[Ips-dsgr] ASWFC Daily Report - 14 October 23 issued 2330 UT on 14 Oct 2023 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Sun Oct 15 10:30:10 EST 2023


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/14 OCTOBER 2023
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 14 OCTOBER AND FORECAST FOR 15 OCTOBER - 17 OCTOBER
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 14 Oct:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 14 Oct: 148/102


1B. SOLAR FORECAST
             15 Oct             16 Oct             17 Oct
Activity     R0, chance of R1   R0, chance of R1   R0, chance of R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   145/99             145/99             140/94

COMMENT: Solar activity on UT day 14-Oct was at the R0 level, 
with two strong C-class flares, a C9.8 at 14/0516UT and an C3.5 
at 14/1632UT. There are currently seven numbered sunspot regions 
visible on the solar disk. AR3463 (S17W04, beta), AR3465 (N10E31, 
beta) and AR3466 (N08W34, beta) all exhibited development of 
trailer spots. AR3460 (S11W56, beta) was responsible for the 
largest flare of the day, but showed decay in its trailer spots. 
Newly arrived region AR3467 (N14E68, beta) produced the C3.5 
flare at 14/1632UT and is still too close to the eastern limb 
to be completely confident of its beta magnetic characteristics. 
There are no significantly magnetically complex sunspot regions 
currently visible on the solar disk. All other sunspot regions 
are either stable or in decay. Solar activity is expected to 
be at the R0 level over 15-17 Oct, with a chance of R1. Several 
CMEs were observed, but none are considered geoeffective. A wide 
north-northwest directed CME is visible in SOHO and STEREO-A 
imagery from 14/0500UT. This may be associated with a filament 
lift off visible in SDO and GOES SUVI imagery from 14/0339UT, 
although H-Alpha imagery shows that the filament involved in 
the lift off is very small and only a portion disappeared from 
the surface. Modelling indicates this CME is not geoeffective. 
A northwest directed, faint, slow CME is visible in SOHO imagery 
from 14/1412UT. This may be associated with an on disk eruption 
visible at around N18W30 from 14/1325UT in SDO, GOES SUVI and 
H-Alpha imagery. Modelling indicates this CME has no geoeffective 
component, however confidence is low due to no STEREO-A imagery. 
The solar wind speed on UT day 13-Oct decreased, ranging from 
548 to 456 km/s and is currently near 470 km/s. The peak total 
interplanetary field strength (IMF, Bt) was 6 nT and the north-south 
IMF component (Bz) range was +4 to -2 nT. The solar wind is expected 
to remain moderately elevated over 15-Oct, with a declining trend 
due to ongoing coronal hole high speed wind stream effects. The 
solar wind speed is expected to be mostly at background speeds 
over 16-17 Oct until an increase on 17-Oct due to high speed 
wind stream effects from a narrow coronal hole, currently rotating 
towards a geoeffective position.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 14 Oct: G0

Estimated Indices 14 Oct : A   K           
   Australian Region       6   22121131
      Cocos Island         4   12111030
      Darwin               4   22111121
      Townsville           6   22121131
      Learmonth            6   22221131
      Alice Springs        4   22111021
      Gingin               6   22221131
      Canberra             3   12120021
      Hobart               5   12221121    

Estimated Antarctic Regional K Indices 14 Oct :
      Macquarie Island     4   12130020
      Casey               13   34422132
      Mawson              22   24332164

Observed Regional daily pc3 Indices 14 Oct : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               6   (Quiet)
      Canberra             6   (Quiet)
      Hobart               6   (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 14 Oct : A 
           Fredericksburg         8
           Planetary              9                         

Observed AFr/Ap Indices 13 Oct :  A   K
           Fredericksburg        11
           Planetary             12   1232 3432     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
15 Oct     7    G0
16 Oct     5    G0
17 Oct    10    G0, chance of G1

COMMENT: G0 geomagnetic conditions were observed in the Australian 
region on UT day 14-Oct. Mostly G0 conditions were observed in 
the Antarctic region, with an isolated period of G2 at Mawson. 
G0 geomagnetic conditions are expected over 15-17 Oct, with a 
chance of G1 conditions on 17-Oct, due to anticipated coronal 
hole high speed wind stream effects.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
15 Oct      Normal         Normal         Normal
16 Oct      Normal         Normal         Normal
17 Oct      Normal         Normal         Normal-fair

COMMENT: HF radio propagation conditions were mostly normal on 
14-Oct. Normal HF propagation conditions are expected over 15-17 
Oct. Isolated minor shortwave fadeouts are possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
14 Oct   124

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 15% during local day.
      Enhanced by 40% during local night.
   Niue Island Region:
      Enhanced by 15% during local day.
      Enhanced by 15% during local night.
   Northern Australian Region:
      Near predicted monthly values during local day.
      Enhanced by 15% during local night.
   Southern Australian Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Davis/Mawson):
      Near predicted monthly values over the UT day.

Monthly T index:
Month  T index
Sep      104
Oct      98
Nov      96

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
15 Oct   135    Near to 15% above predicted monthly values
16 Oct   135    Near to 15% above predicted monthly values
17 Oct   130    Near to 15% above predicted monthly values

COMMENT: Maximum usable frequencies (MUFs) on UT day 14-Oct were 
near predicted monthly values in the Australian region, with 
enhancements of up to 15% observed in the northern Australian 
region during local night. Mild Spread F was observed at Hobart 
during local night. MUFs are expected to be near predicted monthly 
values to 15% enhanced over 15-17 Oct. Isolated minor shortwave 
fadeouts are possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 13 Oct
       Daily Proton Fluence >1 MeV:   4.2E+05
       Daily Proton Fluence >10 MeV:  1.9E+04
       Daily Electron Fluence >2 MeV: 2.20E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B8.1

DSCOVR Satellite Solar Wind Day Averaged Data for 13 Oct
Speed: 372 km/sec  Density:    1.9 p/cc  Temp:    89800 K  Bz:   5 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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