[Ips-dsgr] ASWFC Daily Report - 20 January 23 issued 2331 UT on 20 Jan 2023 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Sat Jan 21 10:31:20 EST 2023


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/20 JANUARY 2023
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 20 JANUARY AND FORECAST FOR 21 JANUARY - 23 JANUARY
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 20 Jan:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 20 Jan: 218/168


1B. SOLAR FORECAST
             21 Jan             22 Jan             23 Jan
Activity     R1                 R1                 R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   215/165            210/161            210/161

COMMENT: Solar activity on UT day 20-Jan was at the R0 level 
with several C-class flares produced. The largest flare, with 
magnitude of C7.4 at 20/2240UT, was produced by AR3192 (N18W14, 
beta-gamma), the next three largest flares C6.7 at 20/0152UT, 
C4.8 at 20/1257UT, C5.3 at 20/1407UT were all produced by AR3190 
(S16W15, beta-gamma). A slight rise was observed in the greater 
than 10 MeV proton flux. This is likely due to a farside event. 
There are currently eleven numbered sunspot regions visible on 
the solar disk and three unnumbered regions. AR3190, AR3194 (S24W30, 
beta), AR3196 (N12E17, beta), AR3197 (N24E45, beta), AR3198 (N27E57, 
beta) and AR3199 (N17E60, beta) all displayed spot development 
over the UT day. AR3190 remains the largest sunspot region, and 
the most magnetically complex alongside AR3192. All other sunspot 
regions are either stable or in decay. Despite no M-class flares 
over 20-Jan, Solar activity is expected to be at the R1 level 
over 21-23 Jan, due to the presence of AR3190 and several newly 
arrived, developing, sunspot regions. A southwest CME was observed 
in LASCO and STEREO-A imagery from 20/1336UT. This CME is associated 
with a large filament eruption, visible in SDO, H-alpha and GOES 
SUVI imagery from 20/1209UT between S48W21 and S24W60. Another 
CME was observed in LASCO and STEREO-A imagery from 20/1556UT. 
This CME is associated with a C5.3 magnitude flare produced at 
20/1407UT from AR3190. Modelling of these CMEs indicates that 
a glancing impact with Earth is possible on 24-Jan at 0100UT 
+/- 12 hours. The solar wind speed on UT day 20-Jan declined, 
ranging from 556 to 373 km/s, and is currently near 390 km/s. 
The peak total interplanetary field strength (IMF, Bt) was 10 
nT, and the north-south IMF component (Bz) range was +7 to -7 
nT. A period of sustained southward IMF conditions was observed 
from 20/1309UT to 20/1416UT. The solar wind speed is expected 
to remain low to moderate over 21-22 Jan, with an increase expected 
on 23-Jan due to the combined effects of a possible glancing 
blow from a CME first observed on 19-Jan and high speed wind 
stream effects from an equatorial coronal hole, which is rotating 
towards a geoeffective position.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 20 Jan: Quiet

Estimated Indices 20 Jan : A   K           
   Australian Region       4   12011212
      Cocos Island         3   11111211
      Darwin               4   22111112
      Townsville           -   --------
      Learmonth            4   12012212
      Alice Springs        4   12011212
      Gingin               3   11011212
      Canberra             3   11011212
      Hobart               5   22111212    

Estimated Antarctic Regional K Indices 20 Jan :
      Macquarie Island     6   11022411
      Casey               18   55322222
      Mawson              16   43123424

Observed Regional daily pc3 Indices 20 Jan : 
      Darwin               0   (Quiet)
      Townsville          NA
      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 20 Jan : A 
           Fredericksburg         8
           Planetary             11                         

Observed AFr/Ap Indices 19 Jan :  A   K
           Fredericksburg         6
           Planetary              6   1122 3111     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
21 Jan    12    G0
22 Jan     8    G0
23 Jan    12    G0, slight chance of G1

COMMENT: G0 geomagnetic conditions were observed in the Australian 
region on UT day 20-Jan. Mostly G0 geomagnetic conditions were 
observed in the Antarctic region, with periods of G1 observed 
at Casey. G0 geomagnetic conditions are expected over 21-22 Jan, 
there is a slight chance of G1 conditions on 23-Jan due to the 
combined effects of a possible glancing blow from a CME first 
observed on 19-Jan and high speed wind stream effects from an 
equatorial coronal hole, which is rotating towards a geoeffective 
position.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
20 Jan      Normal         Normal         Normal         

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
21 Jan      Normal         Normal         Normal-fair
22 Jan      Normal         Normal         Normal-fair
23 Jan      Normal         Normal         Normal-fair

COMMENT: Mostly normal HF conditions are expected over 21-23 
Jan, with a slight chance of disturbed conditions on 23-Jan due 
to possible geomagnetic activity. Shortwave fadeouts are possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
20 Jan   111

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 20% during local day.
      Enhanced by 25% during local night.
      Enhanced by 25% after local dawn.
   Niue Island Region:
      Near predicted monthly values during local day.
      Enhanced by 15% during local night.
   Northern Australian Region:
      Enhanced by 15% during local day.
      Near predicted monthly values during local night.
   Southern Australian Region:
      Near predicted monthly values during local day.
      Enhanced by 20% during local night.
      Enhanced by 20% after local dawn.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day.

Monthly T index:
Month  T index
Dec      84
Jan      71
Feb      72

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
21 Jan   120    Near to 15% above predicted monthly values
22 Jan   120    Near to 15% above predicted monthly values
23 Jan   120    Near to 15% above predicted monthly values

COMMENT: Maximum usable frequencies (MUFs) in the Australian 
region on UT day 20-Jan were near predicted monthly values to 
20% enhanced. Significant sporadic E was observed at Brisbane, 
Canberra and Cocos Islands during local night, with small amounts 
of sporadic E observed across the Australian region. MUFs are 
expected to be near predicted monthly values to 15% enhanced 
over 21-23 Jan, with a slight chance of depressed conditions 
on 23-Jan due to possible geomagnetic activity. Shortwave fadeouts 
are possible. Sporadic E is possible during local night, affecting 
lower frequencies.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 19 Jan
       Daily Proton Fluence >1 MeV:   3.4E+05
       Daily Proton Fluence >10 MeV:  2.4E+04
       Daily Electron Fluence >2 MeV: 2.70E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C1.8

DSCOVR Satellite Solar Wind Day Averaged Data for 19 Jan
Speed: 391 km/sec  Density:    3.0 p/cc  Temp:    67800 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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