The Relationship Between the Kinematics of Coronal Mass Ejections and the Brightness of the Corona

We present an investigation into an apparent relationship between white-light coronal brightness and the kinematics of flare-associated coronal mass ejections (CMEs). Using a unique data set, known as the Large Angle and Spectrometric Coronagraph Coronal Brightness Index (CBI), we conduct a study th...

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Main Authors: Kelly Victor-French, Karl Battams, Brian E. Wood
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/add3fb
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author Kelly Victor-French
Karl Battams
Brian E. Wood
author_facet Kelly Victor-French
Karl Battams
Brian E. Wood
author_sort Kelly Victor-French
collection DOAJ
description We present an investigation into an apparent relationship between white-light coronal brightness and the kinematics of flare-associated coronal mass ejections (CMEs). Using a unique data set, known as the Large Angle and Spectrometric Coronagraph Coronal Brightness Index (CBI), we conduct a study that explores the brightness in the lower solar corona and its relationship to the velocity of flare-associated CMEs. We analyze all M- and X-class flares that took place on or near the limbs of the Earth-facing disk of the Sun between 1996 and 2022, determine if these flares are associated with CMEs, and record the projection-corrected velocity of the eruptions if they occurred. Using the CBI data set, we evaluate the brightness in the corona directly overlying the flare source locations between 2.4 and 6.2 solar radii, and we find that above a certain level of coronal brightness, the likelihood of a high-velocity CME significantly decreases. This result implies that coronal brightness could be an important indicator of the kinematics of solar CMEs. We also highlight and discuss the unique nature of active region 12192 in 2014, observing that its unprecedented overlying coronal brightness may be related to the low CME productivity of that region.
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spelling doaj-art-e6f63acbe9dd4dd5bd52fa046bf511442025-08-20T03:15:35ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-01987213010.3847/1538-4357/add3fbThe Relationship Between the Kinematics of Coronal Mass Ejections and the Brightness of the CoronaKelly Victor-French0https://orcid.org/0000-0003-4070-5518Karl Battams1https://orcid.org/0000-0002-8692-6925Brian E. Wood2https://orcid.org/0000-0002-4998-0893U.S. Naval Research Laboratory , 4555 Overlook Ave SW, Washington, DC 20375, USA ; kelly.d.victor-french.civ@us.navy.milU.S. Naval Research Laboratory , 4555 Overlook Ave SW, Washington, DC 20375, USA ; kelly.d.victor-french.civ@us.navy.milU.S. Naval Research Laboratory , 4555 Overlook Ave SW, Washington, DC 20375, USA ; kelly.d.victor-french.civ@us.navy.milWe present an investigation into an apparent relationship between white-light coronal brightness and the kinematics of flare-associated coronal mass ejections (CMEs). Using a unique data set, known as the Large Angle and Spectrometric Coronagraph Coronal Brightness Index (CBI), we conduct a study that explores the brightness in the lower solar corona and its relationship to the velocity of flare-associated CMEs. We analyze all M- and X-class flares that took place on or near the limbs of the Earth-facing disk of the Sun between 1996 and 2022, determine if these flares are associated with CMEs, and record the projection-corrected velocity of the eruptions if they occurred. Using the CBI data set, we evaluate the brightness in the corona directly overlying the flare source locations between 2.4 and 6.2 solar radii, and we find that above a certain level of coronal brightness, the likelihood of a high-velocity CME significantly decreases. This result implies that coronal brightness could be an important indicator of the kinematics of solar CMEs. We also highlight and discuss the unique nature of active region 12192 in 2014, observing that its unprecedented overlying coronal brightness may be related to the low CME productivity of that region.https://doi.org/10.3847/1538-4357/add3fbSolar flaresSolar coronal mass ejectionsSolar active regionsSolar corona
spellingShingle Kelly Victor-French
Karl Battams
Brian E. Wood
The Relationship Between the Kinematics of Coronal Mass Ejections and the Brightness of the Corona
The Astrophysical Journal
Solar flares
Solar coronal mass ejections
Solar active regions
Solar corona
title The Relationship Between the Kinematics of Coronal Mass Ejections and the Brightness of the Corona
title_full The Relationship Between the Kinematics of Coronal Mass Ejections and the Brightness of the Corona
title_fullStr The Relationship Between the Kinematics of Coronal Mass Ejections and the Brightness of the Corona
title_full_unstemmed The Relationship Between the Kinematics of Coronal Mass Ejections and the Brightness of the Corona
title_short The Relationship Between the Kinematics of Coronal Mass Ejections and the Brightness of the Corona
title_sort relationship between the kinematics of coronal mass ejections and the brightness of the corona
topic Solar flares
Solar coronal mass ejections
Solar active regions
Solar corona
url https://doi.org/10.3847/1538-4357/add3fb
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