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

  • Authors: R. Ramesh, V. Muthu Priyal, Jagdev Singh, K. Sasikumar Raja, Wageesh Mishra, C. Monstein

R. Ramesh et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 1.

Schematic of the positions of the four straight slits in the VELC spectroscopy channel. The inner filled black circle corresponds to the occulter (radius = 1.05R⊙). The white circular patch indicates the FoV, i.e., 1.05–1.5R⊙. Solar north and east directions are straight up and to the left, respectively.

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