[Ips-dsgr] ASWFC Daily Report - 02 October 22 issued 2331 UT on 02 Oct 2022 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Mon Oct 3 10:31:14 EST 2022


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/02 OCTOBER 2022
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 02 OCTOBER AND FORECAST FOR 03 OCTOBER - 05 OCTOBER
STATUS INDICATORS SOL:** RED **   MAG:** YELLOW **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 02 Oct:  R3

Flares    Max     Fadeout    Freq.  Sectors
  M8.8    0221UT  probable   lower  E. Asia/Aust.
  M1.3    1405UT  possible   lower  South American/
                                    Atlantic
  M1.1    1545UT  possible   lower  South American/
                                    Atlantic
  X1.1    2025UT  probable   all    East Pacific/
                                    North American

Observed 10.7 cm flux/Equivalent Sunspot Number for 02 Oct: 154/109


1B. SOLAR FORECAST
             03 Oct             04 Oct             05 Oct
Activity     R1-R2, chance R3   R1-R2, chance R3   R1-R2, chance R3
Fadeouts     Probable           Possible           Possible
10.7cm/SSN   155/109            155/109            145/99

COMMENT: Solar activity on UT day 02-Sep reached R3 levels, with 
X-ray flux levels reaching X1.0. Two regions, AR3112 (N23E60, 
beta-gamma-delta) and AR3110 (N16W50, beta), produced flares 
at 02/2026UT contributing to the X1.0 flux. Both of these regions 
have grown in size and complexity over 02-Oct. There are currently 
five sunspot regions on the solar disk. In addition to the R3 
event, AR3110 (N16W50, beta) produced an M8.8 flare at 02/0220UT. 
AR3107 (S25W75, beta) appears to have decayed as it rotates over 
the western limb, however it produced an M1.0 flare at 02/1544UT. 
Region AR3113 (N16W40, beta) has been unstable, and all other 
regions are either stable or in decay. Solar activity is expected 
to be at predominantly R0-R1 levels over 03-05 Oct, with isolated 
R2 and R3 flares possible. Several filament eruptions were associated 
with the flaring activity from AR3110 on UT day 02-Oct and can 
be observed in GOES SUVI imagery. Several CMEs were observed 
in LASCO and STEREO-A imagery from 02/0236UT, 02/0548UT and 02/1514UT 
from the northwest quadrant of the solar disk. Analysis suggests 
these CMEs may interact, causing a glancing blow to Earth on 
04-Oct, however confidence in low. The solar wind speed on UT 
day 02-Oct steadily increased, and ranged from 387 to 588 km/s 
and is currently near 545 km/s, suggesting the late arrival of 
a coronal hole high speed wind stream. The solar wind is expected 
to remain elevated over 03-05 Oct due to the combined effects 
of coronal hole high speed wind streams and impacts of several 
recent CMEs. The peak total interplanetary field strength (IMF, 
Bt) was 9 nT and the north-south IMF component (Bz) range was 
+8 to -9 nT. Bz has been southward since 02/1950UT.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 02 Oct: G0

Estimated Indices 02 Oct : A   K           
   Australian Region       7   22122223
      Cocos Island         6   22122212
      Darwin               6   2212----
      Townsville          10   32132233
      Learmonth            9   22123323
      Alice Springs        9   22232223
      Gingin               8   31222223
      Canberra             7   22122223
      Hobart               9   22232223    

Estimated Antarctic Regional K Indices 02 Oct :
      Macquarie Island    15   21143325
      Casey               18   44432333
      Mawson              26   43223635

Observed Regional daily pc3 Indices 02 Oct : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             0   (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 02 Oct : A 
           Fredericksburg        10
           Planetary             13                         

Observed AFr/Ap Indices 01 Oct :  A   K
           Fredericksburg         2
           Planetary              3   0000 1112     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
03 Oct    20    G0-G1, chance G2
04 Oct    36    G1-G2, chance G3
05 Oct    26    G0-G1

COMMENT: G0 geomagnetic conditions were observed in the Australian 
region on UT day 02-Oct. Mostly G0 geomagnetic conditions were 
observed in the Antarctica region, with an isolated period of 
G2 at Mawson. G0-G1 conditions are generally expected on 03-Oct 
as the late arrival of a coronal hole high speed wind stream 
is expected to increase geomagnetic activity. G1-G2 geomagnetic 
conditions are expected on 04-Oct, as coronal hole effects continue 
and are combined with possible impacts from several recent CMEs. 
G0-G1 conditions are expected on 05-Oct as these effects ease.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
02 Oct      Normal         Normal         Normal         

PCA Event : No event.

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

COMMENT: Mostly normal HF propagation conditions are initially 
expected for 03-Oct, with degraded HF conditions possible over 
late 03-Oct to 05-Oct in response to anticipated geomagnetic 
activity, particularly in middle to high latitude regions during 
local night hours.

-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
02 Oct    93

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 25% during local day.
      Enhanced by 15% during local night.
   Niue Island Region:
      Near predicted monthly values.
   Northern Australian Region:
      Near predicted monthly values during local day.
      Enhanced by 25% during local night.
   Southern Australian Region:
      Near predicted monthly values during local day.
      Enhanced by 25% during local night.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day.

Monthly T index:
Month  T index
Sep      74
Oct      69
Nov      69

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
03 Oct    80    Near predicted monthly values
04 Oct    75    Near predicted monthly values to
05 Oct    75    Near predicted monthly values

COMMENT: Maximum usable frequencies (MUFs) on UT day 02-Oct were 
mostly near predicted monthly values to 25% enhanced during local 
night hours. Sporadic-E was observed briefly at northern sites 
during local night hours. MUFs are expected to be near 15% enhanced 
on 03-Oct, becoming near predicted monthly values by local night. 
Degraded local night conditions with possible mild depressions 
after local dawn may be experienced for southern Australian regions 
over 03-05 Oct, in association with an anticipated increase in 
geomagnetic activity. The degree of ionospheric depression is 
difficult to estimate due to the current enhanced ionospheric 
conditions.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 01 Oct
       Daily Proton Fluence >1 MeV:   3.1E+05
       Daily Proton Fluence >10 MeV:  3.1E+04
       Daily Electron Fluence >2 MeV: 1.50E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C1.5

DSCOVR Satellite Solar Wind Day Averaged Data for 01 Oct
Speed: 429 km/sec  Density:    0.6 p/cc  Temp:   144000 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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