Coronal Dimming Diagnostics for Stellar CMEs: Contrasting CMEs and Confined Flares

Candidate events on stars, supported by clear events on the Sun, suggest “coronal dimming” signals may be a powerful way to study coronal mass ejections (CMEs) across a range of stars. However, magnetically confined events can also produce signals that resemble CME-induced dimming, complicating identification. Here, we present modeling and observational analysis of both confined and eruptive events on the Sun to quantitatively compare dimming morphology and evolution. We show that eruptive events preferentially produce deeper, longer-lived, and more spatially extended dimmings, whereas confined flares tend to yield weaker, shorter-lived, and more localized signatures. Using the newly developed SPECTRUM code, we synthesize EUV/UV spectra to identify features that distinguish eruptive from confined cases. We then extend these results to stellar scenarios, identifying challenges and recommending solutions for using coronal dimming to detect stellar CMEs. With insights from models validated with detailed solar observations, we argue that it is possible to use coronal dimming as a reliable indicator of stellar CMEs.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-08-21
DOI
https://doi.org/10.5281/zenodo.22049060
Primary Topic
Solar and Space Plasma Dynamics
Type
article
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article

Coronal Dimming Diagnostics for Stellar CMEs: Contrasting CMEs and Confined Flares

W. B. Manchester, R. O. Parke Loyd, James Mason, X. Liu et al.
Zenodo (CERN European Organization for Nuclear Research)
Solar and Space Plasma Dynamics
article

Coronal Dimming Diagnostics for Stellar CMEs: Contrasting CMEs and Confined Flares

W. B. Manchester, R. O. Parke Loyd, James Mason, X. Liu, Kevin France, Marc L. DeRosa, Mark C. M. Cheung, Tong Shi, Karin Dissauer, Meng Jin, Allison Youngblood, N. Nitta
article en

Abstract

Candidate events on stars, supported by clear events on the Sun, suggest “coronal dimming” signals may be a powerful way to study coronal mass ejections (CMEs) across a range of stars. However, magnetically confined events can also produce signals that resemble CME-induced dimming, complicating identification. Here, we present modeling and observational analysis of both confined and eruptive events on the Sun to quantitatively compare dimming morphology and evolution. We show that eruptive events preferentially produce deeper, longer-lived, and more spatially extended dimmings, whereas confined flares tend to yield weaker, shorter-lived, and more localized signatures. Using the newly developed SPECTRUM code, we synthesize EUV/UV spectra to identify features that distinguish eruptive from confined cases. We then extend these results to stellar scenarios, identifying challenges and recommending solutions for using coronal dimming to detect stellar CMEs. With insights from models validated with detailed solar observations, we argue that it is possible to use coronal dimming as a reliable indicator of stellar CMEs.

Zenodo (CERN European Organization for Nuclear Research)
Lockheed Martin (United States) (US), Commonwealth Scientific and Industrial Research Organisation (AU), Goddard Space Flight Center (US), University of Colorado Boulder (US), University of Michigan (US), University of Colorado System (US), Johns Hopkins University Applied Physics Laboratory (US), Health Sciences and Nutrition (AU), Lockheed Martin (Australia) (AU), Lockheed Martin (United Kingdom) (GB), Northwest Research Associates (US), Eureka Scientific (US), Search for Extraterrestrial Intelligence (US)
Openalex Percentile: Top 10%
Solar and Space Plasma Dynamics
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