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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 5.

SDO/AIA 211 Å running difference image showing the coronal dimming associated with the CME observed on 2024 August 5 at ≈13:28 UT from AR13767 (Section 2 of the main text). The white circle indicates the solar limb. Solar north is straight up and east is to the left. The red line indicates the location of slit 4 of VELC on the west limb. The center of the slit is at r = 1.17R. The numbers 225°–315° on the white circle correspond to the solar position angles.

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