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Resonant damping of solar p-modes by the chromospheric magnetic field
W. J. Tirry
*
, M. Goossens
,
B. Pintér
, V. Čadež
, P. Vanlommel
*
Corresponding author for this work
Department of Physics
KU Leuven
Center for Astrophysics Harvard & Smithsonian
Research output
:
Contribution to journal
›
Article
›
peer-review
34
Citations (Scopus)
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Earth and Planetary Sciences
Damping
100%
Solar Oscillation
75%
Magnetohydrodynamics
50%
Magnetic Field
50%
Continuous Spectra
50%
Dissipation
50%
Rate
25%
Frequency Shift
25%
Solar Atmosphere
25%
Plasma
25%
Effort
25%
Model
25%
Chromosphere
25%
Heat
25%
Tool
25%
Plasma Density
25%
Resonant Frequency
25%
Coupling
25%
Couple
25%
Nonuniformity
25%
Plasma Temperature
25%
Physics
Yaw
100%
Solar Oscillations
75%
Magnetohydrodynamics
50%
Frequencies
50%
Dissipation
50%
Magnetohydrodynamic Wave
50%
Magnetic Fields
50%
Continuous Spectra
50%
Frequency Shift
25%
Gravitational Singularities
25%
Heat
25%
Model
25%
Plasma Temperature
25%
Plasma Density
25%
Resonant Frequencies
25%
Nonuniformity
25%