[Ips-dsgr] ASWFC Daily Report - 08 June 24 issued 2330 UT on 08 Jun 2024 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Sun Jun 9 09:30:42 AEST 2024


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/08 JUNE 2024
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 08 JUNE AND FORECAST FOR 09 JUNE - 11 JUNE
STATUS INDICATORS SOL:** YELLOW **   MAG:** RED **     ION: ** YELLOW **
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 08 Jun:  R2

Flares    Max     Fadeout    Freq.  Sectors
  M1.8    0028UT  possible   lower  West Pacific
  M3.4    0051UT  possible   lower  West Pacific
  M9.7    0150UT  probable   lower  West Pacific
  M1.5    0528UT  possible   lower  E. Asia/Aust.
  M1.2    0844UT  possible   lower  Mid East/Indian

Observed 10.7 cm flux/Equivalent Sunspot Number for 08 Jun: 190/143


1B. SOLAR FORECAST
             09 Jun               10 Jun               11 Jun
Activity     R0-R1, chance R2-R3  R0-R1, chance R2-R3  R0-R1, chance R2-R3
Fadeouts     Possible             Possible             Possible
10.7cm/SSN   190/143              175/129              175/129

COMMENT: Solar activity on UT day 08-Jun was R2. Two R1 flares 
were observed from near AR3707 (S18E35, beta). A long duration 
R2 level flare that was categorised as M9.6 was observed from 
AR3697 (S18W68, gamma), in addition to four other low-level M-class 
flares. There are currently nine numbered sunspot regions on 
the solar disk. AR3697 has been slightly unstable, but otherwise 
all other sunspot regions are either stable or in decay. Solar 
activity over 09-11 Jun is expected to be predominantly R0-R1, 
with a chance for R2-R3 flares. 

The M9 flare from AR3697 as associated with a fast  asymmetric halo CME. 
A filament was weaved throughout the sunspot region, which appeared 
to be ripped out during the flare event. This CME has been assessed
 to have an Earth-directed component, however models are suggesting 
a high variability in the time of arrival. Current modelling suggests 
a likely arrival in the second half of UT day 10-Jun. 
No other CMEs were observed on 08-Jun.

 In response to the M9 flare event, the 10 MeV, 50 MeV 
and 100 MeV protons rose. The 10 MeV protons peaked at 1030 pfu, 
just briefly breaching S3 solar radiation storm conditions. S1 
solar radiation storm conditions are expected on 09-Jun, before 
falling to near background levels. 

The solar wind environment was slightly disturbed at the beginning
 of the day, but currently is near background levels. The maximum 
solar wind speed observed was 555 km/s, but is currently near 470 km/s.
 The peak total interplanetary field strength (IMF, Bt) was 12 nT and the 
north-south IMF component (Bz) range was +11 to -6 nT. The solar 
wind is expected to stay near background levels until the arrival 
of the CME. Afterwards, disturbed conditions can be expected 
over 10-11 Jun.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 08 Jun: G0

Estimated Indices 08 Jun : A   K           
   Australian Region       8   32322211
      Cocos Island         5   22321200
      Darwin              10   42322212
      Townsville          11   42323212
      Learmonth            9   33322211
      Alice Springs        8   32322211
      Gingin              10   42322221
      Canberra             7   32222211
      Kennaook Cape Grim   8   32223221
      Hobart               9   32213321    

Estimated Antarctic Regional K Indices 08 Jun :
      Macquarie Island    10   42123311
      Casey               11   33332222
      Mawson              23   64332242

Observed Regional daily pc3 Indices 08 Jun : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               2   (Quiet)
      Canberra             2   (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 08 Jun : A 
           Fredericksburg        15
           Planetary             22                         

Observed AFr/Ap Indices 07 Jun :  A   K
           Fredericksburg        20
           Planetary             22   1323 5533     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
09 Jun     6    G0
10 Jun    28    G1-G2, chance G3
11 Jun    18    G1-G2

COMMENT: ASWFC Geomagnetic Warning 27 was issued on 8 June and 
is current for 10-11 Jun. G0 geomagnetic conditions were observed 
in the Australian region on UT day 08-Jun. Mostly G0 conditions 
were observed in Antarctica, with an isolated period of G2. G0 
geomagnetic conditions are expected on 09-Jun. G1-G2 geomagnetic 
conditions are expected to commence in the second half of UT 
day 10-Jun, with a chance for G3 due to an anticipated CME arrival. 
G1-G2 conditions are likely to persist on 11-Jun, but on a declining 
trend.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
08 Jun      Normal-fair    Normal         Poor(PCA)      

PCA Event : 10MeV Proton/PCA Event Began 08 06 2024 0250UT and is in progress
 and, 100MeV Proton/PCA Event Began at 0215UT 08/06, Ended at 1435UT 08/06

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
09 Jun      Normal         Normal         Poor(PCA)
10 Jun      Normal-fair    Fair           Fair
11 Jun      Normal-fair    Fair           Fair

COMMENT: HF radio communication conditions on UT day 08-Jun were 
mostly normal in low and middle latitudes, with some degraded 
conditions during local night hours. Conditions at high latitudes 
were poor due to an ongoing polar cap absorption (PCA) event. 
HF radio communication conditions are expected to be normal at 
low and middle latitudes and poor at high latitudes on 09-Jun, 
before becoming degraded over 10-11 Jun due to anticipated geomagnetic 
activity..

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
08 Jun   134

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values.
   Niue Island Region:
      Enhanced by 25% during local day.
      Near predicted monthly values during local night.
   Northern Australian Region:
      Mostly near predicted monthly values.
   Southern Australian Region:
      Near predicted monthly values during local day.
      Enhanced by 15% during local night.
   Antarctic Region (Casey/Davis/Mawson):
      Near predicted monthly values over the UT day.
      Proton event in progress, increased absorption observed.

Monthly T index:
Month  T index
May      121
Jun      116
Jul      117

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
09 Jun   120    Near predicted monthly values
10 Jun   105    Near predicted monthly values to 20% depressed
11 Jun   100    Near predicted monthly values to 20% depressed

COMMENT: ASWFC SWF HF Communications Warning 62 was issued on 
8 June and is current for 8-10 Jun. ASWFC Preliminary HF Communications 
Warning 63 was issued on 8 June and is current for 10-12 Jun. 
Maximum usable frequencies (MUFs) on UT day 08-Jun were mostly 
near predicted values to 15% enhanced. Spread-F was observed 
in Darwin and Hobart during local night hours. A polar cap absorption 
event began from around 08/0300 UT and is ongoing, blacking out 
radio signals at high latitudes. MUFs are expected to be near 
predicted monthly values on 09-Jun, but expected to become depressed 
after the CME arrival on 10-Jun into 11-Jun by 20%.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 07 Jun
       Daily Proton Fluence >1 MeV:   2.0E+05
       Daily Proton Fluence >10 MeV:  1.5E+04
       Daily Electron Fluence >2 MeV: 1.40E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C2.9

DSCOVR Satellite Solar Wind Day Averaged Data for 07 Jun
Speed: 422 km/sec  Density:    3.3 p/cc  Temp:   124000 K  Bz:  -2 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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