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HEATING OF THE PARTIALLY IONIZED SOLAR CHROMOSPHERE BY WAVES IN MAGNETIC STRUCTURES

journal contribution

posted on 2016-03-01, 00:00 authored by Sergiy ShelyagSergiy Shelyag, E Khomenko, A De Vicente, D Przybylski

HEATING OF THE PARTIALLY IONIZED SOLAR CHROMOSPHERE BY WAVES IN MAGNETIC STRUCTURES

History

Journal

Astrophysical Journal Letters

Volume

819

Issue

1

Article number

ARTN L11

Publisher

IOP PUBLISHING LTD

Publisher DOI

https://doi.org/10.3847/2041-8205/819/1/L11

ISSN

2041-8205

eISSN

2041-8213

Language

English

Author URL

http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000371044200011&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=a045e4b2bb1f2b747c68c720ec8913b7

Publication classification

C1.1 Refereed article in a scholarly journal

Copyright notice

2016, The American Astronomical Society

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Keywords

Science & Technology Physical Sciences Astronomy & Astrophysics Sun: chromosphere Sun: magnetic fields Sun: oscillations ION-NEUTRAL COLLISIONS ALFVEN WAVES MAGNETOHYDRODYNAMIC WAVES PARTIAL IONIZATION QUIET SUN SIMULATIONS OSCILLATIONS PHOTOSPHERE CONVECTION GENERATION

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All Rights Reserved

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