Detecting Stellar Coronal Mass Ejections via Coronal Dimming in the Extreme Ultraviolet Article Swipe
James Mason
,
Allison Youngblood
,
Kevin France
,
Astrid Veronig
,
Meng Jin
·
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/ade4bc
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/ade4bc
Stellar flares and coronal mass ejections (CMEs) can strip planetary atmospheres, reducing the potential habitability of terrestrial planets. While flares have been observed for decades, stellar CMEs remain elusive. Extreme-ultraviolet (EUV) emissions are sensitive to both flares and CME-induced coronal dimming. We assess the detectability of stellar CME-induced EUV dimming events by adapting a known “Sun-as-a-star” dimming technique—validated by the Solar Dynamics Observatory’s EUV Variability Experiment (EVE)—to stellar conditions. We adapt the solar data to reflect a range of stellar intensities, accounting for intrinsic brightness, distance, and interstellar medium (ISM) attenuation. We generate synthetic light curves for two different missions: the legacy EUV Explorer (EUVE) and the proposed ESCAPE mission. Our results indicate that dimming detections are well within reach. EUVE’s broadband imager was capable of detecting stellar CMEs—albeit with limited spectral (temperature) resolution—but that was not part of the observing plan. EUVE’s spectroscopic survey lacked sufficient sensitivity for CME detections. Optimizing modern instrument design for this task would make the observation fully feasible. In this work, we present a tool to explore the stellar-CME detection parameter space. Our tool shows that with an instrument with performance similar to ESCAPE, setting a 600 s integration period, and integrating the spectra into bands, any star with a X-ray flux ≥2.51 × 10 −12 erg s −1 cm −2 should have a ≥3 σ detection even for a modest few-percent dimming profile, regardless of ISM attenuation. Such measurements would be crucial for understanding the space weather environments of exoplanet host stars and, ultimately, for evaluating planetary habitability.
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Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4357/ade4bc
- OA Status
- gold
- Cited By
- 2
- References
- 91
- Related Works
- 10
- OpenAlex ID
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All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4412557397Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-4357/ade4bcDigital Object Identifier
- Title
-
Detecting Stellar Coronal Mass Ejections via Coronal Dimming in the Extreme UltravioletWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
-
2025Year of publication
- Publication date
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2025-07-22Full publication date if available
- Authors
-
James Mason, Allison Youngblood, Kevin France, Astrid Veronig, Meng JinList of authors in order
- Landing page
-
https://doi.org/10.3847/1538-4357/ade4bcPublisher landing page
- Open access
-
YesWhether a free full text is available
- OA status
-
goldOpen access status per OpenAlex
- OA URL
-
https://doi.org/10.3847/1538-4357/ade4bcDirect OA link when available
- Concepts
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Physics, Coronal mass ejection, Extreme ultraviolet, Astrophysics, Astronomy, Ultraviolet, Coronal plane, Corona (planetary geology), Solar flare, Solar wind, Plasma, Astrobiology, Optics, Medicine, Nuclear physics, Venus, Radiology, LaserTop concepts (fields/topics) attached by OpenAlex
- Cited by
-
2Total citation count in OpenAlex
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2025: 2Per-year citation counts (last 5 years)
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91Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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| referenced_works_count | 91 |
| abstract_inverted_index.a | 54, 77, 170, 192, 206, 220, 226 |
| abstract_inverted_index.s | 194, 214 |
| abstract_inverted_index.10 | 211 |
| abstract_inverted_index.In | 165 |
| abstract_inverted_index.We | 42, 70, 92 |
| abstract_inverted_index.an | 184 |
| abstract_inverted_index.be | 238 |
| abstract_inverted_index.by | 52, 59 |
| abstract_inverted_index.cm | 216 |
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| abstract_inverted_index.to | 35, 75, 172, 189 |
| abstract_inverted_index.we | 168 |
| abstract_inverted_index.× | 210 |
