[Ips-dsgr] ASWFC Daily Report - 02 May 24 issued 2330 UT on 02 May 2024 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Fri May 3 09:30:46 EST 2024


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/02 MAY 2024
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 02 MAY AND FORECAST FOR 03 MAY - 05 MAY
STATUS INDICATORS SOL:** YELLOW **   MAG:** RED **     ION: ** RED **
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 02 May:  R1

Flares    Max     Fadeout    Freq.  Sectors
  M1.0    0217UT  possible   lower  E. Asia/Aust.
  M2.7    2057UT  possible   lower  East Pacific/
                                    North American

Observed 10.7 cm flux/Equivalent Sunspot Number for 02 May: 142/96


1B. SOLAR FORECAST
             03 May             04 May             05 May
Activity     R1                 R1                 R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   135/89             132/86             132/86

COMMENT: Solar activity on UT day 02-May was R1, due to an M1.0 
flare from AR3663(N26E16, beta-gamma) and an M2.7 flare from 
AR3664(S18E54, beta-gamma). These solar regions have shown growth 
in the past 24 hours. Large solar region AR3654(S06W88, --) is 
almost completely off disk, with its trailer spots just visible. 
There are currently seven numbered sunspot regions on the solar 
disk. Other solar regions are small and stable or in decay. Solar 
activity is expected to be R1 over 03-05 May. No Earth directed 
CMEs were observed on 02-May in the available imagery. A westward 
CME was observed from 02/1036UT in LASCO C2 which could not be 
confidently correlated with on disk activity, possibly from AR3654 
just over the western solar limb. S0 solar radiation storm conditions 
were observed on 02-May. S0 solar radiation storm conditions 
are expected over 03-05 May. An unexpected shock was observed 
in the solar wind at 02/1315UT. The interplanetary magnetic field 
became enhanced due to the CME transit. The peak total interplanetary 
field strength (IMF, Bt) reached 22 nT and the north-south IMF 
component (Bz) range was +18 to -19 nT with Bz becoming strongly 
southward during the interval 02/1315-1900UT, then swinging northwards. 
The solar wind speed ranged from approximately 323 km/s to 477 
km/s. The solar wind speed was only moderately elevated following 
the shock arrival. The temperature parameter of the solar wind 
data did not show a discontinuity preventing auto detection. 
A small isolated coronal hole is visible centred at N12W15, which 
may mildly increase solar wind speed during 04-05 May. A solar 
filament with centre located at S35W12 is showing movement over 
the past two days and could be unstable.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 02 May: G1

Estimated Indices 02 May : A   K           
   Australian Region      21   22234553
      Cocos Island        16   22234443
      Townsville          22   22334553
      Learmonth           26   32335553
      Alice Springs       21   22234553
      Gingin              26   32334562
      Canberra            21   12234553
      Kennaook Cape Grim  25   12234563
      Hobart              21   12234553    

Estimated Antarctic Regional K Indices 02 May :
      Macquarie Island    35   11255663
      Casey               17   22333353
      Mawson              36   33343573

Observed Regional daily pc3 Indices 02 May : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               2   (Quiet)
      Canberra             5   (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 02 May : A 
           Fredericksburg        24
           Planetary             45                         

Observed AFr/Ap Indices 01 May :  A   K
           Fredericksburg        10
           Planetary             10   4220 2232     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
03 May    25    G1, chance G2 early in the UT day
04 May    12    G0
05 May     8    G0

COMMENT: ASWFC Geomagnetic Warning 18 was issued on 2 May and 
is current for 2-3 May. G1 geomagnetic conditions were observed 
in the Australian region on UT day 02-May. G1-G3 geomagnetic 
conditions were observed in the Antarctic region. The planetary 
Kp geomagnetic index reached G3 for two periods 02/15-21UT. The 
geomagnetic storm activity followed an unexpected CME arrival 
observed in the solar wind at 02/1315UT, with a a weak (12nT) 
impulse observed in the regional geomagnetic field at 02/1408UT. 
The geomagnetic storm conditions are expected to decline today.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
03 May      Normal         Fair           Fair-poor
04 May      Normal         Fair-normal    Fair-normal
05 May      Normal         Normal         Normal-fair

COMMENT: HF radio communication conditions were initially normal 
on 02-May becoming degraded at middle to high latitudes during 
the second half of the UT day. The degraded conditions were due 
to an unexpected CME arrival inducing geomagnetic storm activity. 
HF radio communication conditions are expected to degraded for 
middle to high latitudes on 03-May, with low latitude conditions 
remaining normal. Improved HF conditions for middle to high latitudes 
are expected for 04-May. Isolated minor shortwave fadeouts are 
possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
02 May   108

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values during local day.
      Depressed by 15% during local night.
   Niue Island Region:
      Near predicted monthly values during local day.
      Enhanced by 20% during local night.
   Northern Australian Region:
      Near predicted monthly values.
   Southern Australian Region:
      Mostly near predicted monthly values.
      Depressed by 35% after local dawn.
   Antarctic Region (Casey/Davis/Mawson):
      Depressed by 20% 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
03 May    70    Depressed 20 to 30%/near predicted monthly values
04 May   120    Near predicted monthly values
05 May   120    Near predicted monthly values

COMMENT: ASWFC HF Communications Warning 44 was issued on 2 May 
and is current for 3 May only. Maximum usable frequencies (MUFs) 
on UT day 02-May were mostly near predicted monthly values in 
the Australian region during the local day. Degraded conditions 
were observed during local night hours due to the onset of geomagnetic 
activity, with strong spread F observed at Hobart. Spread F was 
observed at Canberra and Perth. After local dawn this morning 
southern Australian regional MUFs were depressed 20-30%. Northern 
Australian regional MUFs are mostly near normal. Depressed and 
degraded HF conditions are now expected for the southern Australian 
region for 03-May. Isolated minor shortwave fadeouts are possible.
Ionospheric scintillation was observed 02/0833-1413UT at Darwin and Niue.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 01 May
       Daily Proton Fluence >1 MeV:   1.6E+05
       Daily Proton Fluence >10 MeV:  1.8E+04
       Daily Electron Fluence >2 MeV: 1.20E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B9.0

DSCOVR Satellite Solar Wind Day Averaged Data for 01 May
Speed: 369 km/sec  Density:    6.7 p/cc  Temp:    20600 K  Bz:   9 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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