[Ips-dsgr] ASWFC Daily Report - 24 March 26 issued 2330 UT on 24 Mar 2026 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Wed Mar 25 10:30:48 AEDT 2026


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/24 MARCH 2026
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 24 MARCH AND FORECAST FOR 25 MARCH - 27 MARCH
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 24 Mar:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 24 Mar: 128/81


1B. SOLAR FORECAST
             25 Mar             26 Mar             27 Mar
Activity     R0-R1              R0-R1              R0-R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   128/81             130/84             135/89

COMMENT: Solar flare activity on UT day 24-Mar was R0 with no 
significant flare activity from the on disk solar regions. A 
C7.2 flare was observed at 24/1754UT on the northeast solar limb 
at solar latitude N12, with the presumed leader spot of a new 
region just becoming visible. Recent region of interest AR4400 
(S10W49, beta) is now in rapid decay. Solar region AR4401 (N24E38, 
beta-gamma) continues to show development in its trailer spots 
and produced a C2.3 flare at 24/2156UT. There are currently seven 
numbered sunspots on the solar disk and one new unnumbered region 
is currently rotating onto the disk. All other sunspot regions 
are either stable or in decay. Solar activity is expected to 
be R0-R1 over 25-27 Mar. No Earth directed CMEs were observed 
on 24-Mar. A non-Earth directed northeast CME was observed from 
24/2024UT associated with flare activity from the new sunspot 
region that is currently rotating onto the solar disk. S0 solar 
radiation storm conditions were observed on UT day 24-Mar. S0 
solar radiation storm conditions are expected over 25-27 Mar. 
A small isolated coronal hole is visible in the northeast solar 
quadrant and is approaching the solar central meridian. The solar 
wind speed on UT day 24-Mar was strong with a declining trend 
as the influence of a high speed wind stream from a large coronal 
hole now located in the northwest solar quadrant slowly reduces. 
The solar wind speed ranged from 535 to 637 km/s and is currently 
at 535 km/s. The interplanetary magnetic field strength (IMF, 
Bt) was 5 nT and the north-south IMF component range (Bz) was 
+3 to -4 nT. The IMF is currently small in magnitude. The solar 
wind speed is expected to continue to slowly decline. The possible 
weak glancing blow from a recent southeast directed filament 
eruption/CME has failed to eventuate. The flux of electrons of 
energy greater than 2MeV at geosynchronous orbit altitude is 
currently high, which is associated with an increased risk of 
satellite operational anomalies.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 24 Mar: G0

Estimated Indices 24 Mar : A   K           
   Australian Region      12   23343222
      Cocos Island         6   22222221
      Darwin               -   --------
      Townsville          12   23343222
      Learmonth           13   33243232
      Alice Springs       10   23233222
      Gingin              14   33243332
      Canberra            11   22343122
      Kennaook Cape Grim  13   23343232
      Hobart              12   23343222    

Estimated Antarctic Regional K Indices 24 Mar :
      Macquarie Island    26   33465321
      Casey               19   44443232
      Mawson              41   44443665

Observed Regional daily pc3 Indices 24 Mar : 
      Darwin              NA
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             2   (Quiet)
      Hobart              29   (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 24 Mar : A 
           Fredericksburg        12
           Planetary             17                         

Observed AFr/Ap Indices 23 Mar :  A   K
           Fredericksburg        15
           Planetary             28   5423 554-     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
25 Mar    14    G0, slight chance G1
26 Mar    11    G0
27 Mar     8    G0

COMMENT: ASWFC Geomagnetic Warning 20 was issued on 24 March 
and is current for 24-26 Mar. G0 geomagnetic conditions were 
observed in the Australian region on UT day 24-Mar. G0-G2 geomagnetic 
conditions were observed in the Antarctic region. G0 conditions 
are expected for 25-27 Mar, with a slight chance for isolated 
G1 conditions on 25-Mar.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
24 Mar      Normal         Fair-normal    Poor-fair      

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
25 Mar      Normal         Fair-normal    Fair
26 Mar      Normal         Normal         Normal-fair
27 Mar      Normal         Normal         Normal-fair

COMMENT: HF radio propagation conditions on UT day 24-Mar were 
poor to fair, with poor conditions at times at high latitudes. 
A brief period of increased absorption was observed at Casey, 
Davis and Mawson Antarctic riometers at 23/1800UT. HF radio propagation 
conditions are expected to fair to normal at middle latitudes 
and fair at high latitudes on 25-Mar with a slowly improving 
trend over 26-27 Mar.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
24 Mar    52

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values during local day.
      Depressed by 35% during local night.
   Niue Island Region:
      No data.
   Northern Australian Region:
      Near predicted monthly values during local day.
      Depressed by 20% during local night.
   Southern Australian Region:
      Depressed by 25% during local day.
      Depressed by 15% during local night.
   Antarctic Region (Casey/Davis/Mawson):
      Depressed by 20% over the UT day.

Monthly T index:
Month  T index
Feb      98
Mar      87
Apr      85

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
25 Mar    70    Depressed 10 to 20%/near predicted monthly values
26 Mar    90    Near predicted monthly values
27 Mar    90    Near predicted monthly values

COMMENT: Maximum usable frequencies in the southern Australian 
region on UT day 24-Mar were depressed 15-25%. In the northern 
Australian region MUFs were 20% depressed during the local night. 
Spread F was observed during the local night hours at Hobart, 
Canberra, Brisbane and Perth. Australian regional MUFs are expected 
to be mildly depressed by 10-20% to near predicted monthly values 
on 25-Mar and near predicted monthly values over 26-27 Mar.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 23 Mar
       Daily Proton Fluence >1 MeV:   5.5E+06
       Daily Proton Fluence >10 MeV:  2.7E+04
       Daily Electron Fluence >2 MeV: 1.50E+08   (moderate fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability:13%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B6.8

DSCOVR Satellite Solar Wind Day Averaged Data for 23 Mar
Speed: 661 km/sec  Density:    1.5 p/cc  Temp:   152000 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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