[Ips-dsgr] ASWFC Daily Report - 25 February 25 issued 2330 UT on 25 Feb 2025 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Wed Feb 26 10:30:51 AEDT 2025


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/25 FEBRUARY 2025
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 25 FEBRUARY AND FORECAST FOR 26 FEBRUARY - 28 FEBRUARY
STATUS INDICATORS SOL:** YELLOW **   MAG:** YELLOW **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 25 Feb:  R1

Flares    Max     Fadeout    Freq.  Sectors
  M3.9 24/2302UT  possible   lower  West Pacific
  M1.3    0247UT  possible   lower  E. Asia/Aust.
  M3.6    1159UT  possible   lower  European

Observed 10.7 cm flux/Equivalent Sunspot Number for 25 Feb: 190/143


1B. SOLAR FORECAST
             26 Feb             27 Feb             28 Feb
Activity     R1, chance R2      R1, chance R2      R1, chance R2
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   190/143            190/143            185/138

COMMENT: Solar activity on UT day 25-Feb was at the R1 level 
due to two M-class flares, the largest of which was an M3.6 flare 
at 25/1159UT produced by AR3998 (S12W51, beta). There are currently 
seven numbered sunspot regions visible on the solar disk. AR3998 
is the largest region on the disk and has decayed over the UT 
day. AR4000 (N18W44, beta) has also decayed. AR3996 (S15W65, 
beta) has shown mild growth in its trailer spot. AR4006 (N17E34, 
beta) has exhibited mild growth in its intermediate spots. AR4007 
(S12E34, beta) has shown spot growth. Newly numbered region AR4008 
(N07E68, alpha) recently rotated over the eastern limb and is 
stable. All other sunspot regions are either stable or in decay. 
Solar activity is expected to be at the R1 level over 26-28 Feb, 
with a chance of R2. S1 solar radiation storm conditions were 
observed on UT day 25-Feb, which declined to S0 in the second 
half of the UT day. S0 solar proton conditions are expected over 
26-28 Feb, with a chance of S1. A filament eruption was observed, 
visible in H-alpha imagery from 25/1133UT immediately prior to 
the M3.6 flare from AR3998. A subsequent southwest-directed CME 
was observed, visible in STEREO-A coronagraph imagery from 25/1238UT. 
Preliminary modelling suggests this CME does not have an Earth-directed 
component, however further modelling will be completed when additional 
coronagraph imagery becomes available. No other Earth-directed 
CMEs have been observed. The solar wind speed on UT day 25-Feb 
decreased, ranging from 330 to 430 km/s and is currently near 
330 km/s. The peak total interplanetary field strength (IMF, 
Bt) was 16 nT and the north-south IMF component (Bz) range was 
+13 to -11 nT. A sustained period of southward IMF conditions 
was observed over the interval 25/1840-2153UT. Two coronal holes 
are currently crossing the central meridian and are expected 
to influence the solar wind speed on 28-Feb. The solar wind speed 
is expected to remain near background levels over 26-27 Feb, 
then increase on 28-Feb due to coronal hole high speed wind stream 
effects.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 25 Feb: G0

Estimated Indices 25 Feb : A   K           
   Australian Region       7   22221123
      Cocos Island         6   22211132
      Darwin               6   22221122
      Townsville           8   22221133
      Learmonth            9   32222133
      Alice Springs        7   22221123
      Gingin               7   22211133
      Canberra             6   12221023
      Kennaook Cape Grim   6   12221123
      Hobart               6   12212123    

Estimated Antarctic Regional K Indices 25 Feb :
      Macquarie Island     7   11113223
      Casey               20   44532233
      Mawson              16   33522224

Observed Regional daily pc3 Indices 25 Feb : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin              18   (Quiet)
      Canberra            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 25 Feb : A 
           Fredericksburg         7
           Planetary              7                         

Observed AFr/Ap Indices 24 Feb :  A   K
           Fredericksburg        10
           Planetary             12   3012 2252     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
26 Feb     8    G0
27 Feb    10    G0
28 Feb    20    G0-G1

COMMENT: G0 geomagnetic conditions were observed in the Australian 
region on UT day 25-Feb. Mostly G0 geomagnetic conditions were 
observed in the Antarctic region, with an isolated period of 
G1 observed at Casey. G0 geomagnetic conditions are expected 
over 26-27 Feb. G0-G1 geomagnetic conditions are expected on 
28-Feb due to coronal hole high speed wind stream effects.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
25 Feb      Normal         Normal         Normal         

PCA Event : 10MeV Proton/PCA Event Began at 0010UT 25/02, Ended at 0830UT 25/02

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
26 Feb      Normal         Normal         Normal-fair
27 Feb      Normal         Normal         Normal-fair
28 Feb      Normal         Normal-fair    Fair

COMMENT: HF radio propagation conditions were mostly normal on 
UT day 25-Feb. Mostly normal HF conditions are expected over 
26-27 Feb, tending to fair at middle and high latitudes on 28-Feb 
due to anticipated geomagnetic activity. Shortwave fadeouts are 
possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
25 Feb   116

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values during local day.
      Enhanced by 15% during local night.
      Enhanced by 25% after local dawn.
   Niue Island Region:
      Near predicted monthly values.
   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
Jan      124
Feb      118
Mar      115

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
26 Feb   120    Near predicted monthly values
27 Feb   120    Near predicted monthly values
28 Feb   120    Near predicted monthly values

COMMENT: ASWFC SWF HF Communications Warning 25 was issued on 
25 February and is current for 25-27 Feb. Maximum usable frequencies 
(MUFs) on UT day 25-Feb in the Australian region were near predicted 
monthly values. Mild spread F was observed at Hobart. MUFs are 
expected to be near predicted monthly values over 26-28 Feb. 
Shortwave fadeouts are possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 24 Feb
       Daily Proton Fluence >1 MeV:   2.7E+06
       Daily Proton Fluence >10 MeV:  6.3E+04
       Daily Electron Fluence >2 MeV: 1.60E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C2.4

DSCOVR Satellite Solar Wind Day Averaged Data for 24 Feb
Speed: 359 km/sec  Density:    7.3 p/cc  Temp:    61400 K  Bz:   4 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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