[Ips-dsgr] ASWFC Daily Report - 21 April 24 issued 2330 UT on 21 Apr 2024 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Mon Apr 22 09:30:58 EST 2024


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/21 APRIL 2024
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 21 APRIL AND FORECAST FOR 22 APRIL - 24 APRIL
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 21 Apr:  R1

Flares    Max     Fadeout    Freq.  Sectors
  M1.0    1259UT  possible   lower  European
  M2.2    1514UT  possible   lower  South American/
                                    Atlantic
  M3.4    2152UT  possible   lower  East Pacific/
                                    North American

Observed 10.7 cm flux/Equivalent Sunspot Number for 21 Apr: 217/167


1B. SOLAR FORECAST
             22 Apr             23 Apr             24 Apr
Activity     R1-R2              R1-R2              R1-R2 
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   215/165            215/165            200/152

COMMENT: Solar activity on UT day 21-Apr was R1, with three M 
class flares observed. There are currently thirteen numbered 
sunspots on the visible solar disk, with several additional regions 
currently rotating over the western solar limb. The complex cluster 
of sunspots in the southwestern solar hemisphere remained relatively 
stable in size and complexity, with some signs of redistribution 
observed. All flares observed originated from this cluster. AR3645 
(S08W30, beta-gamma) is the largest and the most complex region. 
Other regions in the cluster have begun to show signs of decay. 
Outside of this cluster, AR3646 (N22E11, beta) and AR3649 (N17W47, 
alpha) have shown signs of growth, AR3650 (S11W06, beta) has 
shown signs of growth in its intermediate and trailer spots, 
and AR3652 (N15E31, beta-gamma) has grown rapidly over UT day 
21 -Apr. All other sunspot regions are either stable or decaying. 
Solar activity over 22-24 Apr is expected to be R1-R2. Some activity 
originating within the complex cluster of sunspots in the southwest 
has been associated with narrow and weak CMEs, the material appears 
to be mostly directed to the south and west. It is not expected 
this activity will be significantly geoeffective, although weak 
impacts are possible from 24-Apr. No other significantly geo-effective 
CMEs were observed. S0 solar radiation storm conditions were 
observed on 21-Apr. S0 solar radiation storm conditions are expected 
over 22-24 Apr. The solar wind speed remained slightly enhanced, 
increasing slightly across UT day 21-Apr. This increase may be 
attributable to a weak glancing arrival of CMEs observed in recent 
days. Solar wind speed ranged from 360 to 515 km/s and is currently 
at around 455 km/s. The peak total interplanetary field strength 
(IMF, Bt) was 8 nT and the north-south IMF component range (Bz) 
was +3 to -6 nT. Isolated periods of southward Bz were also observed. 
The solar wind may remain mildly enhanced over 22-24 Apr due 
to weak glancing blows associated with recent CME activity. Otherwise, 
the solar wind speed should tend to background levels over 22-24 
Apr.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 21 Apr: G0

Estimated Indices 21 Apr : A   K           
   Australian Region      15   22244333
      Cocos Island         9   22223322
      Darwin              11   22234232
      Townsville          15   32244332
      Learmonth           16   32244333
      Alice Springs       14   22244233
      Gingin              16   22244334
      Canberra            14   22343333
      Kennaook Cape Grim  15   23343333
      Hobart              17   23344333    

Estimated Antarctic Regional K Indices 21 Apr :
      Macquarie Island    37   32475442
      Casey               13   33233323
      Mawson              46   54433755

Observed Regional daily pc3 Indices 21 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 21 Apr : A 
           Fredericksburg        15
           Planetary             19                         

Observed AFr/Ap Indices 20 Apr :  A   K
           Fredericksburg        10
           Planetary             12   2134 2333     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
22 Apr     8    G0-G1
23 Apr     8    G0-G1
24 Apr     8    G0-G1

COMMENT: ASWFC Geomagnetic Warning 16 was issued on 21 April 
and is current for 21-24 Apr. G0 geomagnetic conditions were 
observed in the Australian region on UT day 21-Apr. Mostly G0 
geomagnetic conditions were observed in Antarctica, with isolated 
periods of G2 observed. One period of G3 geomagnetic conditions 
was observed in Macquarie Island. G0 geomagnetic conditions are 
expected over 22-24 Apr, with a chance for G1 due to the potential 
arrival of recently observed CME activity.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
22 Apr      Normal         Normal         Normal-fair
23 Apr      Normal         Normal         Normal-fair
24 Apr      Normal         Normal         Normal-fair

COMMENT: HF radio communication on UT day 21-Apr was generally 
normal at low latitudes, but degraded near mid to high latitudes 
due to ongoing impacts of recent geomagnetic storm and CME activity. 
HF radio conditions over 22-24 are generally expected to be normal 
to fair. Shortwave fadeouts are possible.

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


Date   T index
21 Apr   138

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values during local day.
      Enhanced by 30% during local night.
      Enhanced by 20% after local dawn.
   Niue Island Region:
      Enhanced by 25% during local day.
      Enhanced by 20% during local night.
   Northern Australian Region:
      Mostly near predicted monthly values.
      Enhanced by 25% after local dawn.
   Southern Australian Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Davis/Mawson):
      Depressed by 20% 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
22 Apr   135    Near predicted monthly values
23 Apr   135    Near predicted monthly values
24 Apr   135    Near predicted monthly values

COMMENT: ASWFC SWF HF Communications Warning 40 was issued on 
21 April and is current for 22-24 Apr. Maximum usable frequencies 
(MUFs) in the northern Australian region on UT day 21-Apr were 
near predicted monthly values, with 25% enhancement observed 
after local dawn. MUFs in the southern Australian region were 
near predicted monthly values. Spread-F was observed in Hobart 
during local night hours. Periods of sporadic-E were observed 
in Brisbane and Perth. MUFs in the Australian region are expected 
to be near predicted monthly values over 22-24 Apr with some 
mild depressions possible due to geomagnetic activity. Shortwave 
fadeouts are possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 20 Apr
       Daily Proton Fluence >1 MeV:   1.9E+05
       Daily Proton Fluence >10 MeV:  1.6E+04
       Daily Electron Fluence >2 MeV: 1.50E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C1.7

DSCOVR Satellite Solar Wind Day Averaged Data for 20 Apr
Speed: 459 km/sec  Density:    0.8 p/cc  Temp:   105000 K  Bz:  -3 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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