[Ips-dsgr] ASWFC Daily Report - 26 March 23 issued 2330 UT on 26 Mar 2023 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Mon Mar 27 10:30:56 EST 2023


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/26 MARCH 2023
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 26 MARCH AND FORECAST FOR 27 MARCH - 29 MARCH
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 26 Mar:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 26 Mar: 159/113


1B. SOLAR FORECAST
             27 Mar             28 Mar             29 Mar
Activity     R0                 R0                 R0
Fadeouts     None expected      None expected      None expected
10.7cm/SSN   160/114            155/109            145/99

COMMENT: Solar activity on UT day 26-Mar was at the R0 level, 
with low level C-class flaring only. There are currently nine 
numbered sunspot regions visible on the solar disk. AR3256 (S23W35, 
gamma) is the most magnetically complex region and is stable. 
AR3263 (N17W24, beta) has exhibited spot development over the 
24-hour period. AR3265 (N21W05, beta) has shown some minor growth 
over the UT day. All other sunspot regions are either stable 
or in decay. The background level of X-ray flux remains at high 
B-class levels. Despite the large number of sunspot regions, 
most are magnetically simple and unremarkable. Solar activity 
is expected to be at the R0 level over 27-29 Mar. Several CMEs 
were observed, but none are considered geoeffective. The solar 
wind speed on UT day 26-Mar increased, ranging from 550 to 680 
km/s, and is currently near 575 km/s. The peak total interplanetary 
field strength (IMF, Bt) was 8 nT and the north-south IMF component 
(Bz) range was +4 to -5 nT. The solar wind speed is expected 
to remain elevated over 27-29 Mar due to ongoing 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 26 Mar: G0

Estimated Indices 26 Mar : A   K           
   Australian Region       6   23210122
      Cocos Island         3   22100112
      Darwin               5   23210022
      Townsville           6   23210122
      Learmonth            6   32210032
      Alice Springs        5   23210022
      Gingin               7   32200033
      Canberra             4   22200122
      Hobart               5   23200122    

Estimated Antarctic Regional K Indices 26 Mar :
      Macquarie Island     3   12101022
      Casey               15   34422233
      Mawson              23   54411254

Observed Regional daily pc3 Indices 26 Mar : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             0   (Quiet)
      Hobart               2   (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 26 Mar : A 
           Fredericksburg         8
           Planetary              9                         

Observed AFr/Ap Indices 25 Mar :  A   K
           Fredericksburg        12
           Planetary             12   2233 3232     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
27 Mar    14    G0, chance G1
28 Mar     8    G0
29 Mar     8    G0

COMMENT: G0 geomagnetic conditions were observed in the Australian 
region on UT day 26-Mar. Mostly G0 geomagnetic conditions were 
observed in the Antarctic region, with two isolated periods of 
G1 observed at Mawson. G0 geomagnetic conditions are expected 
on 27-Mar, with a chance of G1 due to ongoing coronal hole high 
speed wind stream effects from a broad southern hemisphere coronal 
hole. G0 geomagnetic conditions are expected over 28-29 Mar.

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

PCA Event : No event.

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

COMMENT: Normal HF propagation conditions were observed on 26-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 on 27-Mar. Middle to low latitude HF conditions are 
expected to remain normal. Normal HF propagation conditions are 
expected over 28-29 Mar.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
26 Mar   137

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 15% during local day.
      Enhanced by 55% during local night.
   Niue Island Region:
      Enhanced by 50% during local day.
      Enhanced by 110% during local night.
   Northern Australian Region:
      Enhanced by 30% during local day.
      Enhanced by 40-45% during local night and after local dawn.
   Southern Australian Region:
      Enhanced by 20% during local day.
      Near predicted monthly values during local night.
      Enhanced by 30% 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
27 Mar   135    Near to 20% above predicted monthly values
28 Mar   135    Near to 20% above predicted monthly values
29 Mar   135    Near to 20% above predicted monthly values

COMMENT: Maximum usable frequencies (MUFs) on UT day 26-Mar in 
the Australian region were enhanced by 30-45% in Northern Australia 
and 20% enhanced in Southern Australia during local day. Sporadic 
E was observed at Brisbane. Degraded HF conditions during local 
night hours are possible for southern Australia over 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 27-29 Mar.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 25 Mar
       Daily Proton Fluence >1 MeV:   2.8E+05
       Daily Proton Fluence >10 MeV:  2.2E+04
       Daily Electron Fluence >2 MeV: 2.30E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 4%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B7.0

DSCOVR Satellite Solar Wind Day Averaged Data for 25 Mar
Speed: 515 km/sec  Density:    8.4 p/cc  Temp:   247000 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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