6–10 Sept 2021
Online
Europe/Rome timezone

Non-thermal parametric variations using Si IV and O IV spectral lines

8 Sept 2021, 12:05
13m
Online

Online

Poster Session 2 - The Solar Atmosphere: Heating, Dynamics and Coupling Poster Session 6.3

Speaker

Ms Yamini K Rao (DAMTP, University of Cambridge)

Description

We study the various regions of the Sun, using high-resolution spectral observations from the Interface Region Imaging Spectrograph (IRIS). We observe the Quiet-Sun observation targeting the same region using different exposure times at different times and study the variation in the different parameters such as electron densities and filling factors using O IV line probing the transition region. We discuss the non-thermal width variations of Si IV line, as well. These observations will be able to provide better insights into interpreting upcoming new observations from Solar Orbiter SPICE spectrometer.

Primary author

Ms Yamini K Rao (DAMTP, University of Cambridge)

Co-authors

Giulio Del Zanna (DAMTP, University of Cambridge) Helen Mason (DAMTP, University of Cambridge)

Presentation materials