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

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Mon Mar 30 10:30:43 AEDT 2026


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/29 MARCH 2026
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 29 MARCH AND FORECAST FOR 30 MARCH - 01 APRIL
STATUS INDICATORS SOL:** YELLOW **   MAG:** YELLOW **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 29 Mar:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 29 Mar: 158/112


1B. SOLAR FORECAST
             30 Mar             31 Mar             01 Apr
Activity     R0,chance R1       R0,chance R1       R0,chance R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   155/109            152/107            155/109

COMMENT: Solar activity on UT day 29-Mar was R0, with no significant 
flares observed. Solar region AR4401 (N24W23, beta) continues 
to show decay in its trailer spots and shows umbral convergence in 
its leader spot. Region AR4405 (S26E42, beta) may be in initial 
decay with the umbra within its leader spot appearing to separate 
and the surrounding penumbra reducing in area. Other solar regions 
are smaller in size. There are currently nine solar regions on 
the visible solar disk. All other sunspot regions are either 
stable or in decay. Solar activity is expected to be R0, chance 
R1 over 30-Mar to 01-Apr. No Earth directed CMEs have been observed. 
S0 solar radiation storm conditions were observed on UT day 29-Mar. 
S0 solar radiation storm conditions are expected over 30-Mar 
to 01-Apr. An isolated coronal hole is visible in the northwest 
solar quadrant and another is visible in the southeast solar 
quadrant. The solar wind speed on UT day 29-Mar was initially 
light then increased to moderate as the Earth entered the solar 
wind stream from the coronal hole in the northwest solar quadrant. 
The solar wind ranged from 335 to 470 km/s and is currently at 
440 km/s. The peak total interplanetary field strength (IMF, 
Bt) was 13 nT and the north-south IMF component range (Bz) was 
+11 to -7 nT. The IMF Bz component was mildly southward during 
the interval 29/0000-0800UT. The solar wind speed is expected 
to be moderate to strong during the interval 30-Mar to 31-Mar. 
The coronal hole in the southeast solar quadrant is beginning 
to approach the solar central meridian and 27 day recurrence 
patterns suggest the Earth will enter the wind stream from this 
hole on 03-Apr. The flux of electrons with an energy of greater 
than 2 MeV at geosynchronous orbit as measured by the US GOES 
satellite has been recently enhanced though may be now reducing, 
and is statistically associated with the increased risk of 
geosynchronous satellite operational anomalies.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 29 Mar: G0

Estimated Indices 29 Mar : A   K           
   Australian Region       8   22232311
      Cocos Island         4   21112210
      Darwin              10   22233322
      Townsville          10   23233321
      Learmonth            -   --------
      Alice Springs        8   12233311
      Gingin               7   22222321
      Canberra             7   12232311
      Kennaook Cape Grim   9   22242311
      Hobart               9   22242311    

Estimated Antarctic Regional K Indices 29 Mar :
      Macquarie Island    23   13364510
      Casey               10   33422211
      Mawson              18   44523311

Observed Regional daily pc3 Indices 29 Mar : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth           NA
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             4   (Quiet)
      Hobart              20   (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 Mar : A 
           Fredericksburg        13
           Planetary             18                         

Observed AFr/Ap Indices 28 Mar :  A   K
           Fredericksburg         8
           Planetary             11   3233 2213     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
30 Mar    19    G0-G1
31 Mar    15    G0, chance G1
01 Apr     8    G0

COMMENT: ASWFC Geomagnetic Warning 21 was issued on 27 March 
and is current for 29-31 Mar. G0 geomagnetic conditions were 
observed in the Australian region on UT day 29-Mar. G0-G1 geomagnetic 
conditions were observed in the Antarctic region. Periods of 
G1 conditions are possible over over 30-31 Mar due to a coronal 
hole wind stream.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
30 Mar      Normal         Fair-normal    Fair
31 Mar      Normal         Fair-normal    Fair
01 Apr      Normal         Normal         Normal-fair

COMMENT: HF radio propagation on UT day 29-Mar were fair to normal, 
with fair conditions at middle to high latitudes. HF conditions 
are expected to be mildly degraded during 30-31 Mar at middle 
to high latitudes, particularly during local night hours.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
29 Mar    84

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values during local day.
      Depressed by 20% during local night.
   Niue Island Region:
      Near predicted monthly values.
   Northern Australian Region:
      Mostly near predicted monthly values.
   Southern Australian Region:
      Near predicted monthly values during local day.
      Depressed by 15% during local night.
   Antarctic Region (Casey/Davis/Mawson):
      Depressed by 25% 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
30 Mar    95    Near predicted monthly values
31 Mar    70    Depressed 10 to 15%/near predicted monthly values
01 Apr    80    Near predicted monthly values

COMMENT: Maximum usable frequencies (MUFs) in the Australian 
region on UT day 29-Mar were generally near predicted values 
with 15% depressions observed during local night hours in the 
southern Australian region. Spread F was observed at Hobart and 
Perth during the local night. MUFs are expected to be near predicted 
monthly values on 30-Mar and 15% depressed to near predicted 
monthly values on 31-Mar due to expected mild geomagnetic activity 
associated with a coronal hole wind stream. Mildly degraded HF 
conditions may be experienced during local night hours during 
30-31 Mar.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 28 Mar
       Daily Proton Fluence >1 MeV:   8.7E+05
       Daily Proton Fluence >10 MeV:  1.6E+04
       Daily Electron Fluence >2 MeV: 5.00E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 7%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C1.0

DSCOVR Satellite Solar Wind Day Averaged Data for 28 Mar
Speed: 372 km/sec  Density:    0.4 p/cc  Temp:    36900 K  Bz:  -3 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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