[Ips-dsgr] ASWFC Daily Report - 16 September 25 issued 2330 UT on 16 Sep 2025 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Wed Sep 17 09:30:49 AEST 2025


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/16 SEPTEMBER 2025
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 16 SEPTEMBER AND FORECAST FOR 17 SEPTEMBER - 19 SEPTEMBER
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 16 Sep:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 16 Sep: 135/89


1B. SOLAR FORECAST
             17 Sep             18 Sep             19 Sep
Activity     R0, chance of R1   R0, chance of R1   R0, chance of R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   138/92             138/92             140/94

COMMENT: Solar activity on UT day 16-Sep was at R0. There are 
currently nine numbered regions visible on the solar disk. AR4216 
(N11E17,beta) is the largest region on the disk and has shown 
a mixture of growth and slight decay in its intermediate spots. 
AR4217 (S15E48,beta) has showed a reorganisation of its leaders 
spots. AR4221 (N04E45,beta) has shown some growth in the leader 
spot. AR4220 (S18E15,beta) and AR4224(S10E50,beta) are both small 
regions which have shown some growth over the UT day. AR4225 
(N14E80,beta) is a new larger spot which has rotated onto the 
solar disk which appears beta complexity however is difficult 
to classify noting its proximity to the limb. All other sunspot 
regions are either stable or in decay. Solar activity is expected 
to be at the R0, chance of R1 over 17-19 Sep. No Earth directed 
CMEs have been observed however several eastward non earth directed 
CME were observed. Early in the UT day a southeast directed CME 
was observed in association with an erupting east limb solar 
prominence. Plasma ejecta was observed in SUVI 094 imagery at 
16/1240UT possibly attributed to C class flare activity from 
AR4223 and a corresponding CME observed in LASCO C2 imagery from 
16/1524UT. The small CME was slow moving and unlikely to impact 
earth. Two small disappearing solar filaments were observed, 
S30E20 at 16/1338UT and N22W22 at 16/1501UT with no associated 
CMEs observed. S0 solar radiation storm conditions were observed 
on UT day 16-Sep. S0 solar radiation storm conditions are expected 
over 17-19 Sep. The solar wind speed on UT day 16-Sep remained 
elevated throughout the day ranging from 670 to 800 km/s and 
is currently near 670 km/s. The solar wind speed is very strong 
and is expected to start to decline over 17 Sep due to the coronal 
hole moving out of a geoeffective position. The peak total interplanetary 
magnetic field strength (IMF, Bt) was 6 nT and the north-south 
IMF component (Bz) range was -5 to +6nT.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 16 Sep: G0

Estimated Indices 16 Sep : A   K           
   Australian Region      12   33333222
      Cocos Island         6   22322111
      Darwin              13   33333223
      Townsville          13   33343222
      Learmonth           13   33333322
      Alice Springs       12   33333222
      Gingin              13   33333322
      Canberra            13   33433222
      Kennaook Cape Grim  15   33443222
      Hobart              15   33443222    

Estimated Antarctic Regional K Indices 16 Sep :
      Macquarie Island    26   33555332
      Casey               19   45433222
      Mawson              47   55553366

Observed Regional daily pc3 Indices 16 Sep : 
      Darwin              14   (Quiet)
      Townsville           4   (Quiet)
      Learmonth           23   (Quiet to unsettled)
      Alice Springs       13   (Quiet)
      Gingin             103   (Major storm)
      Canberra           107   (Major storm)
      Hobart             103   (Major 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 16 Sep : A 
           Fredericksburg        17
           Planetary             22                         

Observed AFr/Ap Indices 15 Sep :  A   K
           Fredericksburg        34
           Planetary             48   7555 5544   


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
17 Sep    14    G0, chance of G1
18 Sep    10    G0
19 Sep    10    G0

COMMENT: G0 geomagnetic conditions were observed in the Australian 
and G1 with isolated G2 conditions in Antarctic regions on UT 
day 16-Sep. Planetary conditions briefly reached G1 early in 
the UT day in association with a brief southward IMF conditions 
during very strong winds due to a coronal hole. The wind stream 
from this coronal hole is a chance of causing isolated periods 
of G1 geomagnetic conditions on 17-Sep. G0 conditions are expected 
on 18-19 Sep.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
17 Sep      Normal         Normal         Normal-fair
18 Sep      Normal         Normal         Normal-fair
19 Sep      Normal         Normal         Normal-fair

COMMENT: HF radio propagation conditions on UT day 16-Sep were 
degraded at high latitudes. HF radio propagation conditions are 
expected to be normal, grading fair to normal over high latitudes 
over 17-19 Sep due to declining geomagnetic activity induced 
by coronal hole wind stream. Increased absorption of up to 2db 
was observed at times between 16/0000-0200UT and 16/1200-1500UT 
at Macquarie Island.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
16 Sep    96

Observed Australian Regional MUFs
   Cocos Island Region:
      No data available.
   Niue Island Region:
      Mostly near predicted monthly values.
   Northern Australian Region:
      Near predicted monthly values.
   Southern Australian Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Davis/Mawson):
      Depressed by 30% 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
17 Sep   100    Near predicted monthly values
18 Sep   100    Near predicted monthly values
19 Sep   100    Near predicted monthly values

COMMENT: ASWFC HF Communications Warning 84 was issued on 15 
September and is current for 15-17 Sep. Maximum usable frequencies 
(MUFs) on UT day 16-Sep were mostly near predicted values. Spread-F 
was observed in Perth and Hobart during local night hours. MUFs 
are expected to be near predicted values on 17-19 Sep.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 15 Sep
       Daily Proton Fluence >1 MeV:   N/A
       Daily Proton Fluence >10 MeV:  N/A
       Daily Electron Fluence >2 MeV: N/A
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: N/A

DSCOVR Satellite Solar Wind Day Averaged Data for 15 Sep
Speed: 668 km/sec  Density:    2.6 p/cc  Temp:   375000 K  Bz:   1 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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