Estimation of the Energy Involved in a Solar Coronal Mass Ejection Using Spectroscopic Observations in the 5303 Å Emission Line

While the amount of solar coronal energy flux leaving the “quiet” Sun, coronal holes, and active regions has been estimated by many, similar calculations for transients like coronal mass ejections (CMEs) based on observations are few. Using spectroscopic observations in the 5303 Å coronal emission l...

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Váldodahkkit:	R. Ramesh, V. Muthu Priyal, Jagdev Singh, K. Sasikumar Raja, Wageesh Mishra, C. Monstein
Materiálatiipa:	Artigo
Giella:	Inglês
Almmustuhtton:	IOP Publishing 2026-01-01
Ráidu:	The Astrophysical Journal Letters
Fáttát:	The Sun Solar corona Solar flares Solar coronal mass ejections Solar coronal heating
Liŋkkat:	https://doi.org/10.3847/2041-8213/ae7bf0
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