[Ips-dsgr] ASWFC Daily Report - 18 August 26 issued 2330 UT on 18 Aug 2026 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Wed Aug 19 09:30:48 AEST 2026


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/18 AUGUST 2026
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 18 AUGUST AND FORECAST FOR 19 AUGUST - 21 AUGUST
STATUS INDICATORS SOL:** YELLOW **   MAG:** YELLOW **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 18 Aug:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 18 Aug: 125/78


1B. SOLAR FORECAST
             19 Aug             20 Aug             21 Aug
Activity     R0                 R0                 R0
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   125/78             125/78             120/72

COMMENT: Solar flare activity on UT day 18-Aug was at the R0 
level, with several minor C-class flares observed. There are 
currently five numbered active regions (ARs) visible on the solar 
disk. AR 4507 (N05W55, beta-gamma) is the largest and most magnetically 
complex region on the visible solar disk, however it has no history 
of flaring above the R0 level and has decayed over the UT day. 
All other ARs are either stable or in decay. Solar flare activity 
is expected to be at R0-R1 levels over 19-21 Aug, due to the 
size and magnetic complexity of region 4507. S0 solar radiation 
storm conditions were observed on UT day 18-Aug and are expected 
to remain there over 19-21 Aug. No Earth-directed coronal mass 
ejections (CMEs) have been observed. A pair of west directed 
CMEs are visible in SOHO imagery from 18/0948UT and 18/1412UT, 
although the 2nd CME is partially obscured by the earlier one. 
The first CME appears to be associated with an eruption over 
the western limb from 18/0858UT, visible in GOES SUVI imagery. 
The second CME appears to be associated with an eruption on the 
disk at around N20W80, visible from 18/1334UT in GOES SUVI and 
SDO imagery. Modelling suggests both CMEs will pass ahead of 
Earth. The solar wind speed increased over the UT day due to 
the early arrival of coronal hole high speed wind stream effects. 
The wind speed mostly ranged between 370 km/s and 605 km/s and 
is currently at around 560 km/s. The peak total interplanetary 
magnetic field strength (IMF, Bt) was 15 nT and the north-south 
IMF component (Bz) range was -11 to +12 nT. The solar wind speed 
is expected to remain elevated over 19-21 Aug due to ongoing 
high speed wind stream effects from a coronal hole in the southern 
hemisphere, combined with the expected arrival of a further high 
speed wind stream from a coronal hole in the northern hemisphere 
on 20-Aug.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 18 Aug: G1

Estimated Indices 18 Aug : A   K           
   Australian Region      14   33222153
      Cocos Island        10   22222143
      Darwin              13   33322143
      Townsville          13   24222243
      Learmonth           17   33322154
      Alice Springs       13   23222153
      Gingin              15   33211154
      Canberra            12   24222143
      Kennaook Cape Grim  21   34------
      Hobart              16   34211154    

Estimated Antarctic Regional K Indices 18 Aug :
      Macquarie Island    15   35310034
      Casey               16   33311154
      Mawson              26   44312165

Observed Regional daily pc3 Indices 18 Aug : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin              11   (Quiet)
      Canberra            20   (Quiet)
      Hobart              53   (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 18 Aug : A 
           Fredericksburg        18
           Planetary             27                         

Observed AFr/Ap Indices 17 Aug :  A   K
           Fredericksburg        19
           Planetary             11   2121 2344     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
19 Aug    18    G0-G1
20 Aug    16    G0-G1
21 Aug    12    G0, chance of G1

COMMENT: G1 geomagnetic conditions were observed at the planetary 
level and in the Australian region on UT day 18-Aug. Due to coronal 
hole high speed wind stream effects. Mostly G1 conditions were 
observed in the Antarctic region, with a period of G2 observed 
at Mawson. G0-G1 geomagnetic conditions are expected over 19-20 
Aug due to ongoing coronal hole high speed wind stream effects, 
combined with an anticipated further coronal hole enhancement 
on 20-Aug. G0 conditions, with a chance of G1 are expected on 
21-Aug.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
18 Aug      Normal-fair    Normal-fair    Normal-fair    

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
19 Aug      Normal         Normal-fair    Fair
20 Aug      Normal         Normal-fair    Fair
21 Aug      Normal         Normal         Normal-fair

COMMENT: HF radio propagation conditions on UT day 18-Aug were 
mostly normal in the southern hemisphere, with degradations observed 
in the northern hemisphere, particularly at high latitudes. HF 
radio propagation conditions are expected to be mostly normal 
to fair over 19-21 Aug. Due to recent and anticipated geomagnetic 
conditions. Propagations conditions are expected to gradually 
improve over the period.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
18 Aug    77

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

Monthly T index:
Month  T index
Jul      75
Aug      64
Sep      61

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
19 Aug    65    Near predicted monthly values
20 Aug    65    Near predicted monthly values
21 Aug    75    Near predicted monthly values

COMMENT: Maximum usable frequencies (MUFs) in the Australian 
region on UT day 18-Aug were near predicted monthly values. Spread 
F was observed at Hobart and Townsville during local night hours, 
sporadic E was also observed at Hobart during local night hours. 
MUFs are expected to be near predicted monthly values over 19-21 
Aug, with mild depressions possible in the southern Australian 
region over 19-20 Aug due to ongoing and forecast geomagnetic 
activity.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 17 Aug
       Daily Proton Fluence >1 MeV:   2.6E+05
       Daily Proton Fluence >10 MeV:  2.0E+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: B6.3

DSCOVR Satellite Solar Wind Day Averaged Data for 17 Aug
Speed: 336 km/sec  Density:    9.4 p/cc  Temp:   103000 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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