most citedCalibration of Spectropolarimetry channel of Visible Emission Line Coronagraph onboard Aditya-L1

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astro-ph.SR2026

Coordinated Coronagraphic Observations from Proba-3 and Aditya-L1: Investigating CME Energetics in the Inner Corona

Anjali Agarwal, Wageesh Mishra, R. Ramesh +16

Constraining the plasma properties and energetics of coronal mass ejections (CMEs) in the inner corona is essential for understanding their early evolution, yet remains challenging…

astro-ph.SR2026

Aditya-L1/VELC observations of CME associated broadening of 5303Å coronal emission line

K. Sasikumar Raja, V. Muthu Priyal, R. Ramesh +2

We present Aditya-L1/VELC spectroscopic observations of 5303Å coronal emission line widths before and after coronal mass ejections (CMEs) which showed coronal dimming. The sit \& s…

astro-ph.SR2024

New Results on the Onset of a Coronal Mass Ejection from 5303 Å Emission Line Observations with VELC/ADITYA-L1

R. Ramesh, V. Muthu Priyal, Jagdev Singh +3

We report on the onset of a coronal mass ejection (CME) using spectroscopic observations in 5303 Å coronal emission line with the Visible Emission Line Coronagraph (VELC) onboard A…

astro-ph.SR20242 cited

Calibration of Spectropolarimetry channel of Visible Emission Line Coronagraph onboard Aditya-L1

Venkata Suresh Narra, K. Sasikumar Raja, Raghavendra Prasad B +11

The magnetic field strength and its topology play an important role in understanding the formation, evolution, and dynamics of the solar corona. Also, it plays a significant role i…

astro-ph.SR2024

Equator to Pole Solar Chromospheric Differential Rotation using Ca-K Features Derived from Kodaikanal Data

Hema Kharayat, Jagdev Singh, Muthu Priyal +1

Differential rotation is one of the basic characteristics of the Sun, and it plays an important role in generating the magnetic fields and its activities. We investigated rotation…