Bibcode
Arregui, I.; Goossens, M.
Bibliographical reference
Astronomy and Astrophysics, Volume 622, id.A44, 10 pp.
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2
2019
Journal
Citations
19
Refereed citations
19
Description
The aim of this paper is to point out that the classic seismological
problem using observations and theoretical expressions for the periods
and damping times of transverse standing magnetohydrodynamic waves in
coronal loops is better referred to as a reduced seismological problem.
"Reduced" emphasises the fact that only a small number of characteristic
quantities of the equilibrium profiles can be determined. Reduced also
implies that there is no unique solution to the full seismological
problem. Even the reduced seismological problem does not allow a unique
solution. Bayesian inference results support our mathematical arguments
and offer insight into the relationship between the algebraic and the
probabilistic inversions.
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