High-resolution wave dynamics in the lower solar atmosphere
High-resolution wave dynamics in the lower solar atmosphere
About this item
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Author / Creator
Publisher
England: Royal Society
Journal title
Language
English
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Publication information
Publisher
England: Royal Society
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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
Author / Creator
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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