A Solar cycle correlation of coronal element abundances in Sun-as-a-star observations

The Sun’s elemental composition is a vital part of understanding the processes that transport energy from the interior to the outer atmosphere. Here, the authors show that if the Sun is observed as a star, then the variation of coronal composition is highly correlated with the F10.7cm radio flux.

Guardado en:

Detalles Bibliográficos
Autores principales:	David H. Brooks, Deborah Baker, Lidia van Driel-Gesztelyi, Harry P. Warren
Formato:	article
Lenguaje:	EN
Publicado:	Nature Portfolio 2017
Materias:	Science Q
Acceso en línea:	https://doaj.org/article/1c8300afa243440dbb205c7aeea9a194
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

id	oai:doaj.org-article:1c8300afa243440dbb205c7aeea9a194
record_format	dspace
spelling	oai:doaj.org-article:1c8300afa243440dbb205c7aeea9a1942021-12-02T10:48:10ZA Solar cycle correlation of coronal element abundances in Sun-as-a-star observations10.1038/s41467-017-00328-72041-1723https://doaj.org/article/1c8300afa243440dbb205c7aeea9a1942017-08-01T00:00:00Zhttps://doi.org/10.1038/s41467-017-00328-7https://doaj.org/toc/2041-1723The Sun’s elemental composition is a vital part of understanding the processes that transport energy from the interior to the outer atmosphere. Here, the authors show that if the Sun is observed as a star, then the variation of coronal composition is highly correlated with the F10.7cm radio flux.David H. BrooksDeborah BakerLidia van Driel-GesztelyiHarry P. WarrenNature PortfolioarticleScienceQENNature Communications, Vol 8, Iss 1, Pp 1-7 (2017)
institution	DOAJ
collection	DOAJ
language	EN
topic	Science Q
spellingShingle	Science Q David H. Brooks Deborah Baker Lidia van Driel-Gesztelyi Harry P. Warren A Solar cycle correlation of coronal element abundances in Sun-as-a-star observations
description	The Sun’s elemental composition is a vital part of understanding the processes that transport energy from the interior to the outer atmosphere. Here, the authors show that if the Sun is observed as a star, then the variation of coronal composition is highly correlated with the F10.7cm radio flux.
format	article
author	David H. Brooks Deborah Baker Lidia van Driel-Gesztelyi Harry P. Warren
author_facet	David H. Brooks Deborah Baker Lidia van Driel-Gesztelyi Harry P. Warren
author_sort	David H. Brooks
title	A Solar cycle correlation of coronal element abundances in Sun-as-a-star observations
title_short	A Solar cycle correlation of coronal element abundances in Sun-as-a-star observations
title_full	A Solar cycle correlation of coronal element abundances in Sun-as-a-star observations
title_fullStr	A Solar cycle correlation of coronal element abundances in Sun-as-a-star observations
title_full_unstemmed	A Solar cycle correlation of coronal element abundances in Sun-as-a-star observations
title_sort	solar cycle correlation of coronal element abundances in sun-as-a-star observations
publisher	Nature Portfolio
publishDate	2017
url	https://doaj.org/article/1c8300afa243440dbb205c7aeea9a194
work_keys_str_mv	AT davidhbrooks asolarcyclecorrelationofcoronalelementabundancesinsunasastarobservations AT deborahbaker asolarcyclecorrelationofcoronalelementabundancesinsunasastarobservations AT lidiavandrielgesztelyi asolarcyclecorrelationofcoronalelementabundancesinsunasastarobservations AT harrypwarren asolarcyclecorrelationofcoronalelementabundancesinsunasastarobservations AT davidhbrooks solarcyclecorrelationofcoronalelementabundancesinsunasastarobservations AT deborahbaker solarcyclecorrelationofcoronalelementabundancesinsunasastarobservations AT lidiavandrielgesztelyi solarcyclecorrelationofcoronalelementabundancesinsunasastarobservations AT harrypwarren solarcyclecorrelationofcoronalelementabundancesinsunasastarobservations
_version_	1718396634454294528

A Solar cycle correlation of coronal element abundances in Sun-as-a-star observations

Ejemplares similares