[Ips-dsgr] ASWFC Daily Report - 14 April 24 issued 2330 UT on 14 Apr 2024 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Mon Apr 15 09:30:57 EST 2024


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/14 APRIL 2024
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 14 APRIL AND FORECAST FOR 15 APRIL - 17 APRIL
STATUS INDICATORS SOL:** YELLOW **   MAG:** YELLOW **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 14 Apr:  R0

Flares    Max     Fadeout    Freq.  Sectors
  M4.3    0232UT  possible   lower  E. Asia/Aust.

Observed 10.7 cm flux/Equivalent Sunspot Number for 14 Apr: 178/131


1B. SOLAR FORECAST
             15 Apr             16 Apr             17 Apr
Activity     R0-R1,chance R2    R0-R1,chance R2    R0-R1,chance R2
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   180/133            180/133            180/133

COMMENT: Solar activity on UT day 14-Apr was at the R1 level, 
due to an impulsive M4.3 flare from AR3637 (S10E52, beta) at 
14/0232UT. There are currently ten numbered sunspot regions on 
the solar disk. AR3634 (N25W32, beta) showed spot development 
and redistribution over the UT day, this region is the largest 
active region on the solar disk. AR3641 (N16E22, beta) showed 
signs of rapid growth and AR3635 (N19W07, beta) showed signs 
of growth in its trailer spots. All other numbered regions are 
either stable or in decay. Solar activity is expected to be at 
R0-R1, with a chance of R2 levels over 15-17 Apr. Solar radiation 
conditions were at the S0 level and are expected to remain at 
this level over 15-17 Apr. No significantly geoeffective CMEs 
were observed on 14-Apr. An east directed CME was observed associated 
with the M4.3 flare but is not considered geoeffective. A CME 
associated with a filament eruption on the western limb was also 
observed at around 14/0518UT. Modelling suggests a chance of 
a glancing impact at 17/2000UT (-/+ 12 hours), this impact is 
not expected to be significant. An eruption on the disk was observed 
from 14/1016UT at S20E40 in GOES SUVI and H-Alpha imagery, there 
is no associated CME visible in currently available coronagraph 
imagery. The solar wind speed increased slightly over UT day 
14-Apr. Solar wind speed ranged from 320 to 400 km/s. The wind 
speed is currently around 370 km/s. The peak total interplanetary 
field strength (IMF, Bt) was 6 nT and the north-south IMF component 
(Bz) range was +5 to -4 nT. A halo CME first observed on 12-Apr 
is expected to impact in the first half of 15-Apr, producing 
an increase in the solar wind speed. Solar wind speed is expected 
to be at background levels until this impact occurs and to begin 
to return to background levels over 16-17 Apr.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 14 Apr: G0

Estimated Indices 14 Apr : A   K           
   Australian Region       3   21211001
      Cocos Island         2   21210000
      Darwin               3   21210002
      Townsville           5   31211012
      Learmonth            2   21211000
      Alice Springs        2   11210002
      Gingin               2   21211000
      Canberra             2   11210002
      Kennaook Cape Grim   2   11211001
      Hobart               2   11211001    

Estimated Antarctic Regional K Indices 14 Apr :
      Macquarie Island     0   00101000
      Casey                5   22321001
      Mawson               9   32200134

Observed Regional daily pc3 Indices 14 Apr : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             8   (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 14 Apr : A 
           Fredericksburg         6
           Planetary              6                         

Observed AFr/Ap Indices 13 Apr :  A   K
           Fredericksburg         6
           Planetary              4   1200 2222     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
15 Apr    20    G0-G1
16 Apr     8    G0
17 Apr    10    G0

COMMENT: ASWFC Geomagnetic Warning 13 was issued on 14 April 
and is current for 14-15 Apr. G0 geomagnetic conditions were 
observed in the Australian and Antarctic regions on UT day 14-Apr. 
G0-G1 geomagnetic conditions are expected on 15-Apr due to an 
anticipated impact from a CME first observed on 12-Apr. G0 conditions 
are expected on 16-17 Apr.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
15 Apr      Normal         Normal-fair    Fair
16 Apr      Normal         Normal         Normal-fair
17 Apr      Normal         Normal         Normal-fair

COMMENT: HF radio propagation conditions on UT day 14-Apr were 
mostly normal. HF radio propagation conditions are expected to 
be mostly normal over 15-17 Apr, with the possibility of mildly 
degraded conditions at mid to high latitudes on 15-Apr due to 
anticipated geomagnetic activity. Shortwave fadeouts are possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
14 Apr   118

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 20% during local day.
      Enhanced by 25% during local night.
   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
Mar      120
Apr      114
May      115

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
15 Apr   115    Near predicted monthly values
16 Apr   120    Near predicted monthly values
17 Apr   120    Near predicted monthly values

COMMENT: ASWFC SWF HF Communications Warning 36 was issued on 
14 April and is current for 15-17 Apr. Maximum usable frequencies 
(MUFs) in the Australian region on UT day 14-Apr were near predicted 
monthly values. MUFs are expected to be near predicted monthly 
values over 15-17 Apr, with a chance of mild depressions in the 
southern Australian region on 15-Apr due to anticipated geomagnetic 
activity. Shortwave fadeouts are possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 13 Apr
       Daily Proton Fluence >1 MeV:   1.8E+05
       Daily Proton Fluence >10 MeV:  1.7E+04
       Daily Electron Fluence >2 MeV: 1.60E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 3%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C1.2

DSCOVR Satellite Solar Wind Day Averaged Data for 13 Apr
Speed: 396 km/sec  Density:    1.3 p/cc  Temp:    59400 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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