Detection and Characterization of a Coronal Mass Ejection Using Interplanetary Scintillation Measurements From the Murchison Widefield Array

Abstract We have shown previously that the Murchison Widefield Array (MWA), can detect 100s of Interplanetary Scintillation (IPS) sources simultaneously across a field of view (FoV) ∼30° in extent. To test if we can use this capability to track heliospheric structures, we undertook a search of 88 hr...

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Main Authors: J. Morgan, P. I. McCauley, A. Waszewski, R. Ekers, R. Chhetri
Format: Article
Language:English
Published: Wiley 2023-05-01
Series:Space Weather
Online Access:https://doi.org/10.1029/2022SW003396
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author J. Morgan
P. I. McCauley
A. Waszewski
R. Ekers
R. Chhetri
author_facet J. Morgan
P. I. McCauley
A. Waszewski
R. Ekers
R. Chhetri
author_sort J. Morgan
collection DOAJ
description Abstract We have shown previously that the Murchison Widefield Array (MWA), can detect 100s of Interplanetary Scintillation (IPS) sources simultaneously across a field of view (FoV) ∼30° in extent. To test if we can use this capability to track heliospheric structures, we undertook a search of 88 hr of MWA IPS data, and identified an observation likely to have a significant Coronal Mass Ejection (CME) in the FoV. We demonstrate that in a single 5‐min MWA observation we are able to localize and image a CME ∼33 hr after launch at an elongation of ∼37° from the Sun. We use IPS observables to constrain the kinematics of the CME, and describe how MWA IPS observations can be used in the future to make a unique contribution to heliospheric modeling efforts.
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institution Kabale University
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spelling doaj-art-ae0550397d0b450888fa09c2ecfa7b702025-01-14T16:26:43ZengWileySpace Weather1542-73902023-05-01215n/an/a10.1029/2022SW003396Detection and Characterization of a Coronal Mass Ejection Using Interplanetary Scintillation Measurements From the Murchison Widefield ArrayJ. Morgan0P. I. McCauley1A. Waszewski2R. Ekers3R. Chhetri4International Centre for Radio Astronomy Research Curtin University Bentley WA AustraliaSchool of Physics University of Sydney Sydney NSW AustraliaInternational Centre for Radio Astronomy Research Curtin University Bentley WA AustraliaInternational Centre for Radio Astronomy Research Curtin University Bentley WA AustraliaInternational Centre for Radio Astronomy Research Curtin University Bentley WA AustraliaAbstract We have shown previously that the Murchison Widefield Array (MWA), can detect 100s of Interplanetary Scintillation (IPS) sources simultaneously across a field of view (FoV) ∼30° in extent. To test if we can use this capability to track heliospheric structures, we undertook a search of 88 hr of MWA IPS data, and identified an observation likely to have a significant Coronal Mass Ejection (CME) in the FoV. We demonstrate that in a single 5‐min MWA observation we are able to localize and image a CME ∼33 hr after launch at an elongation of ∼37° from the Sun. We use IPS observables to constrain the kinematics of the CME, and describe how MWA IPS observations can be used in the future to make a unique contribution to heliospheric modeling efforts.https://doi.org/10.1029/2022SW003396
spellingShingle J. Morgan
P. I. McCauley
A. Waszewski
R. Ekers
R. Chhetri
Detection and Characterization of a Coronal Mass Ejection Using Interplanetary Scintillation Measurements From the Murchison Widefield Array
Space Weather
title Detection and Characterization of a Coronal Mass Ejection Using Interplanetary Scintillation Measurements From the Murchison Widefield Array
title_full Detection and Characterization of a Coronal Mass Ejection Using Interplanetary Scintillation Measurements From the Murchison Widefield Array
title_fullStr Detection and Characterization of a Coronal Mass Ejection Using Interplanetary Scintillation Measurements From the Murchison Widefield Array
title_full_unstemmed Detection and Characterization of a Coronal Mass Ejection Using Interplanetary Scintillation Measurements From the Murchison Widefield Array
title_short Detection and Characterization of a Coronal Mass Ejection Using Interplanetary Scintillation Measurements From the Murchison Widefield Array
title_sort detection and characterization of a coronal mass ejection using interplanetary scintillation measurements from the murchison widefield array
url https://doi.org/10.1029/2022SW003396
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