[Ips-dsgr] ASWFC Daily Report - 09 May 24 issued 2332 UT on 09 May 2024 [SEC=OFFICIAL]

rwc rwc at ips.gov.au
Fri May 10 09:32:17 EST 2024


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/09 MAY 2024
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 09 MAY AND FORECAST FOR 10 MAY - 12 MAY
STATUS INDICATORS SOL:** RED **   MAG:** RED **     ION: ** RED **
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 09 May:  R3

Flares    Max     Fadeout    Freq.  Sectors
  M4.0    0317UT  possible   lower  E. Asia/Aust.
  M4.5    0332UT  possible   lower  E. Asia/Aust.
  X2.2    0913UT  probable   all    Mid East/Indian
  X1.1    1744UT  probable   all    South American/
                                    Atlantic
  M1.0    2121UT  possible   lower  East Pacific/
                                    North American
  M2.7    2241UT  possible   lower  East Pacific/
                                    North American

Observed 10.7 cm flux/Equivalent Sunspot Number for 09 May: 233/183


1B. SOLAR FORECAST
             10 May             11 May             12 May
Activity     R2-R3              R2-R3              R2-R3
Fadeouts     Probable           Probable           Probable
10.7cm/SSN   230/180            225/175            220/170

COMMENT: Solar activity on UT day 09-May was at the R3 level 
due to two X-class flares. The strongest flare was an X2.2 at 
09/0913UT from AR3664 (S20W31, beta-gamma-delta). An X1.1 flare 
was observed at 09/1744UT, also produced by AR3664. Several other 
flares at R1-R2 levels were observed over the UT day. There are 
currently seven numbered sunspot regions visible on the solar 
disk. AR3664 is the largest and most magnetically complex region 
and has exhibited spot development in its trailer spots over 
the UT day. This region has continued to grow in size and maintains 
multiple delta spots in its current configuration. AR3663 (N25W82, 
beta) appeared to show decay in its intermediate spots and is 
now rotating over the western limb. AR3666 (N07W65, beta) has 
developed a small trailer spot. Newly numbered regions AR3671 
(N20E34, beta) and AR3672 (N18E58, beta) both recently appeared 
on the solar disk and have shown spot growth. All other sunspot 
regions are either stable or in decay. Solar activity is expected 
to be at R2-R3 levels over 10-12 May. A mild enhancement in the 
proton flux was observed on 09-May, with conditions remaining 
at S0. S0-S1 solar radiation conditions are expected over 10-12 
May. A halo CME was observed late on 08-May, visible in LASCO 
C2 coronagraph imagery from 08/2224UT. This CME is likely associated 
with the X1.0 flare at 08/2140UT from AR3664. Modelling indicates 
this CME is Earth-directed and is the third successive halo CME 
to be geoeffective. On UT day 09-May a fourth halo CME was observed, 
visible in coronagraph imagery from 09/0936UT. This CME is associated 
with the aforementioned X2.2 flare from AR3664, with modelling 
indicating this CME is also Earth-directed. The first three halo 
CMEs are expected to merge into a combined front, estimated to 
arrive at Earth at 10/1000UT +/- 10 hours. The fourth halo CME 
is estimated to arrive later in the UT day at 10/1700UT. A partial 
halo CME was observed, visible in LASCO C2 coronagraph imagery 
from 09/1852UT. Analysis of this CME is ongoing. No other Earth-directed 
CMEs have been observed. The solar wind speed on UT day 09-May 
mildly declined, ranging from 410 to 480 km/s and is currently 
near 420 km/s. The peak total interplanetary field strength (IMF, 
Bt) was 7 nT and the north-south IMF component (Bz) range was 
+4 to -5 nT. A small northern hemisphere coronal hole is now 
in the western hemisphere and may influence the solar wind speed 
over the coming days. The solar wind speed is expected to increase 
over 10-12 May due to the arrival of four halo CMEs first observed 
over 08-09 May.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 09 May: G0

Estimated Indices 09 May : A   K           
   Australian Region       2   11110021
      Cocos Island         2   11120011
      Darwin               3   12110021
      Townsville           3   11110121
      Learmonth            3   12110022
      Alice Springs        2   11100021
      Gingin               3   12010022
      Canberra             2   02000111
      Kennaook Cape Grim   2   11000121
      Hobart               2   01000121    

Estimated Antarctic Regional K Indices 09 May :
      Macquarie Island     0   01010000
      Casey                7   24211121
      Mawson              11   14111234

Observed Regional daily pc3 Indices 09 May : 
      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 09 May : A 
           Fredericksburg         9
           Planetary             11                         

Observed AFr/Ap Indices 08 May :  A   K
           Fredericksburg        10
           Planetary              6   1112 2212     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
10 May    80    G4
11 May    50    G3, chance of G4
12 May    18    G1

COMMENT: ASWFC Geomagnetic Warning 22 was issued on 9 May and 
is current for 10-12 May. G0 geomagnetic conditions were observed 
in the Australian and Antarctic regions on UT day 09-May. G4 
geomagnetic conditions are expected on 10-May due to the arrival 
of four halo CMEs first observed over 08-09 May. G3 geomagnetic 
conditions are expected on 11-May, with a chance of G4 due to 
ongoing CME effects. G1 geomagnetic conditions are expected on 
12-May as CME effects abate.

-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
09 May      Normal         Normal         Normal         

PCA Event : No event.

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

COMMENT: HF radio communication conditions on UT day 09-May were 
generally normal, though with frequent fadeouts impacting lower 
HF frequencies. HF radio communication conditions are expected 
to be fair to poor over 10-12 May due to expected geomagnetic 
activity. Frequent shortwave fadeouts are expected.

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


Date   T index
09 May   111

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values during local day.
      Enhanced by 35% 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
Apr      125
May      114
Jun      116

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
10 May    70    20 to 30% below predicted monthly values
11 May    50    30 to 40% below predicted monthly values
12 May    90    Depressed 15%/near predicted monthly values

COMMENT: ASWFC Preliminary HF Communications Warning 49 was issued 
on 9 May and is current for 10-12 May. ASWFC SWF HF Communications 
Warning 50 was issued on 9 May and is current for 10-12 May. 
Maximum usable frequencies (MUFs) on UT day 09-May were near 
predicted monthly values. MUFs are expected to be depressed by 
20-40% over 10-12 May due to anticipated geomagnetic activity. 
Frequent shortwave fadeouts are expected.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 08 May
       Daily Proton Fluence >1 MeV:   8.9E+04
       Daily Proton Fluence >10 MeV:  1.9E+04
       Daily Electron Fluence >2 MeV: 2.70E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C6.1

DSCOVR Satellite Solar Wind Day Averaged Data for 08 May
Speed: 470 km/sec  Density:    2.2 p/cc  Temp:    74600 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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