What do spectral line profile asymmetries tell us about the solar atmosphere?

Astrophysical Journal

Volumn 732, Issue 2, 2011, Pages

  Martínez Sykora, Juan ^a,b   De Pontieu, Bart ^a   Hansteen, Viggo ^b   McIntosh, Scott W ^c  

^a LOCKHEED MARTIN   (United States)

^b UNIVERSITY OF OSLO   (Norway)

^c NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

Author keywords

magnetohydrodynamics (MHD); methods: numerical; radiative transfer; Sun: atmosphere; Sun: chromosphere; Sun: corona; Sun: transition region

Indexed keywords

EID: 79955650596     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/732/2/84     Document Type: Article

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