[Ips-dsgr] ASWFC Daily Report - 28 April 26 issued 2330 UT on 28 Apr 2026 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Wed Apr 29 09:30:23 AEST 2026


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/28 APRIL 2026
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 28 APRIL AND FORECAST FOR 29 APRIL - 01 MAY
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 28 Apr:  R1

Flares    Max     Fadeout    Freq.  Sectors
  M1.0    1223UT  possible   lower  European
  M1.5    1353UT  possible   lower  European
  M1.1    1407UT  possible   lower  South American/
                                    Atlantic

Observed 10.7 cm flux/Equivalent Sunspot Number for 28 Apr: 149/104


1B. SOLAR FORECAST
             29 Apr             30 Apr             01 May
Activity     R1, chance of R2   R1, chance of R2   R1, chance of R2
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   148/102            148/102            145/99

COMMENT: Solar flare activity reached the R1 level on UT day 
28-Apr, with an M1.0 flare at 28/1217UT, and a M1.5 flare at 
28/1349UT, both originating from Active Region (AR) 4420 (N16W44, 
beta-delta). This region is one of seven sunspot regions on the 
visible disk, and has shown some minor decay over the past UT 
day. Previously flare active region AR 4425 (N05E24, beta-gamma) 
has shown some growth and spot separation in the last 24 hours. 
AR 4428 (S23E14, beta) has also shown some growth over the same 
period. All other regions are either stable or in decay. Solar 
flare activity is forecast to be at the R1 level, with a chance 
of R2 over 29-Apr to 01-May, given the presence of large, magnetically 
complex sunspot regions on the Earth‑facing solar disk. S0 solar 
proton conditions were observed throughout UT day 28-Apr, with 
solar proton flux persisting at background levels. S0 solar proton 
conditions are forecast for 29-Apr to 01-May. No coronal mass 
ejections (CMEs) were observed over the past UT day. The solar 
wind speed declined towards background levels throughout UT day 
28-Apr, beginning the UT day at approximately 430 km/s, and declining 
to between 350 and 370 km/s. The interplanetary magnetic field 
strength (IMF, Bt) peaked at 5 nT during the UT day, and the 
north-south component (Bz) ranged between -2 and +4 nT over the 
UT day. The solar wind speed is expected to increase over 29-30 
Apr due to high speed wind streams from a small equatorial coronal 
hole. These conditions will then begin to ease on 01-May.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 28 Apr: G0

Estimated Indices 28 Apr : A   K           
   Australian Region       0   00100010
      Cocos Island         1   11000010
      Darwin               2   10100021
      Townsville           1   11100011
      Learmonth            1   10100010
      Alice Springs        0   00100010
      Gingin               0   00100010
      Canberra             0   00100010
      Kennaook Cape Grim   0   00100010
      Hobart               0   00100010    

Estimated Antarctic Regional K Indices 28 Apr :
      Macquarie Island     0   00000000
      Casey                2   22200000
      Mawson               1   11100000

Observed Regional daily pc3 Indices 28 Apr : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               4   (Quiet)
      Canberra            11   (Quiet)
      Hobart              11   (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 28 Apr : A 
           Fredericksburg         4
           Planetary              4                         

Observed AFr/Ap Indices 27 Apr :  A   K
           Fredericksburg         6
           Planetary              7   3211 22-1     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
29 Apr    12    G0, chance of G1
30 Apr    14    G0, chance of G1
01 May    10    G0

COMMENT: G0 geomagnetic conditions were recorded in the Australian 
region throughout UT day 28-Apr, with G0 conditions also recorded 
in the Antarctic region, and at the planetary level. G0 geomagnetic 
conditions, with a chance of G1 are forecast over 29-30 Apr due 
to anticipated high speed wind stream effects from an equatorial 
coronal hole, declining to G0 on 01-May as these effects begin 
to subside.

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

PCA Event : No event.

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

COMMENT: Global ionospheric conditions were mostly normal across 
UT day 28-Apr, with some degradations seen in the South American 
and South African regions. Mostly normal ionospheric conditions 
are forecast for 29-Apr, with normal to fair conditions forecast 
on 30-Apr and 01-May due to coronal hole high speed wind stream 
effects. Shortwave fadeouts are possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
28 Apr    75

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 during local day.
      Depressed by 20% 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
Mar      92
Apr      83
May      81

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
29 Apr    80    Near predicted monthly values
30 Apr    70    Near predicted monthly values
01 May    70    Near predicted monthly values

COMMENT: ASWFC SWF HF Communications Warning 43 was issued on 
27 April and is current for 27-29 Apr. Maximum Usable Frequencies 
(MUFs) in the Australian and Antarctic regions were near predicted 
monthly values across UT day 28-Apr, with depressions of around 
20% observed at Niue Island during local night hours. Spread-F 
was observed at Hobart, and sporadic E was observed in Canberra. 
Ionospheric scintillation was observed at Darwin between 28/1338-1510UT. 
MUFs are expected to remain near predicted values on 29-Apr, 
with some small depressions possible on 30-Apr and 01-May due 
to forecast geomagnetic activity. Shortwave fadeouts are possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 27 Apr
       Daily Proton Fluence >1 MeV:   2.0E+05
       Daily Proton Fluence >10 MeV:  1.8E+04
       Daily Electron Fluence >2 MeV: 1.40E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 3%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B7.4

DSCOVR Satellite Solar Wind Day Averaged Data for 27 Apr
Speed: 447 km/sec  Density:    3.8 p/cc  Temp:    85700 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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