Forward modeling of the corona of the sun and solarlike stars: from a three-dimensional magnetohydrodynamic model to syntheic extreme-ultraviolet spectra

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningfagfællebedømt

Transition Region Lines, AB-Initio Approach; Nonequilibrium Inozation; Doppler Shifts; Emission-Lines; Quiet-Sun; Sumer Telescope; Atomic Database; Magnetic-Field; Thin Plasmas
OriginalsprogEngelsk
TidsskriftAstrophysical Journal
Vol/bind638
Sider (fra-til)1086-1100
ISSN0004-637X
StatusUdgivet - 2006

ID: 1121248