[Ips-dsgr] ASWFC Daily Report - 09 February 25 issued 2331 UT on 09 Feb 2025 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Mon Feb 10 10:31:18 AEDT 2025


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/09 FEBRUARY 2025
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 09 FEBRUARY AND FORECAST FOR 10 FEBRUARY - 12 FEBRUARY
STATUS INDICATORS SOL:** YELLOW **   MAG:** RED **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 09 Feb:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 09 Feb: 163/117


1B. SOLAR FORECAST
             10 Feb             11 Feb             12 Feb
Activity     R0-R1, chance R2   R0-R1              R0-R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   165/119            170/124            175/129

COMMENT: Solar activity on UT day 09-Feb was at the R0 level 
with multiple C-class flares observed. There are currently nine 
numbered active regions visible on the solar disk. AR3981 (N07W62, 
beta-gamma) remains the largest and most magnetically complex 
active region. This region is expected to rotate off the solar 
disk on 11-Feb and has shown spot decay over the UT day. AR3983 
(N06W03, beta) and AR3988 (S21W33, beta) both showed spot development 
on 09-Feb but remain magnetically simple. All other active regions 
are either stable or in decay. Solar activity is expected to 
be at R0-R1 levels, with a chance of R2 on 10-Feb and at R0-R1 
levels on 11-12 Feb as AR3981 rotates off the solar disk. S0 
solar proton conditions were observed on UT day 09-Feb. S0 solar 
proton conditions are expected over 10-12 Feb. No geoeffective 
CMEs were observed on 09-Feb. A disappearing filament was observed 
from 09/1216UT in H-Alpha, SDO and GOES SUVI imagery at around 
S25W14. Despite material appearing to lift off the disk no associated 
CME is visible in available coronagraph imagery. Two faint CMEs 
from 7 and 8-Feb have been analysed and are expected to produce 
glancing impacts with Earth at 11/1300UT and 12/1800UT +/- 12 
hours respectively. The solar wind speed on UT day 09-Feb increased 
due to the arrival of a high speed wind stream from an equatorial 
coronal hole. The solar wind speed mostly ranged between 320 
km/s and 600 km/s and is currently at around 545 km/s. The peak 
total interplanetary field strength (IMF, Bt) was 23 nT and the 
north-south IMF component (Bz) range was +16 to -17 nT. Bz has 
been mostly negative since 09/1300UT. The solar wind is expected 
to remain elevated over 10-12 Feb due to ongoing coronal hole 
high speed wind stream effects combined with anticipated glancing 
CME impacts.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 09 Feb: G1

Estimated Indices 09 Feb : A   K           
   Australian Region      20   23233445
      Cocos Island        15   22233344
      Darwin              17   23233335
      Townsville          20   23233445
      Learmonth           20   23233445
      Alice Springs       17   23233335
      Gingin              19   22233445
      Canberra            17   13223435
      Hobart              16   13333434    

Estimated Antarctic Regional K Indices 09 Feb :
      Macquarie Island    21   12223644
      Casey               37   45644345
      Mawson              34   35334546

Observed Regional daily pc3 Indices 09 Feb : 
      Darwin               0   (Quiet)
      Townsville           6   (Quiet)
      Learmonth            3   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin              20   (Quiet)
      Canberra            24   (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 09 Feb : A 
           Fredericksburg        12
           Planetary             16                         

Observed AFr/Ap Indices 08 Feb :  A   K
           Fredericksburg         9
           Planetary             10   0343 3211    


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
10 Feb    25    G1
11 Feb    15    G0, chance G1
12 Feb     8    G0

COMMENT: ASWFC Geomagnetic Warning 8 was issued on 9 February 
and is current for 10-11 Feb. G1 geomagnetic conditions were 
observed in the Australian region on UT day 09-Feb due to coronal 
hole high speed wind stream effects. G2 geomagnetic conditions 
were observed in the Antarctic region. G1 geomagnetic conditions 
are expected on 10-Feb due to ongoing coronal hole high speed 
wind stream effects. G0 conditions, with a chance of G1 are expected 
on 11-12 Feb due to ongoing coronal hole high speed wind stream 
effects combined with a pair of glancing CME impacts.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
09 Feb      Normal-fair    Normal-fair    Fair-poor      

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
10 Feb      Fair           Fair           Fair-poor
11 Feb      Normal-fair    Normal-fair    Fair-normal
12 Feb      Normal         Normal         Normal-fair

COMMENT: HF radio propagation conditions were mostly normal to 
fair on UT day 09-Feb, with degradations observed at high latitudes 
for most of the day and occasionally at mid latitudes. Degraded 
conditions were more common in the southern hemisphere. Mostly 
normal to fair conditions are expected over 10-11 Feb due to 
ongoing coronal hole high speed wind stream effects. Mostly normal 
conditions are expected on 12-Feb. Shortwave fadeouts are possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
09 Feb   111

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 20% 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 during local day.
      Enhanced by 25% during local night.
   Southern Australian Region:
      Depressed by 15% during local day.
      Near predicted monthly values during local night.
      Depressed by 25% after local dawn.
   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
10 Feb   110    Depressed 5 to 15%/near predicted monthly values
11 Feb   110    Depressed 5 to 15%/near predicted monthly values
12 Feb   140    Near to 15% above predicted monthly values

COMMENT: ASWFC SWF HF Communications Warning 19 was issued on 
8 February and is current for 8-10 Feb. ASWFC HF Communications 
Warning 20 was issued on 9 February and is current for 9-11 Feb. 
Maximum usable frequencies (MUFs) in the southern Australian 
region were mostly near predicted monthly values to depressed 
by up to 25%. Enhancements of up to 25% were observed during 
local night in the northern Australian region but MUFs were mostly 
near predicted monthly values. Periods of sporadic E were observed 
at Brisbane and Norfolk Island. MUFs are expected to be near 
predicted monthly values to 15% depressed over 10-11 Feb, due 
to ongoing coronal hole high speed wind stream effects. MUFs 
are expected to be near predicted monthly values to 15% enhanced 
on 12-Feb. Shortwave fadeouts are possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 08 Feb
       Daily Proton Fluence >1 MeV:   1.6E+05
       Daily Proton Fluence >10 MeV:  1.6E+04
       Daily Electron Fluence >2 MeV: 1.90E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C1.5

DSCOVR Satellite Solar Wind Day Averaged Data for 08 Feb
Speed: 348 km/sec  Density:    4.0 p/cc  Temp:    31700 K  Bz:   2 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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