% depressed to near predicted monthly values

COMMENT: Maximum usable frequencies (MUFs) in the northern Australian 
region on UT day 05-Sep were near predicted monthly values to 
30% enhanced. Enhanced MUFs were observed during local night 
hours. Spread F was observed at Hobart during local night hours. 
MUFs are generally expected to be near to predicted monthly values 
over 06-08 Sep with degraded HF conditions during local night 
hours for the southern Australian region. Mild depressions of 
15% may be experienced after local dawn for the southern Australian 
region. MUFs for the southern Australian region may become 15% 
depressed on 08-Sep due to a possible weak CME arrival on 07-Sep. 
Isolated minor shortwave fadeouts are possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 04 Sep
       Daily Proton Fluence >1 MeV:   1.4E+06
       Daily Proton Fluence >10 MeV:  1.6E+04
       Daily Electron Fluence >2 MeV: 1.50E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 3%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C1.5

DSCOVR Satellite Solar Wind Day Averaged Data for 04 Sep
Speed: 463 km/sec  Density:    0.7 p/cc  Temp:   109000 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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