| abstract_inverted_index.σ | 222 |
| abstract_inverted_index.600 | 193 |
| abstract_inverted_index.CME | 150 |
| abstract_inverted_index.EUV | 49, 64, 103 |
| abstract_inverted_index.ISM | 233 |
| abstract_inverted_index.Our | 111, 179 |
| abstract_inverted_index.and | 3, 38, 87, 106, 197 |
| abstract_inverted_index.any | 203 |
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| abstract_inverted_index.was | 124, 136 |
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| abstract_inverted_index.Such | 235 |
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| abstract_inverted_index.both | 36 |
| abstract_inverted_index.data | 74 |
| abstract_inverted_index.even | 224 |
| abstract_inverted_index.flux | 208 |
| abstract_inverted_index.have | 21, 219 |
| abstract_inverted_index.host | 248 |
| abstract_inverted_index.into | 201 |
| abstract_inverted_index.make | 160 |
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| abstract_inverted_index.star | 204 |
| abstract_inverted_index.task | 158 |
| abstract_inverted_index.that | 114, 135, 182 |
| abstract_inverted_index.this | 157, 166 |
| abstract_inverted_index.tool | 171, 180 |
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| abstract_inverted_index.with | 130, 183, 186, 205 |
| abstract_inverted_index.−1 | 215 |
| abstract_inverted_index.−2 | 217 |
| abstract_inverted_index.≥3 | 221 |
| abstract_inverted_index.(EUV) | 31 |
| abstract_inverted_index.(ISM) | 90 |
| abstract_inverted_index.Solar | 61 |
| abstract_inverted_index.While | 19 |
| abstract_inverted_index.X-ray | 207 |
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| abstract_inverted_index.fully | 163 |
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| abstract_inverted_index.range | 78 |
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| abstract_inverted_index.space | 243 |
| abstract_inverted_index.stars | 249 |
| abstract_inverted_index.strip | 9 |
| abstract_inverted_index.work, | 167 |
| abstract_inverted_index.would | 159, 237 |
| abstract_inverted_index.−12 | 212 |
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| abstract_inverted_index.(EUVE) | 105 |
| abstract_inverted_index.ESCAPE | 109 |
| abstract_inverted_index.assess | 43 |
| abstract_inverted_index.bands, | 202 |
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| abstract_inverted_index.flares | 2, 20, 37 |
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| abstract_inverted_index.legacy | 102 |
| abstract_inverted_index.medium | 89 |
| abstract_inverted_index.modern | 153 |
| abstract_inverted_index.modest | 227 |
| abstract_inverted_index.reach. | 120 |
| abstract_inverted_index.remain | 28 |
| abstract_inverted_index.should | 218 |
| abstract_inverted_index.space. | 178 |
| abstract_inverted_index.survey | 145 |
| abstract_inverted_index.within | 119 |
| abstract_inverted_index.ESCAPE, | 190 |
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| abstract_inverted_index.coronal | 4, 40 |
| abstract_inverted_index.crucial | 239 |
| abstract_inverted_index.dimming | 50, 57, 115, 229 |
| abstract_inverted_index.explore | 173 |
| abstract_inverted_index.limited | 131 |
| abstract_inverted_index.period, | 196 |
| abstract_inverted_index.present | 169 |
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| abstract_inverted_index.results | 112 |
| abstract_inverted_index.setting | 191 |
| abstract_inverted_index.similar | 188 |
| abstract_inverted_index.spectra | 200 |
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| abstract_inverted_index.weather | 244 |
| abstract_inverted_index.≥2.51 | 209 |
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| abstract_inverted_index.Explorer | 104 |
| abstract_inverted_index.adapting | 53 |
| abstract_inverted_index.decades, | 25 |
| abstract_inverted_index.dimming. | 41 |
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| abstract_inverted_index.feasible. | 164 |
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| abstract_inverted_index.parameter | 177 |
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| abstract_inverted_index.accounting | 82 |
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| abstract_inverted_index.regardless | 231 |
| abstract_inverted_index.sufficient | 147 |
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| abstract_inverted_index.brightness, | 85 |
| abstract_inverted_index.conditions. | 69 |
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