Analytic Approximate Seismology of Propagating Magnetohydrodynamic Waves in the Solar Corona
Observations show that propagating magnetohydrodynamic (MHD) waves are ubiquitous in the solar atmosphere. The technique of MHD seismology uses the wave observations combined with MHD wave theory to indirectly infer physical parameters of the solar atmospheric plasma and magnetic field. Here, we present an analytical seismological inversion scheme
Goossens, M. et al.
Fecha de publicación:
12
2012