[Ips-dsgr] ASWFC Daily Report - 25 May 25 issued 2331 UT on 25 May 2025 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Mon May 26 09:31:04 AEST 2025


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/25 MAY 2025
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 25 MAY AND FORECAST FOR 26 MAY - 28 MAY
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: ** YELLOW **
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 25 May:  R3

Flares    Max     Fadeout    Freq.  Sectors
  X1.1    0152UT  probable   all    West Pacific
  M1.7    0635UT  possible   lower  Mid East/Indian
  M3.4    1018UT  possible   lower  European
  M8.9    1630UT  probable   lower  South American/
                                    Atlantic

Observed 10.7 cm flux/Equivalent Sunspot Number for 25 May: 133/87


1B. SOLAR FORECAST
             26 May             27 May             28 May
Activity     R1-R2              R1-R2              R1-R2
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   135/89             130/84             125/78

COMMENT: Solar activity on UT day 25-May was at the R3 level 
due to an X1.1 flare at 25/0152UT produced by AR4098 (S04W48, 
beta). This region also produced an M8.9 (R2) flare at 25/1630UT 
and two additional flares at the R1 level. There are currently 
seven numbered sunspot regions visible on the solar disk and 
one unnumbered region. AR4098 is the most flare active region 
on the disk and has exhibited spot growth over the UT day. The 
region appears to have lost its delta spot and will remain on 
the visible disk until 28-May. AR4099 (S13E70, beta) has shown 
spot growth. An unnumbered region recently rotated over the eastern 
limb near N08E80 (beta). This region is likely the return of 
previous region AR4079 and has shown some spot growth. All other 
sunspot regions are either stable or in decay. Solar activity 
is expected to be at R1-R2 levels over 26-28 May. No Earth-directed 
CMEs have been observed. A narrow west-directed CME was observed, 
visible in LASCO C2 coronagraph imagery from 25/0236UT. This 
CME is likely associated with the aforementioned X1.1 flare from 
AR4098. This CME is not considered geoeffective. The solar wind 
speed on UT day 25-May declined to background levels, ranging 
from 330 to 460 km/s and is currently near 375 km/s. The peak 
total interplanetary magnetic field strength (IMF, Bt) was 11 
nT and the north-south IMF component (Bz) range was -6 to +8 
nT. A small equatorial coronal hole is currently crossing the 
central meridian and may influence the solar wind speed on 28-May. 
The solar wind speed is expected to remain near background levels 
over 26-27 May, then increase on 28-May due to coronal hole high 
speed wind stream effects.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 25 May: G0

Estimated Indices 25 May : A   K           
   Australian Region       3   22211001
      Cocos Island         2   11211000
      Darwin               4   22211111
      Townsville           4   22211111
      Learmonth            6   32311101
      Alice Springs        3   12211001
      Gingin               3   22211001
      Canberra             2   12201000
      Kennaook Cape Grim   3   12211001
      Hobart               3   12211001    

Estimated Antarctic Regional K Indices 25 May :
      Macquarie Island     1   11011000
      Casey                6   23311011
      Mawson              11   34322222

Observed Regional daily pc3 Indices 25 May : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin              21   (Quiet to unsettled)
      Canberra            25   (Quiet to unsettled)
      Hobart              26   (Quiet to 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 25 May : A 
           Fredericksburg         7
           Planetary              8                         

Observed AFr/Ap Indices 24 May :  A   K
           Fredericksburg         6
           Planetary              5       


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
26 May     6    G0
27 May     6    G0
28 May    12    G0, chance of G1

COMMENT: G0 geomagnetic conditions were observed in the Australian 
and Antarctic regions on UT day 25-May. G0 geomagnetic conditions 
are expected over 26-28 May, with a chance of G1 on 28-May due 
to coronal hole effects from a recurrent coronal hole feature.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
26 May      Normal         Normal         Normal
27 May      Normal         Normal         Normal
28 May      Normal         Normal         Normal-fair

COMMENT: HF radio propagation conditions on UT day 25-May were 
normal to fair. HF radio propagation conditions are expected 
to be mostly normal over 26-28 May. Shortwave fadeouts are probable.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
25 May    79

Observed Australian Regional MUFs
   Cocos Island Region:
      Depressed by 15% during local day.
      Depressed by 35% during local night.
   Northern Australian Region:
      Depressed by 15% during local day.
      Depressed by 35% during local night.
   Southern Australian Region:
      Near predicted monthly values during local day.
      Depressed 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      123
May      113
Jun      111

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
26 May    75    15 to 20% below predicted monthly values
27 May    75    15 to 20% below predicted monthly values
28 May    75    15 to 20% below predicted monthly values

COMMENT: ASWFC SWF HF Communications Warning 52 was issued on 
25 May and is current for 25-27 May. Maximum usable frequencies 
(MUFs) in the Australian region on UT day 25-May were near predicted 
monthly values to 15-35% depressed. Spread F was observed at 
Hobart and Brisbane during local night hours. MUFs are expected 
to be 15-20% depressed over 26-28 May. Shortwave fadeouts are 
probable.

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5. SPACE ENVIRONMENT SUMMARY

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

DSCOVR Satellite Solar Wind Day Averaged Data for 24 May
Speed: 403 km/sec  Density:    2.9 p/cc  Temp:    54200 K  Bz:   0 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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