[Ips-dsgr] ASWFC Daily Report - 30 April 26 issued 2330 UT on 30 Apr 2026 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Fri May 1 09:30:46 AEST 2026


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/30 APRIL 2026
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 30 APRIL AND FORECAST FOR 01 MAY - 03 MAY
STATUS INDICATORS SOL:** YELLOW **   MAG:** YELLOW **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 30 Apr:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 30 Apr: 143/97


1B. SOLAR FORECAST
             01 May             02 May             03 May
Activity     R0-R1              R0-R1              R0-R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   135/89             130/84             128/81

COMMENT: Solar flare activity on UT day 30-Apr was at the R0 
level, with only C-class flares observed. There are currently 
six numbered sunspot regions visible on the solar disk and two 
unnumbered regions. Active Region (AR) 4420 (N16W67, beta) has 
exhibited growth in its trailer spots over the UT day. This region 
is now approaching the western limb, limiting a definitive assessment 
of its magnetic classification. AR 4424 (N17W32, beta) has shown 
spot development in its intermediate spots, whilst its trailers 
have shown some decay. Region 4429 (S05E38, beta) has shown spot 
growth over the UT day. Two unnumbered regions are visible near 
N12W15 (beta) and S18E65 (beta). Both unnumbered regions have 
shown growth since appearing on the visible disk. All other sunspot 
regions are either stable or in decay. Solar flare activity is 
expected to be at R0-R1 levels over 01-03 May. S0 solar proton 
conditions were observed on UT day 30-Apr. S0 solar proton conditions 
are expected over 01-03 May. No Earth-directed coronal mass ejections 
(CMEs) have been observed. The solar wind speed on UT day 30-Apr 
increased, ranging from 350 to 505 km/s and is currently near 
470 km/s. The peak total interplanetary magnetic field strength 
(IMF, Bt) was 14 nT and the north-south IMF component (Bz) range 
was -12 to +11 nT. Periods of sustained southward IMF conditions 
were observed over the intervals 30/1028-1256UT and 30/1909-2134UT. 
The solar wind speed is expected to remain elevated on 01-May. 
A northern hemisphere coronal hole may influence the solar wind 
speed over 02-03 May, though its effects will likely be limited 
by its high latitudinal extent.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 30 Apr: G0

Estimated Indices 30 Apr : A   K           
   Australian Region       6   11112223
      Cocos Island         5   11112222
      Darwin               6   21112223
      Townsville           7   21122223
      Learmonth            4   21112---
      Alice Springs        6   11112223
      Gingin               8   21112224
      Canberra             6   11022223
      Kennaook Cape Grim   6   11122223
      Hobart               6   11122223    

Estimated Antarctic Regional K Indices 30 Apr :
      Macquarie Island    11   10034333
      Casey               11   33222233
      Mawson              23   33212365

Observed Regional daily pc3 Indices 30 Apr : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             0   (Quiet)
      Hobart               0   (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 30 Apr : A 
           Fredericksburg         8
           Planetary             10                         

Observed AFr/Ap Indices 29 Apr :  A   K
           Fredericksburg         6
           Planetary              4   0111 2122     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
01 May    18    G0-G1
02 May    12    G0
03 May    14    G0, chance of G1

COMMENT: G0 geomagnetic conditions were observed in the Australian 
and planetary regions on UT day 30-Apr. Mostly G0-G1 geomagnetic 
conditions were observed in the Antarctic region, with an isolated 
period of G2 observed at Mawson. G0-G1 planetary geomagnetic 
conditions are expected on 01-May due to the current elevated 
solar wind conditions. G0 geomagnetic conditions are expected 
over 02-03 May, with a chance of G1 on 03-May due to coronal 
hole high speed wind stream effects from a northern hemisphere 
coronal hole.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
30 Apr      Normal         Normal         Normal         

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
01 May      Normal         Normal-fair    Fair
02 May      Normal         Normal         Normal-fair
03 May      Normal         Normal         Normal-fair

COMMENT: Global ionospheric conditions were mostly normal across 
UT day 30-Apr, with some degradations observed in the southern 
hemisphere. Normal to fair ionospheric conditions are forecast 
for 01-03 May. Shortwave fadeouts are possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
30 Apr    77

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 15% 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
01 May    80    Near predicted monthly values
02 May    85    Near predicted monthly values
03 May    85    Near predicted monthly values

COMMENT: ASWFC SWF HF Communications Warning 44 was issued on 
30 April and is current for 30 Apr to 2 May. Maximum Usable Frequencies 
(MUFs) in the Australian region were near predicted monthly values 
on UT day 30-Apr. Spread F was observed at Hobart and Canberra 
during local night hours. MUFs are expected to be generally near 
predicted monthly values over 01-03 May, with mild depressions 
possible on 01-May. Shortwave fadeouts are possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 29 Apr
       Daily Proton Fluence >1 MeV:   2.8E+05
       Daily Proton Fluence >10 MeV:  1.7E+04
       Daily Electron Fluence >2 MeV: 1.90E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 3%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B8.8

DSCOVR Satellite Solar Wind Day Averaged Data for 29 Apr
Speed: 321 km/sec  Density:    3.8 p/cc  Temp:    22400 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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