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High-resolution wave dynamics in the lower solar atmosphere

The magnetic and convective nature of the Sun’s photosphere provides a unique platform from which generated waves can be modelled, observed and interpreted across a wide breadth of spatial and temporal scales. As oscillations are generated in-situ or emerge through the photospheric layers, the inter...

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Dades bibliogràfiques
Publicat a:Philos Trans A Math Phys Eng Sci
Autors principals: Jess, D. B., Keys, P. H., Stangalini, M., Jafarzadeh, S.
Format: Artigo
Idioma:Inglês
Publicat: The Royal Society Publishing 2021
Matèries:
Accés en línia:https://ncbi.nlm.nih.gov/pmc/articles/PMC7780137/
https://ncbi.nlm.nih.gov/pubmed/33342388
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rsta.2020.0169
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