[Ips-dsgr] ASWFC Daily Report - 19 March 23 issued 2330 UT on 19 Mar 2023 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Mon Mar 20 10:30:54 EST 2023


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/19 MARCH 2023
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 19 MARCH AND FORECAST FOR 20 MARCH - 22 MARCH
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 19 Mar:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 19 Mar: 143/97


1B. SOLAR FORECAST
             20 Mar             21 Mar             22 Mar
Activity     R0,chance R1       R0,chance R1       R0, chance R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   143/97             140/94             140/94

COMMENT: Solar activity on UT day 19-Mar was at the R0 level. 
Solar regions AR3256(S22E63, beta) and AR3257(S27E70, beta) both 
produced minor C class flares. AR3256 showed very minor spot 
development, other regions were mostly stable. A new region AR3260(N25E77, 
alpha) has rotated onto the disk but is not very magnetically 
complex. There are currently 6 numbered solar regions on the 
disk. No new Earth directed CMEs were observed. A non Earth directed 
southward CME was observed in LASCO C2 from 19/1058UT in association 
with south polar limb/behind the limb activity. GOES 10MeV solar 
proton flux gradually became very slightly enhanced during the 
UT day and is currently at around 1.2PFU, far below the S1 threshold. 
Solar activity is expected to be R0, with the chance of an isolated 
low level R1 flare. The solar wind speed on UT day 19-Mar was 
steady, though noisy and ranged from 410 to 460 km/s, and is 
currently near 430 km/s. The peak total interplanetary field 
strength (IMF, Bt) was 7 nT and the north-south IMF component 
(Bz) range was +5 to -5 nT. The anticipated arrival of a glancing 
blow from a filament eruption/CME on 17-Mar did not eventuate, 
with the ACE EPAM precursor data remaining flat over the past 
24 hours, and it is likely the CME has passed under the Earth. 
A large coronal hole is visible in the south east solar quadrant.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 19 Mar: G0

Estimated Indices 19 Mar : A   K           
   Australian Region       6   22211222
      Cocos Island         4   12211121
      Darwin               6   22212222
      Townsville           6   22212222
      Learmonth            6   22212221
      Alice Springs        6   22211222
      Gingin               6   22201231
      Canberra             4   12201221
      Hobart               5   12201222    

Estimated Antarctic Regional K Indices 19 Mar :
      Macquarie Island     4   12211211
      Casey               11   33322232
      Mawson              24   24422364

Observed Regional daily pc3 Indices 19 Mar : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             2   (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 19 Mar : A 
           Fredericksburg         9
           Planetary             10                         

Observed AFr/Ap Indices 18 Mar :  A   K
           Fredericksburg         6
           Planetary             10   2213 3331     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
20 Mar    10    G0
21 Mar     8    G0
22 Mar     8    G0

COMMENT: ASWFC Geomagnetic Warning 12 was issued on 18 March 
and is current for 19-20 Mar. G0 geomagnetic conditions were 
observed in the Australian region UT day 19-Mar. G0 conditions 
generally observed in the Antarctic region, with an isolated 
period of G2 observed at Mawson. The anticipated increase in 
geomagnetic activity due to a recent solar filament eruption/CME 
has failed to eventuate and it is likely that the CME has passed 
under the Earth.

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

PCA Event : No event.

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

COMMENT: HF propagation conditions on 19-Mar were normal. The 
expected increase in geomagnetic activity due to a recent solar 
filament eruption/CME did not eventuate and HF conditions are 
now expected to remain normal.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
19 Mar   146

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 35-80%.
   Niue Island Region:
      Enhanced by 20-35%.
   Northern Australian Region:
      Enhanced by 20-45%.
   Southern Australian Region:
      Enhanced by 25-40%.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Enhanced by 15% over the UT day.

Monthly T index:
Month  T index
Feb      117
Mar      80
Apr      80

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
20 Mar   130    15 to 30% above predicted monthly values
21 Mar   130    15 to 30% above predicted monthly values
22 Mar   130    15 to 30% above predicted monthly values

COMMENT: ASWFC Preliminary HF Communications Warning 30 was issued 
on 18 March and is current for 20 Mar only. Maximum usable frequencies 
(MUFs) on UT day 19-Mar in the Australian region were enhanced 
by 20-80%. MUFs are expected to be enhanced by 15-30%. Degraded 
HF communication conditions are now not expected as the anticipated 
increase in geomagnetic activity has failed to eventuate. Isolated 
minor fadeouts possible. Ionospheric scintillation was observed 
at Weipa during the interval 19/1256-1320UT.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 18 Mar
       Daily Proton Fluence >1 MeV:   5.9E+05
       Daily Proton Fluence >10 MeV:  5.1E+04
       Daily Electron Fluence >2 MeV: 2.90E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B8.7

DSCOVR Satellite Solar Wind Day Averaged Data for 18 Mar
Speed: 424 km/sec  Density:    4.4 p/cc  Temp:   104000 K  Bz:   1 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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