[Ips-dsgr] ASWFC Daily Report - 25 March 23 issued 2331 UT on 25 Mar 2023 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Sun Mar 26 10:31:22 EST 2023


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/25 MARCH 2023
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 25 MARCH AND FORECAST FOR 26 MARCH - 28 MARCH
STATUS INDICATORS SOL:** YELLOW **   MAG:** YELLOW **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 25 Mar:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 25 Mar: 160/114


1B. SOLAR FORECAST
             26 Mar             27 Mar             28 Mar
Activity     R0, chance R1      R0, chance R1      R0, chance R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   165/119            160/114            155/109

COMMENT: Solar activity on UT day 25-Mar was at the R0 level, 
with no significant flaring activity. There are currently eight 
numbered sunspot regions visible on the solar disk and one unnumbered 
region. AR3258 (N20W46, beta) and AR3263 (N17W11, beta) have 
both shown growth in their trailer spots over the 24-hour period. 
An unnumbered region recently appeared at ~N20E12 and is stable. 
All other sunspot regions are either stable or in decay. The 
background X-ray flux is at high B-class levels. Solar activity 
is expected to be at the R0 level, with a chance of R1. A northwest 
CME was observed, visible in LASCO C2 coronagraph imagery from 
24/2212UT. Modelling indicates this CME is not geoeffective. 
No other Earth-directed CMEs have been observed. The solar wind 
speed on UT day 25-Mar increased, ranging from 460 to 550 km/s, 
and is currently near 550 km/s. The peak total interplanetary 
field strength (IMF, Bt) was 10 nT and the north-south IMF component 
(Bz) range was +8 to -8 nT. The solar wind speed is expected 
to remain elevated over 26-28 Mar due to coronal hole high speed 
wind stream effects from a broad southern hemisphere coronal 
hole.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 25 Mar: G0

Estimated Indices 25 Mar : A   K           
   Australian Region       9   22233222
      Cocos Island         7   22231221
      Darwin               7   22223122
      Townsville          10   22333222
      Learmonth           10   32233222
      Alice Springs        9   22233222
      Gingin              10   32223232
      Canberra             9   22333122
      Hobart              10   22333222    

Estimated Antarctic Regional K Indices 25 Mar :
      Macquarie Island    22   23455332
      Casey               22   45443233
      Mawson              30   43453355

Observed Regional daily pc3 Indices 25 Mar : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               4   (Quiet)
      Canberra            13   (Quiet)
      Hobart              26   (Quiet to unsettled)

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 25 Mar : A 
           Fredericksburg        16
           Planetary             21                         

Observed AFr/Ap Indices 24 Mar :  A   K
           Fredericksburg        40
           Planetary             72   6874 2344     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
26 Mar    18    G0-G1
27 Mar    16    G0, chance G1
28 Mar     8    G0

COMMENT: G0 geomagnetic conditions were observed in the Australian 
region on UT day 25-Mar. G0-G1 geomagnetic conditions were observed 
in the Antarctic region. G0-G1 geomagnetic conditions are expected 
on 26-Mar due to coronal hole high speed wind stream effects 
from a broad southern hemisphere coronal hole. G0 geomagnetic 
conditions are expected on 27-Mar, with a chance of G1. G0 geomagnetic 
conditions are expected on 28-Mar.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
25 Mar      Normal         Normal         Normal         

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
26 Mar      Normal         Normal-fair    Fair
27 Mar      Normal         Normal-fair    Fair
28 Mar      Normal         Normal         Normal-fair

COMMENT: Normal HF propagation conditions were observed on 25-Mar. 
An extended period of mildly degraded HF conditions for middle 
to high latitudes is possible due to a broad solar coronal hole 
wind stream over 26-27 Mar. Middle to low latitude HF conditions 
are expected to remain normal.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
25 Mar   139

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 35% during local day.
      Near predicted monthly values during local night.
      Enhanced by 20% after local dawn.
   Niue Island Region:
      Enhanced by 25% during local day.
      Enhanced by 35% during local night.
   Northern Australian Region:
      Enhanced by 35% during local day and after local dawn.
      Enhanced by 25% during local night.
   Southern Australian Region:
      Enhanced by 35% during local day.
      Near predicted monthly values 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
Feb      117
Mar      80
Apr      80

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
26 Mar   130    Near to 20% above predicted monthly values
27 Mar   130    Near to 20% above predicted monthly values
28 Mar   130    Near to 20% above predicted monthly values

COMMENT: Maximum usable frequencies (MUFs) on UT day 25-Mar in 
the Australian region were enhanced by 25-35% in Northern Australia 
and 35% enhanced in Southern Australia during local day. Spread 
F was observed at Hobart. Degraded HF conditions during local 
night hours are possible for southern Australia over 26-27 Mar 
due to a mild increase in geomagnetic activity from a broad solar 
coronal hole. MUFs are expected to be near predicted monthly 
values to 20% enhanced over 26-28 Mar.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 24 Mar
       Daily Proton Fluence >1 MeV:   1.4E+06
       Daily Proton Fluence >10 MeV:  2.1E+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: B6.8

DSCOVR Satellite Solar Wind Day Averaged Data for 24 Mar
Speed: 438 km/sec  Density:    9.9 p/cc  Temp:    93000 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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