[Ips-dsgr] ASWFC Daily Report - 26 August 24 issued 2330 UT on 26 Aug 2024 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Tue Aug 27 09:30:50 AEST 2024


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/26 AUGUST 2024
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 26 AUGUST AND FORECAST FOR 27 AUGUST - 29 AUGUST
STATUS INDICATORS SOL:** YELLOW **   MAG:** YELLOW **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 26 Aug:  R1

Flares    Max     Fadeout    Freq.  Sectors
  M1.4    1141UT  possible   lower  European

Observed 10.7 cm flux/Equivalent Sunspot Number for 26 Aug: 232/182


1B. SOLAR FORECAST
             27 Aug             28 Aug             29 Aug
Activity     R1,chance R2       R1,chance R2       R1,chance R2
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   230/180            235/185            242/191

COMMENT: Solar activity on UT day 26-Aug was at the R1 level 
due to an M1.4 flare from solar region AR3796 (S04W37, beta-gamma-delta). 
The intermediate spots of region AR3796 have exhibited both growth 
and decay. The trailer spots of solar regions AR3790 (S13W72, 
beta) and AR3799 (S09W02, beta) are both declining. Solar region 
AR3800 (S27W16, beta-gamma-delta) and AR3801 (N09E10, beta) are 
both developing. There are currently ten numbered sunspot regions 
visible on the solar disk. All other sunspot regions are either 
stable or in decay. A channel of plasma emission/motion was observed 
in SDO 304 imagery located from S45E25 to S10E05 from 26/1718UT. 
In GOES SUVI 195 imagery this activity appears to connect in 
an arch to location S35E60 visible at 26/1828UT. However, no 
solar filament eruption in GONG H-alpha imagery could be identified 
in the southeast solar quadrant. South polar limb prominence 
activity was also observed in GOES SUVI 304 imagery 26/1200-1300UT. 
Solar activity is expected to be at the R1, chance R2 level over 
27-29 Aug. No significantly Earth directed CMEs have been observed. 
A coronal streamer erupted from 26/1325UT with a bright slow 
southward out of the ecliptic plane directed CME. The on disk 
plasma arch motion appeared to have occurred after this CME began 
erupting. Event modelling of this slow streamer CME was conducted 
assuming a southeast disk location and shows an Earth miss. The 
solar wind speed on UT day 26-Aug slowly declined, ranging from 
260 to 325 km/s and is currently near 260 km/s. The peak total 
interplanetary field strength (IMF, Bt) was 5 nT and the north-south 
IMF component (Bz) range was +2 to -4 nT. The solar wind speed 
is expected to mildly increase on 27-Aug due to the arrival of 
a CME first observed on 23-Aug. Old solar region AR3777 which 
previously produced isolated R2 and R3 level flare activity is 
due to return to the southeast solar limb (solar latitude S09) 
on 27-Aug. However, this region was rapidly declining in area 
as it approached the western solar limb on its previous rotation. 
A small coronal hole with centre located at S05W15 may slightly 
increase the solar wind speed on 29-Aug.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 26 Aug: G0

Estimated Indices 26 Aug : A   K           
   Australian Region       1   11101100
      Cocos Island         2   21110000
      Darwin               2   12101101
      Townsville           4   21102112
      Learmonth            1   11001100
      Alice Springs        1   01101101
      Gingin               2   11102200
      Canberra             1   10002100
      Kennaook Cape Grim   2   11012200
      Hobart               2   11012200    

Estimated Antarctic Regional K Indices 26 Aug :
      Macquarie Island     4   00033200
      Casey                4   23200100
      Mawson               7   32111223

Observed Regional daily pc3 Indices 26 Aug : 
      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 26 Aug : A 
           Fredericksburg         6
           Planetary              6                         

Observed AFr/Ap Indices 25 Aug :  A   K
           Fredericksburg         8
           Planetary              6   2221 1121     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
27 Aug    16    G0, chance G1
28 Aug    10    G0
29 Aug     8    G0

COMMENT: G0 geomagnetic conditions were observed in the Australian 
and Antarctic region on UT day 26-Aug. G0 geomagnetic conditions 
are expected over 27-29 Aug, with a chance of G1 on 27-Aug due 
to the arrival of a CME first observed on 23-Aug.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
27 Aug      Normal         Normal-fair    Fair
28 Aug      Normal         Normal         Normal-fair
29 Aug      Normal         Normal         Normal-fair

COMMENT: HF radio communication conditions on UT day 26-Aug were 
normal. HF radio communication conditions are expected to be 
generally normal over 27-29 Aug, with fair conditions at high 
latitudes on 27-Aug. Shortwave fadeouts are possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
26 Aug   152

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 30% during local day.
      Enhanced by 115% during local night.
   Niue Island Region:
      Enhanced by 15%.
   Northern Australian Region:
      Near predicted monthly values.
   Southern Australian Region:
      Enhanced by 15-20%.
   Antarctic Region (Casey/Davis/Mawson):
      Enhanced by 20% over the UT day.

Monthly T index:
Month  T index
Jul      131
Aug      119
Sep      119

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
27 Aug   145    Near to 15% above predicted monthly values
28 Aug   145    Near to 15% above predicted monthly values
29 Aug   145    Near to 15% above predicted monthly values

COMMENT: ASWFC SWF HF Communications Warning 95 was issued on 
26 August and is current for 26-28 Aug. Maximum usable frequencies 
(MUFs) in the Australian region on UT day 26-Aug were near predicted 
monthly values to 15% enhanced. Very strong enhancements were 
observed at Cocos Island during local night hours. Spread F was 
observed during local night hours at Hobart. MUFs are expected 
to be near predicted monthly values to 15% enhanced over 27-29 
Aug. Shortwave fadeouts are possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 25 Aug
       Daily Proton Fluence >1 MeV:   3.7E+04
       Daily Proton Fluence >10 MeV:  1.8E+04
       Daily Electron Fluence >2 MeV: 3.70E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C1.9

DSCOVR Satellite Solar Wind Day Averaged Data for 25 Aug
Speed: 344 km/sec  Density:    2.8 p/cc  Temp:    47300 K  Bz:   0 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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