Exploring the Relation Between Magnetic Fields, Starspots, and CMEs

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dc.contributor.authorMenezes F.
dc.contributor.authorValio A.
dc.contributor.authorNetto Y.
dc.contributor.authorAraujo A.
dc.contributor.authorKay C.
dc.contributor.authorOpher M.
dc.date.accessioned2025-04-01T06:38:22Z
dc.date.available2025-04-01T06:38:22Z
dc.date.issued2023
dc.description.abstract© The Author(s), 2024.Solar-type stars, including the Sun, have magnetic fields that extend from their interiors to the surface and beyond, influencing both the stellar activity and interplanetary medium. Magnetic activity phenomena, such as coronal mass ejections (CMEs), significantly impacts space weather. These CMEs, composed of plasma clouds with magnetic fields ejected from the stellar corona, pose a potential threat to planets by affecting their magnetosphere and atmosphere. Despite advancements in detecting stellar CMEs, detection remains limited. We focus on understanding CME propagation by analyzing key parameters like position, velocities, and the configuration of stellar magnetic fields. Using spot transit mapping, we reconstruct magnetograms for Kepler-63 and Kepler-411, employing the ForeCAT model to simulate CME trajectories from these stars. Results indicate that CME deflections generally decrease with radial velocity and increase with ejection latitude. Additionally, stars with stronger magnetic fields, such as Kepler-63, tend to cause more significant CME deflections.
dc.description.firstpage426
dc.description.issuenumberS365
dc.description.lastpage435
dc.description.volume19
dc.identifier.doi10.1017/S1743921324000267
dc.identifier.issnNone
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/40459
dc.relation.ispartofProceedings of the International Astronomical Union
dc.rightsAcesso Restrito
dc.subject.otherlanguagecoronal mass ejections (CMEs)
dc.subject.otherlanguageSolar-type stars
dc.subject.otherlanguageStarspots
dc.subject.otherlanguageStellar magnetic field
dc.titleExploring the Relation Between Magnetic Fields, Starspots, and CMEs
dc.typeArtigo de evento
local.scopus.citations0
local.scopus.eid2-s2.0-85217092455
local.scopus.updated2025-04-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85217092455&origin=inward
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