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High-resolution wave dynamics in the lower solar atmosphere

High-resolution wave dynamics in the lower solar atmosphere

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_pubmedcentral_primary_oai_pubmedcentral_nih_gov_7780137

High-resolution wave dynamics in the lower solar atmosphere

About this item

Full title

High-resolution wave dynamics in the lower solar atmosphere

Publisher

England: Royal Society

Journal title

Philosophical transactions of the Royal Society of London. Series A: Mathematical, physical, and engineering sciences, 2021-02, Vol.379 (2190), p.1-15, Article 20200169

Language

English

Formats

Publication information

Publisher

England: Royal Society

Subjects

Subjects and topics

More information

Scope and Contents

Contents

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 interplay between the rapidly evolving densities, tempe...

Alternative Titles

Full title

High-resolution wave dynamics in the lower solar atmosphere

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_pubmedcentral_primary_oai_pubmedcentral_nih_gov_7780137

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_pubmedcentral_primary_oai_pubmedcentral_nih_gov_7780137

Other Identifiers

ISSN

1364-503X

E-ISSN

1471-2962

DOI

10.1098/rsta.2020.0169

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