[Ips-dsgr] ASWFC Daily Report - 15 March 24 issued 2331 UT on 15 Mar 2024 [SEC=OFFICIAL]

rwc rwc at ips.gov.au
Sat Mar 16 10:32:00 EST 2024


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/15 MARCH 2024
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 15 MARCH AND FORECAST FOR 16 MARCH - 18 MARCH
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 15 Mar:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 15 Mar: 129/82


1B. SOLAR FORECAST
             16 Mar             17 Mar             18 Mar
Activity     R0                 R0                 R0                 
Fadeouts     None expected      None expected      None expected
10.7cm/SSN   130/84             130/84             135/89

COMMENT: Solar activity on UT day 15-Mar was at the R0 level, 
with a long duration C-class flare observed from around 15/0240UT 
to 15/0800UT, peaking at the C6 level. There are currently five 
numbered active regions visible on the solar disk. Recently rotated 
off region AR3599 (S13W94, unknown) was responsible for the long 
duration C6 flare. AR3607 (S17E08, beta) is the largest region 
visible on the solar disk, but it is small and magnetically simple 
and showed decay over the UT day. There are no magnetically complex 
regions currently visible on the solar disk. All other numbered 
regions are either stable or in decay. Solar activity is expected 
to be at the R0 level over 16-18 Mar. S1 conditions were observed 
from 15/2050UT, although the flux has since dropped below the 
S1 level. The source for the increase in proton flux is likely 
the long duration C6 flare off the western limb. S0-S1 conditions 
are expected on 16-Mar, S0 conditions are expected on 17-18 Mar. 
A large, west directed CME was observed from 15/0210UT in SOHO 
and STEREO-A imagery. This event is associated with the long 
duration C6 flare from 15/0240UT and the S1 solar radiation conditions. 
An eruption is visible in SDO, H-Alpha and GOES SUVI imagery 
off the western limb from 15/0144UT at around S20. Modelling 
indicates that the vast majority of the ejected material will 
pass ahead of Earth, however there is a chance of a glancing 
impact on 18-Mar at 0300UT +/- 12 hours. The solar wind speed 
on UT day 15-Mar was mostly stable, ranging from 371 to 481 km/s 
and is currently near 405 km/s. The peak total interplanetary 
field strength (IMF, Bt) was 6 nT and the north south IMF component 
(Bz) range was +5 to -5 nT. The solar wind speed is expected 
to remain steady on 16-Mar, a slight increase is possible from 
the second half of 17-Mar or the first half of 18-Mar due to 
a possible glancing impact from a CME first observed on 15-Mar.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 15 Mar: G0

Estimated Indices 15 Mar : A   K           
   Australian Region       3   21211101
      Darwin               4   22211101
      Townsville           4   22211101
      Learmonth            3   22111100
      Alice Springs        3   21111101
      Gingin               3   31111000
      Canberra             3   21211001
      Kennaook Cape Grim   3   21211100    

Estimated Antarctic Regional K Indices 15 Mar :
      Macquarie Island     3   22220000
      Casey               12   34422112
      Mawson              18   54432113

Observed Regional daily pc3 Indices 15 Mar : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth           NA
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             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 15 Mar : A 
           Fredericksburg         9
           Planetary             12                         

Observed AFr/Ap Indices 14 Mar :  A   K
           Fredericksburg         7
           Planetary              7   1212 2231     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
16 Mar     8    G0
17 Mar    10    G0, chance of G1
18 Mar    10    G0, chance of G1

COMMENT: G0 geomagnetic conditions were observed in the Australian 
region on UT day 15-Mar. Mostly G0 geomagnetic conditions were 
observed in the Antarctic region, with an isolated period of 
G1 observed at Mawson. G0 geomagnetic conditions are expected 
on 16-Mar. G0 conditions, with a chance of G1 are expected on 
17-18 Mar due to a possible glancing impact from a CME first 
observed on 15-Mar.

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

PCA Event : No event.

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

COMMENT: HF radio communication conditions on UT day 15-Mar were 
mostly normal. HF radio communication conditions are expected 
to be mostly normal over 16-18 Mar.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
15 Mar   115

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values.
   Niue Island Region:
      Near predicted monthly values.
   Northern Australian Region:
      Near predicted monthly values.
   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
Feb      138
Mar      111
Apr      112

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
16 Mar   115    Near predicted monthly values
17 Mar   115    Near predicted monthly values
18 Mar   115    Near predicted monthly values

COMMENT: Maximum usable frequencies (MUFs) in the Australian 
region on UT day 15-Mar were near predicted monthly values. Spread 
F was observed at Hobart during local night hours. MUFs are expected 
to be near predicted monthly values over 16-18 Mar.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 14 Mar
       Daily Proton Fluence >1 MeV:   9.6E+04
       Daily Proton Fluence >10 MeV:  1.8E+04
       Daily Electron Fluence >2 MeV: 3.80E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B8.0

DSCOVR Satellite Solar Wind Day Averaged Data for 14 Mar
Speed: 443 km/sec  Density:    5.4 p/cc  Temp:   181000 K  Bz:   2 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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