The Amplitude of Solar p-mode Oscillations from Three-dimensional Convection Simulations
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Zhou, Yixiao; Asplund, Martin; Collet, Remo
Description
The amplitude of solar p-mode oscillations is governed by stochastic excitation and mode damping, both of which take place in the surface convection zone. However, the time-dependent, turbulent nature of convection makes it difficult to self-consistently study excitation and damping processes through the use of traditional one-dimensional (1D) hydrostatic models. To this end, we carried out ab initio three-dimensional (3D), hydrodynamical numerical simulations of the solar atmosphere to...[Show more]
Collections | ANU Research Publications |
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Date published: | 2019-07-18 |
Type: | Journal article |
URI: | http://hdl.handle.net/1885/232538 |
Source: | The Astrophysical Journal |
DOI: | 10.3847/1538-4357/ab262c |
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01_Zhou_The_Amplitude_of_Solar_p-mode_2019.pdf | 874.7 kB | Adobe PDF | Request a copy |
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