[Ips-dsgr] ASWFC Daily Report - 10 July 26 issued 2341 UT on 10 Jul 2026 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Sat Jul 11 09:41:33 AEST 2026


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/10 JULY 2026
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 10 JULY AND FORECAST FOR 11 JULY - 13 JULY
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 10 Jul:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 10 Jul: 107/57


1B. SOLAR FORECAST
             11 Jul             12 Jul             13 Jul
Activity     R0-R1              R0-R1              R0-R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   105/54             105/54             110/60

COMMENT: Solar flare activity on UT day 10-Jul was at the R0 
level, with a C6.0 flare peaking at 10/1459UT from Active Region 
(AR) 4485 (S09W58, beta), the largest recorded. This region is 
one of four on the visible disk, and has shown some mild growth 
over the past UT day. AR 4482 (S08W05, beta) is the largest on 
the disk, and has shown some decay over the same period. All 
other regions are either stable or in decay. Solar flare activity 
is forecast to remain at the R0-R1 level over 11-12 Jul, due 
to the flare activity of AR 4485. This will decrease to R0 on 
13-Jul as this region rotates off the front side of the solar 
disk. S0 solar radiation storm conditions were observed throughout 
UT day 10-Jul, with the proton flux consistent with background 
values. S0 solar radiation storm conditions are forecast for 
11-13 Jul. No new geoeffective coronal mass ejections (CMEs) 
were observed over the previous 24 hours. A low-velocity east-directed 
CME was observed in SOHO/LASCO from 10/1326UT following a filament 
eruption visible in GONG/Halpha imaging at N03E62 from 10/1257UT. 
A southwest-directed CME was also observed in SOHO/LASCO starting 
from 10/1524UT following the C6.0 flare. Both of these CMEs have 
been modelled to miss Earth. Further modelling of the CME activity 
from 09-Jul suggests a glancing impact from the CME visible in 
Stereo-A from 09/0753UT at 12/0800 +/-10 hours. The solar wind 
speed was elevated across UT day 10-Jul due to ongoing high speed 
wind stream effects from an equatorial coronal hole. The solar 
wind speed broadly ranged between 560-620 km/s over the UT day. 
The interplanetary magnetic field strength (IMF, Bt) peaked at 
12 nT, with the north-south component (Bz) ranging between -7 
and +7 nT over the UT day. Sporadic periods of southward Bz were 
also observed between 10/0505UT and 10/0758UT. The solar wind 
is expected to slowly decline over 11-12 Jul, before increasing 
late on 12-Jul and 13-Jul due to a glancing impact of a CME first 
observed on 09-Jul.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 10 Jul: G0

Estimated Indices 10 Jul : A   K           
   Australian Region       9   13333112
      Cocos Island         5   12322001
      Darwin               6   12323001
      Townsville          11   13433112
      Learmonth            8   22333102
      Alice Springs        7   13323002
      Gingin               8   12333112
      Canberra             9   03433011
      Kennaook Cape Grim  11   13433112
      Hobart              11   13433112    

Estimated Antarctic Regional K Indices 10 Jul :
      Macquarie Island    18   22455211
      Casey               10   23333212
      Mawson              29   35542226

Observed Regional daily pc3 Indices 10 Jul : 
      Darwin              NA
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin              40   (Quiet to unsettled)
      Canberra            30   (Quiet to unsettled)
      Hobart              46   (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 10 Jul : A 
           Fredericksburg        11
           Planetary             14                         

Observed AFr/Ap Indices 09 Jul :  A   K
           Fredericksburg        15
           Planetary             16    3124 2344    


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
11 Jul     8    G0
12 Jul    14    G0-G1
13 Jul    14    G0, chance of G1

COMMENT: Geomagnetic conditions in the Australian region were 
at the G0 level on UT day 10-Jul, with G0 conditions also reported 
at the planetary scale. G1 conditions were recorded in the Antarctic 
region. G0 geomagnetic conditions are forecast for 11-Jul. This 
will rise to G0-G1 on 12-Jul, and G0, with chance of G1 on 13-Jul, 
due to a glancing CME impact forecast to arrive on 12-Jul.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
10 Jul      Normal-fair    Fair-normal    Fair           

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
11 Jul      Normal-fair    Normal-fair    Fair-normal
12 Jul      Normal         Normal         Fair-normal
13 Jul      Normal-fair    Normal-fair    Fair-normal

COMMENT: Global high-frequency propagation conditions were fair 
to normal on UT day 10-Jul, with fair conditions reported at 
high latitudes. Degraded conditions were mostly observed across 
northern hemisphere sites, and improved throughout the UT day. 
Ionospheric conditions are forecast to continue to improve toward 
normal conditions over 11-12 Jul, with more degradations forecast 
on 13-Jul due to anticipated geomagnetic activity. Isolated shortwave 
fadeouts are possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
10 Jul    62

Observed Australian Regional MUFs
   Cocos Island Region:
      No data available during local day.
      No data available during local night.
   Niue Island Region:
      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 15% over the UT day.

Monthly T index:
Month  T index
Jun      81
Jul      66
Aug      63

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
11 Jul    60    Near predicted monthly values
12 Jul    60    Near predicted monthly values
13 Jul    55    Near predicted monthly values

COMMENT: Maximum Usable Frequencies (MUFs) in the Australian 
region were near predicted monthly values on UT day 10-Jul. Significant 
spread-F was observed in the southern Australian region, and 
also at Niue Island. Sporadic E was also observed at Darwin. 
MUFs are forecast to remain near predicted monthly values over 
11-12 Jul, with some mild depressions possible on 13-Jul due 
to forecast geomagnetic activity. Isolated shortwave fadeouts 
are possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 09 Jul
       Daily Proton Fluence >1 MeV:   2.66E+05
       Daily Proton Fluence >10 MeV:  1.76E+04
       Daily Electron Fluence >2 MeV: 2.58E+07   (normal fluence)
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B4.2

DSCOVR Satellite Solar Wind Day Averaged Data for 09 Jul
Speed: 438 km/sec  Density:    7.1 p/cc  Temp:   261000 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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