[Ips-dsgr] ASWFC Daily Report - 16 May 24 issued 2330 UT on 16 May 2024 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Fri May 17 09:30:47 EST 2024


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/16 MAY 2024
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 16 MAY AND FORECAST FOR 17 MAY - 19 MAY
STATUS INDICATORS SOL:** RED **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 16 May:  R1

Flares    Max     Fadeout    Freq.  Sectors
 M1/--    0804UT  possible   lower  Mid East/Indian

Observed 10.7 cm flux/Equivalent Sunspot Number for 16 May: 207/158


1B. SOLAR FORECAST
             17 May             18 May             19 May
Activity     R1-R2,chance R3    R1-R2,chance R3    R1-R2,chance R3
Fadeouts     Probable           Probable           Probable
10.7cm/SSN   200/152            190/143            180/133

COMMENT: Solar activity on UT day 16-May was at the R1 level 
due to an M1.0 flare from new solar region AR3685(S13E66, beta-gamma). 
This region produced the recent X2 flare. There is another smaller 
new region rotating onto the solar disk just to the north east 
of AR3685. Another region of note, AR3679(S12E22, beta-gamma) 
produced several C class flares over the last 24 hours. This 
region as shown a mix of development and decay and has grown 
in longitudinal extent. Solar regions AR3674(S13W00, beta) and 
AR3672(N18W35, beta) contributed to the low level C class flare 
activity. There are currently thirteen numbered solar regions 
on the visible solar disk. Solar region AR3683(S23W14, beta) 
is currently growing. All other regions were mostly stable or 
in decline. A solar filament eruption was observed in the GONG 
imagery from 16/1513-1730UT located at S03W33-N10W42. Associated 
plasma motion in SDO171/193 was very localised and slight suggesting 
a weaker eruption. Solar flare activity is expected to be at 
R1-R2, chance R3 over 17-19 May. Solar radiation conditions are 
now S0. S0 conditions are expected 17-19 May. No significantly 
Earth directed CMEs have been observed. A north west CME is visible 
in LASCO C2 from 16/1800UT. Data gaps in both space based coronagraphs 
(STERO-A and LASCO) restricted analysis. An analysis of the north 
west CME was conducted assuming pairing with the the filament 
eruption, though confidence is low due to the weak on disk plasma 
motion. The modelling shows a weak CME arrival is possible 20/1200UT 
+/- 12 hours. The solar wind parameters were mildly enhanced 
due to the indistinct transient of a weak CME. The solar wind 
speed on UT day 16-May ranged from 529 to 381 km/s and is currently 
near 384 km/s. The peak total interplanetary field strength (IMF, 
Bt) was 17 nT and the north-south IMF component (Bz) range was 
+14 to -13 nT. The IMF Bz was orientated southward during the 
interval 16/0445-0935UT. No coronal holes are visible near the 
solar central meridian.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 16 May: G1

Estimated Indices 16 May : A   K           
   Australian Region      15   23543201
      Cocos Island        10   13433210
      Darwin              16   23543212
      Townsville          16   23543212
      Learmonth           16   23544210
      Alice Springs       15   23543201
      Gingin              10   23433200
      Canberra            12   23443101
      Kennaook Cape Grim  17   23553101
      Hobart              17   23553100    

Estimated Antarctic Regional K Indices 16 May :
      Macquarie Island    24   24654110
      Casey               12   34432111
      Mawson              19   34544211

Observed Regional daily pc3 Indices 16 May : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               2   (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 16 May : A 
           Fredericksburg        19
           Planetary             29                         

Observed AFr/Ap Indices 15 May :  A   K
           Fredericksburg        10
           Planetary             10   1232 2233     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
17 May    15    G0, chance G1
18 May    12    G0
19 May     8    G0

COMMENT: ASWFC Geomagnetic Warning 26 was issued on 15 May and 
is current for 15-17 May. G1 geomagnetic conditions were observed 
in the Australian region on UT day 16-May. In the Antarctic region 
conditions were G0 at Casey, with a G1 period observed at Mawson 
and G1-G2 periods observed at Macquarie Island. The mild increase 
in geomagnetic activity was due to a weak CME transient. G0 conditions, 
with a chance of G1 are expected on 17-May. G0 conditions are 
expected on 18-19 May.

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

PCA Event : 10MeV Proton/PCA Event Began at 1355UT 13/05, Ended at 1410UT 16/05

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
17 May      Normal         Normal         Fair-normal
18 May      Normal         Normal         Normal-fair
19 May      Normal         Normal         Normal-fair

COMMENT: HF radio communication conditions on UT day 16-May were 
mostly normal, with some degradation at high latitudes. Mostly 
normal conditions are expected over 17-19 May, with mild degradation 
possible at high latitudes on 17-May. Isolated shortwave fadeouts 
are expected.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
16 May   136

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 15% during local day.
      Near predicted monthly values during local night.
   Niue Island Region:
      Enhanced by 20-40%.
   Northern Australian Region:
      Near predicted monthly values.
   Southern Australian Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Davis/Mawson):
      Depressed by 15% 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
17 May   120    Near predicted monthly values
18 May   120    Near predicted monthly values
19 May   120    Near predicted monthly values

COMMENT: ASWFC SWF HF Communications Warning 53 was issued on 
16 May and is current for 16-18 May. Maximum usable frequencies 
(MUFs) on UT day 16-May were mostly near predicted monthly values. 
Spread F was observed at Hobart during local night hours. Enhanced 
MUFs were observed at Niue. MUFs are expected to be near predicted 
monthly values over 17-19 May. Isolated shortwave fadeouts are 
expected.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 15 May
       Daily Proton Fluence >1 MeV:   2.8E+07
       Daily Proton Fluence >10 MeV:  2.2E+06
       Daily Electron Fluence >2 MeV: 6.30E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 8%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C3.4

DSCOVR Satellite Solar Wind Day Averaged Data for 15 May
Speed: 508 km/sec  Density:    6.0 p/cc  Temp:   247000 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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