[Ips-dsgr] ASWFC Daily Report - 29 May 26 issued 2330 UT on 29 May 2026 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Sat May 30 09:30:51 AEST 2026


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/29 MAY 2026
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 29 MAY AND FORECAST FOR 30 MAY - 01 JUNE
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 29 May:  R1
Flares    Max     Fadeout    Freq.  Sectors
  M1.1    0705UT  possible   lower  Mid East/Indian

Observed 10.7 cm flux/Equivalent Sunspot Number for 29 May: 148/102


1B. SOLAR FORECAST
             30 May             31 May             01 Jun
Activity     R0-R1              R0-R1              R0-R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   145/99             142/96             138/92

COMMENT: Solar flare activity on UT day 29-May was at the R1 
level due to an M1.1 flare at 29/0704UT. There are currently 
eight numbered sunspot regions visible on the solar disk. Newly 
rotated on Active Region (AR) 4455 (N14E46, beta) was responsible 
for the only R1 level flare event of the UT day. This region 
showed some spot decay. AR 4446 (S13W07, beta-gamma) showed spot 
development and 4452 (N09W44, beta-gamma) showed spot movement. 
These two regions are the most magnetically complex sunspot regions 
on the solar disk currently. All other sunspot regions are either 
stable or in decay. Solar flare activity is expected to be at 
R0-R1 levels over 30-May to 01-Jun. S0 solar radiation storm 
conditions were observed on UT day 29-May. S0 solar radiation 
storm conditions are expected over 30-May to 01-Jun. No Earth-directed 
coronal mass ejections (CMEs) have been observed. A west directed 
CME is visible from 29/0012UT in SOHO and STEREO-A imagery. This 
CME is considered a far side event and not geoeffective. The 
solar wind speed declined slightly on UT day 29-May, mostly ranging 
between 370 to 460 km/s and is currently near 420 km/s. The peak 
total interplanetary magnetic field strength (IMF, Bt) was 9 
nT and the north-south IMF component (Bz) range was -8 to +5 
nT. The solar wind speed is expected to remain at current levels 
over 30-May to 01-Jun, with a chance of an increase on 01-Jun 
due to a small equatorial coronal hole rotating towards a geoeffective 
position.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 29 May: G0

Estimated Indices 29 May : A   K           
   Australian Region       8   22123322
      Cocos Island         6   22122222
      Darwin               7   22122322
      Townsville          11   -3223332
      Learmonth           12   32223333
      Alice Springs       10   22223332
      Gingin              13   32223433
      Canberra             8   22113322
      Kennaook Cape Grim   8   22123322
      Hobart               8   22123322    

Estimated Antarctic Regional K Indices 29 May :
      Macquarie Island    16   22235431
      Casey               14   33224333
      Mawson              38   24424475

Observed Regional daily pc3 Indices 29 May : 
      Darwin               0   (Quiet)
      Townsville          11   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               6   (Quiet)
      Canberra            13   (Quiet)
      Hobart              18   (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 29 May : A 
           Fredericksburg        10
           Planetary             13                         

Observed AFr/Ap Indices 28 May :  A   K
           Fredericksburg        13
           Planetary             13   2233 3433     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
30 May    10    G0
31 May     8    G0
01 Jun     8    G0

COMMENT: G0 geomagnetic conditions were observed in the Australian 
and planetary regions on UT day 29-May. Mostly G1 geomagnetic 
conditions were observed in the Antarctic region, with an isolated 
period of G3 observed at Mawson. G0 planetary geomagnetic conditions 
are expected over 30-May to 01-Jun.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
30 May      Normal         Normal         Normal-fair
31 May      Normal         Normal         Normal-fair
01 Jun      Normal         Normal         Normal-fair

COMMENT: Global ionospheric conditions were mostly normal during 
UT day 29-May, with some degradations at high latitudes in the 
northern hemisphere. Ionospheric conditions are expected to be 
mostly normal over 30-May to 01-Jun, with some degradations expected 
at high latitudes over the forecast period.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
29 May    97

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.
      Depressed by 15% during local night.
   Northern Australian Region:
      Enhanced by 20% during local day.
      Near predicted monthly values during local night.
   Southern Australian Region:
      Enhanced by 15% 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
Apr      74
May      71
Jun      68

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
30 May    90    Near to 15% above predicted monthly values
31 May    90    Near to 15% above predicted monthly values
01 Jun    90    Near to 15% above predicted monthly values

COMMENT: Maximum Usable Frequencies (MUFs) on 29-May in the Australian 
region were enhanced by 20% in the northern Australian region 
during local day and near predicted monthly values during local 
night. MUFs in the southern Australian region were enhanced by 
15% throughout the day. Spread-F was observed at Hobart during 
local night hours. Ionospheric scintillation was observed at 
Weipa over the interval 29/1658-1713UT. MUFs are expected to 
be near predicted monthly values to 15% enhanced over 30-May 
to 01-Jun.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 28 May
       Daily Proton Fluence >1 MeV:   5.7E+05
       Daily Proton Fluence >10 MeV:  2.4E+04
       Daily Electron Fluence >2 MeV: 1.70E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 3%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B7.7

DSCOVR Satellite Solar Wind Day Averaged Data for 28 May
Speed: 401 km/sec  Density:    3.8 p/cc  Temp:   100000 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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