[Ips-dsgr] ASWFC Daily Report - 31 May 23 issued 2340 UT on 31 May 2023 [SEC=OFFICIAL]

rwc rwc at ips.gov.au
Thu Jun 1 09:40:48 EST 2023


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/31 MAY 2023
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 31 MAY AND FORECAST FOR 01 JUNE - 03 JUNE
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
Corrected copy: flare list.
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1A. SOLAR SUMMARY
Activity 31 May:  R1

Flares    Max     Fadeout    Freq.  Sectors
  M1.0    0438UT  possible   lower  E. Asia/Aust.
  M1.0    1226UT  possible   lower  European
  M1.0    2208UT  possible   lower  East Pacific/
                                    North American
  M4.2    2252UT  possible   lower  East Pacific/
                                    North American

Observed 10.7 cm flux/Equivalent Sunspot Number for 31 May: 161/115


1B. SOLAR FORECAST
             01 Jun             02 Jun             03 Jun
Activity     R1,chance R2       R1,chance R2       R1,chance R2
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   160/114            160/114            150/105

COMMENT: Solar activity on UT day 31-May reached R1 due to an 
M4.2 flare from AR3323(S05E72, beta) and low level M-class solar 
flares. Additional spots are rotating onto the disk behind AR3323. 
This region is currently located well to the east in solar longitude 
with any subsequent flare associated CMEs likely to miss the 
Earth. Solar region AR3319(S19W24, beta-gamma) produced the later 
M1 event (SDO304/GONG H-alpha 31/1228UT). This region has recently 
shown rapid growth, though this now appears to have more recently 
slowed. Solar region AR3321(S15E57, beta) appears as a medium 
sized single spot and has been flare quiet. The largest region 
on disk AR3315(S17W56, beta) continues to show decay in its trailer 
spots and only produced minor C flares and is now located quite 
westward. Solar activity is expected to be at the R1 level, with 
the chance of an R2 event due to currently flare active AR3323. 
There are currently 10 numbered sunspot regions on the disk. 
Other sunspot regions are relatively small. No significant Earth 
directed CMEs were observed. On disk plasma motion in SDO304 
imagery at 31/0937UT, N35W35, associated with small filament 
activity did not appear to have an associated CME. A slow narrow 
CME was observed to the southwest from 31/0136UT in LASCO C2 
imagery but could not be correlated to on disk activity. The 
solar wind speed on UT day 31-May ranged between 336 to 427 km/s. 
The peak total interplanetary magnetic field strength (IMF, Bt) 
was 8 nT and the north-south IMF component (Bz) range was +7 
to -8 nT, with mild fluctuations southward during the UT day. 
A large southern coronal hole located at a moderately high solar 
latitude (S40) and a small isolated equatorial coronal hole are 
currently both at solar central meridian. There are weak 27 day 
solar wind recurrent patterns of increased solar wind speed of 
up to 500km/sec for 02 and 04 June.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 31 May: G0

Estimated Indices 31 May : A   K           
   Australian Region       5   11211132
      Cocos Island         5   11121131
      Darwin               4   11211122
      Townsville           6   11221132
      Learmonth            7   21221232
      Alice Springs        4   10211032
      Gingin               6   11211232
      Canberra             4   01212121
      Hobart               6   11212231    

Estimated Antarctic Regional K Indices 31 May :
      Macquarie Island     7   00313321
      Casey                9   23232222
      Mawson              23   43431255

Observed Regional daily pc3 Indices 31 May : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             2   (Quiet)
      Hobart               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 31 May : A 
           Fredericksburg         6
           Planetary              5                         

Observed AFr/Ap Indices 30 May :  A   K
           Fredericksburg         6
           Planetary              5   1011 2112     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
01 Jun     6    G0
02 Jun    13    G0, slight chance of G1
03 Jun     8    G0

COMMENT: G0 geomagnetic conditions were generally observed in 
both the Australian and Antarctic regions on UT day 31-May, with 
two periods of G1 at Mawson. G0 geomagnetic conditions are generally 
expected over 01-03-Jun. There are weak 27 day geomagnetic recurrent 
patterns for 02-Jun and 04-Jun, with a chance of an isolated 
G1 period on these days.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
01 Jun      Normal         Normal         Normal-fair
02 Jun      Normal         Normal         Fair
03 Jun      Normal         Normal         Fair-normal

COMMENT: HF communication conditions on UT day 31-May were mostly 
normal. Degraded conditions were observed during local night 
hours for middle to high latitudes. HF communication conditions 
are expected to be generally normal to fair during 01-03-Jun, 
with degradations possible during local night hours on 02-Jun 
for middle to high latitudes. Isolated shortwave fadeouts are 
possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
31 May    93

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values.
   Niue Island Region:
      Near predicted monthly values.
   Northern Australian Region:
      Mostly near predicted monthly values.
   Southern Australian Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day.

Monthly T index:
Month  T index
Apr      120
May      87
Jun      88

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
01 Jun    95    Near predicted monthly values
02 Jun    95    Near predicted monthly values
03 Jun    95    Near predicted monthly values

COMMENT: Maximum usable frequencies (MUFs) on UT day 31-May were 
near predicted monthly values. Strong spread-F was observed at 
Hobart during local night hours. A fadeout impacting lower HF 
frequencies was observed at Niue at 21/2300UT. MUFs are expected 
to be near predicted monthly values over 01-03-Jun. Shortwave 
fadeouts are possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 30 May
       Daily Proton Fluence >1 MeV:   3.4E+04
       Daily Proton Fluence >10 MeV:  2.3E+04
       Daily Electron Fluence >2 MeV: 1.60E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 3%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C1.3

DSCOVR Satellite Solar Wind Day Averaged Data for 30 May
Speed: 380 km/sec  Density:    2.0 p/cc  Temp:    17900 K  Bz:   3 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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