KU Leuven CmPA Seminar: Quasimodes in the cusp continuum in nonuniform photospheric flux tubes

KU Leuven Centre for mathematical Plasma-Astrophysics Seminar

Title:    Quasimodes in the cusp continuum in nonuniform photospheric flux tubes

Speaker: Michaël Geeraerts from CmPA

Abstract

The study of magnetohydrodynamic (MHD) waves is important both for understanding heating in the solar atmosphere (and in particular the corona) and for solar atmospheric seismology. The analytical investigation of wave mode properties in a cylinder is of particular interest in this domain because many atmospheric structures can be modeled as such in a first approximation. The aim of this study is to use linear ideal MHD to investigate quasimodes (global modes that are damped through resonant absorption) with a frequency in the cusp continuum, in a straight cylinder with a circular cross-section and an inhomogeneous layer at its boundary separating two homogeneous plasma regions inside and outside. We are particularly interested in the damping of these modes, and therefore try to determine their frequency for given background conditions and wave parameters. After linearizing the ideal MHD equations, we find solutions to the second-order differential equation for the perturbed total pressure in the inhomogeneous layer in the form of (1) Frobenius series around the regular singular points that are the Alfvén and cusp resonant positions, and (2) power series around regular points. By connecting these solutions appropriately through the inhomogeneous layer and with the solutions of the homogeneous regions inside and outside the cylinder, we derive a dispersion relation for the frequency of the modes of the system. From the dispersion relation, it is possible to find the frequency of quasimodes even though they are not eigenmodes. As an example, we investigate the frequency of the slow surface sausage quasimode as a function of the width of the inhomogeneous layer for background conditions and wave parameters relevant to observations of slow sausage waves in a photospheric pore. The results closely match findings by other authors who studied the resistive slow surface sausage eigenmode in similar conditions.

 

The seminars are in hybrid mode, you can follow in person in room 200B 00.07 or online  at the (permanent) link:

https://eu.bbcollab.com/guest/7406a5ec00dc4ec6948200f9c769d454

Date: 

Thursday, April 28, 2022 - 14:00 to 15:00
 

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