[Ips-dsgr] ASWFC Daily Report - 11 March 25 issued 2330 UT on 11 Mar 2025 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Wed Mar 12 10:30:55 AEDT 2025


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/11 MARCH 2025
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 11 MARCH AND FORECAST FOR 12 MARCH - 14 MARCH
STATUS INDICATORS SOL:** YELLOW **   MAG:** YELLOW **     ION: ** YELLOW **
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 11 Mar:  R1

Flares    Max     Fadeout    Freq.  Sectors
  M1.1    1304UT  possible   lower  European

Observed 10.7 cm flux/Equivalent Sunspot Number for 11 Mar: 161/115


1B. SOLAR FORECAST
             12 Mar             13 Mar             14 Mar
Activity     Low to moderate    Low to moderate    Moderate to high
Fadeouts     Possible           Possible           Probable
10.7cm/SSN   165/119            165/119            170/124

COMMENT: Solar activity on UT day 11-Mar was R1, with an isolated 
M1.1 solar flare from AR4024 (N07W48, beta). There are a total 
of eight numbered sunspots. AR4019 (N07E21, beta), AR4021 (S06E63, 
beta-gamma) and AR4022 (N08E50, beta) have all grown i the past 
day, although their trailing spots are quite dispersed around 
the leader. Solar activity is expected to be R0-R1 over 12-14 
Mar. 

No Earth directed CMEs were observed on UT day 11-Mar. S0 
solar radiation storm conditions were observed on UT day 11-Mar.
 
The 10 MeV protons began a slight increase from 1140 UT, likely 
from a farside event, however this is not expected to reach the 
S1 threshold. S0 solar radiation storm conditions are expected 
over 12-14 Mar. 

The solar wind environment on UT day 11-Mar was 
mostly undisturbed. The solar wind speed ranged from 530 trending 
to near 400 km/s. The peak total interplanetary field strength 
(IMF, Bt) was 8 nT and the north-south IMF component range (Bz) 
was +5 to -6 nT. The solar wind speed may increase over 12-14 
Mar due to a coronal hole.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 11 Mar: G0

Estimated Indices 11 Mar : A   K           
   Australian Region       5   11222112
      Cocos Island         3   10112112
      Darwin               5   11222112
      Townsville           6   21232112
      Learmonth            6   21222212
      Alice Springs        5   11222112
      Gingin               6   21222212
      Canberra             6   11223112
      Kennaook Cape Grim   8   12233212
      Hobart               7   12223212    

Estimated Antarctic Regional K Indices 11 Mar :
      Macquarie Island    13   01335321
      Casey               17   35433222
      Mawson              19   34533233

Observed Regional daily pc3 Indices 11 Mar : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               2   (Quiet)
      Canberra             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 11 Mar : A 
           Fredericksburg         9
           Planetary             13                         

Observed AFr/Ap Indices 10 Mar :  A   K
           Fredericksburg         8
           Planetary              9   3123 3223     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
12 Mar    16    G0, chance G1
13 Mar    16    G0-G1
14 Mar    14    G0-G1

COMMENT: G0 geomagnetic conditions were observed in the Australian 
region on UT day 11-Mar. G0-G1 geomagnetic conditions were observed 
in the Antarctic region. G0-G1 geomagnetic conditions are likely 
over 12-14 Mar due to coronal hole activity.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
12 Mar      Normal         Normal-fair    Normal-fair
13 Mar      Normal         Normal-fair    Fair
14 Mar      Normal-fair    Normal-fair    Fair

COMMENT: HF radio propagation conditions were generally normal 
on UT day 11-Mar with some degradation in the southern hemisphere 
in the first half of the UT day. HF radio propagation conditions 
are expected to be normal to mildly degraded over 12-14 Mar due 
to coronal hole activity. Degraded conditions are possible during 
local night hours. Brief shortwave fadeouts are possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
11 Mar   104

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

Monthly T index:
Month  T index
Feb      127
Mar      117
Apr      114

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
12 Mar   110    Near predicted monthly values to 15% depressed
13 Mar   100    Near predicted monthly values to 20% depressed
14 Mar    95    Near predicted monthly values to 20% depressed

COMMENT: Maximum usable frequencies (MUFs) on UT day 11-Mar were 
near predicted monthly values to 15% depressed in the Australian 
region. Scintillation was observed at Weipa from 1140 UT to 11:59 
UT. MUFs are expected to be near predicted values to 20% depressed 
over 12-14 Mar due to coronal hole activity. Spread-F may be 
present at local night hours in high latitudes.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 10 Mar
       Daily Proton Fluence >1 MeV:   2.6E+05
       Daily Proton Fluence >10 MeV:  1.8E+04
       Daily Electron Fluence >2 MeV: 8.00E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 9%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B8.0

DSCOVR Satellite Solar Wind Day Averaged Data for 10 Mar
Speed: 543 km/sec  Density:    1.1 p/cc  Temp:   235000 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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