[Ips-dsgr] ASWFC Daily Report - 18 April 24 issued 2330 UT on 18 Apr 2024 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Fri Apr 19 09:30:55 EST 2024


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/18 APRIL 2024
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 18 APRIL AND FORECAST FOR 19 APRIL - 21 APRIL
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 18 Apr:  R1

Flares    Max     Fadeout    Freq.  Sectors
  M1.6 17/2208UT  possible   lower  East Pacific/
                                    North American
  M2.2    0248UT  possible   lower  E. Asia/Aust.
  M1.3    0739UT  possible   lower  Mid East/Indian
  M1.6    2001UT  possible   lower  East Pacific/
                                    North American

Observed 10.7 cm flux/Equivalent Sunspot Number for 18 Apr: 227/177


1B. SOLAR FORECAST
             19 Apr             20 Apr             21 Apr
Activity     R1, chance of R2   R1, chance of R2   R1, chance of R2
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   225/175            220/170            220/170

COMMENT: Solar activity on UT day 18-Apr was at the R1 level, 
due to an M2.2 flare at 18/0253UT, an M1.3 flare at 18/0809UT 
and an M1.6 flare which peaked at 18/2001UT and 18/2016UT. There 
are currently thirteen numbered sunspot regions on the solar 
disk and one unnumbered region. The collection of sunspot regions 
consisting of AR3643 (S12E23, beta), AR3645 (S09E10, beta-delta) 
and newly numbered AR3647 (S15E15, beta-delta) along with the 
nearby AR3638 (S16E07, beta) were responsible for all the M-class 
flares over the UT day and are the most significant regions on 
the solar disk. They all showed spot development on 18-Apr, with 
at least two delta spot candidates visible. AR3635 (N19W60, beta), 
AR3636 (S21W22, alpha) and AR3639 (N29E17, beta) also showed 
spot development but are magnetically simple regions with no 
history of flaring. All other numbered regions are either stable 
or in decay. An unnumbered region has developed on the solar 
disk at around N15W08 with beta magnetic characteristics. Solar 
activity is expected to be at the R1 level over 19-21 Apr, with 
a chance of R2. Primarily due to the combination of AR3643, AR3645 
and AR3647. Solar radiation conditions were at the S0 level on 
18-Apr and are expected to remain at this level over 19-21 Apr. 
No geoeffective CMEs were observed on 18-Apr. STEREO-A images 
were unavailable for CME modelling over 18-Apr, making CME analysis 
less certain today. A series of slow southeast directed CMEs 
were observed from 18/0336UT through to 18/1800UT in SOHO and 
STEREO-A imagery. These are likely due to eruptions associated 
with flares produced by the conglomerate of sunspot groups mentioned 
previously. These CMEs are not considered geoeffective. A west 
directed CME is visible in SOHO and STEREO-A imagery from 18/1800UT 
with associated faint coronal movement visible behind the western 
limb in GOES SUVI from 18/1528UT. This CME is not considered 
geoeffective. The solar wind speed was mostly in decline on UT 
day 18-Apr, with an increase observed from 18/2030UT onwards. 
The wind speed ranged from 300 to 440 km/s and is currently around 
350 km/s. The peak total interplanetary field strength (IMF, 
Bt) was 8 nT and the north-south IMF component (Bz) range was 
+8 to -4 nT. A sudden small increase in wind speed and IMF Bt 
at around 18/2030UT suggests the possible late arrival of the 
anticipated glancing impact from a CME first observed on 15-Apr. 
The solar wind speed is expected to remain around current levels 
until a possible increase on 20-Apr due to a possible glancing 
impact from a CME first observed on 16-Apr. The solar wind is 
expected to be slightly enhanced on 21-Apr due to high speed 
wind stream effects from a small coronal hole rotating towards 
a geoeffective location.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 18 Apr: Quiet

Estimated Indices 18 Apr : A   K           
   Australian Region       2   21100001
      Cocos Island         1   21100000
      Darwin               3   22100002
      Townsville           3   22100012
      Learmonth            2   21100001
      Alice Springs        2   21100002
      Gingin               2   21100001
      Canberra             1   11000001
      Kennaook Cape Grim   1   11100001
      Hobart               1   11100001    

Estimated Antarctic Regional K Indices 18 Apr :
      Macquarie Island     0   00000001
      Casey                4   32210001
      Mawson               2   22200000

Observed Regional daily pc3 Indices 18 Apr : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               0   (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 18 Apr : A 
           Fredericksburg         5
           Planetary              6                         

Observed AFr/Ap Indices 17 Apr :  A   K
           Fredericksburg         8
           Planetary              7   3102 2212     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
19 Apr     7    G0
20 Apr    15    G0, chance of G1
21 Apr    10    G0

COMMENT: G0 geomagnetic conditions were observed in the Australian 
and Antarctic regions on UT day 18-Apr. G0 geomagnetic conditions 
are expected over 19-21 Apr, with a chance of G1 on 20-Apr due 
to a possible glancing impact from a CME first observed on 16-Apr.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
18 Apr      Normal         Normal         Normal         

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
19 Apr      Normal         Normal         Normal
20 Apr      Normal         Normal         Normal-fair
21 Apr      Normal         Normal         Normal-fair

COMMENT: HF radio propagation conditions on UT day 18-Apr were 
mostly normal. HF radio propagation conditions are expected to 
be mostly normal over 19-21 Apr, with a chance of mild degradations 
at high latitudes over 20-21 Apr due to possible geomagnetic 
activity on 20-Apr. Shortwave fadeouts are probable.

-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
18 Apr   133

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values during local day.
      Enhanced by 85% during local night.
   Niue Island Region:
      Near predicted monthly values during local day.
      Enhanced by 35% during local night.
   Northern Australian Region:
      Near predicted monthly values during local day.
      Enhanced by 35% during local night.
   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
19 Apr   135    Near to 15% above predicted monthly values
20 Apr   135    Near to 15% above predicted monthly values
21 Apr   135    Near to 15% above predicted monthly values

COMMENT: ASWFC SWF HF Communications Warning 37 was issued on 
18 April and is current for 18-20 Apr. Maximum usable frequencies 
(MUFs) in the Australian region on UT day 18-Apr were near predicted 
monthly values, with enhanced conditions observed at Darwin during 
local night. Long periods of spread F were observed at Canberra 
during local night. MUFs are expected to be near predicted monthly 
values to 15% enhanced over 19-21 Apr, with a chance of mild 
depressions in the southern Australian region over 20-21 Apr 
due to possible geomagnetic activity on 20-Apr. Shortwave fadeouts 
are probable.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 17 Apr
       Daily Proton Fluence >1 MeV:   9.0E+05
       Daily Proton Fluence >10 MeV:  1.5E+04
       Daily Electron Fluence >2 MeV: 9.10E+05   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C1.9

DSCOVR Satellite Solar Wind Day Averaged Data for 17 Apr
Speed: 365 km/sec  Density:    5.5 p/cc  Temp:    56600 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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