Forward modeling of the corona of the sun and solarlike stars: from a three-dimensional magnetohydrodynamic model to syntheic extreme-ultraviolet spectra
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Forward modeling of the corona of the sun and solarlike stars : from a three-dimensional magnetohydrodynamic model to syntheic extreme-ultraviolet spectra. / Hardi, Peter; Gudiksen, Boris V.; Nordlund, Å.
In: Astrophysical Journal, Vol. 638, 2006, p. 1086-1100.Research output: Contribution to journal › Journal article › Research › peer-review
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TY - JOUR
T1 - Forward modeling of the corona of the sun and solarlike stars
T2 - from a three-dimensional magnetohydrodynamic model to syntheic extreme-ultraviolet spectra
AU - Hardi, Peter
AU - Gudiksen, Boris V.
AU - Nordlund, Å.
PY - 2006
Y1 - 2006
N2 - Transition Region Lines, AB-Initio Approach; Nonequilibrium Inozation; Doppler Shifts; Emission-Lines; Quiet-Sun; Sumer Telescope; Atomic Database; Magnetic-Field; Thin Plasmas
AB - Transition Region Lines, AB-Initio Approach; Nonequilibrium Inozation; Doppler Shifts; Emission-Lines; Quiet-Sun; Sumer Telescope; Atomic Database; Magnetic-Field; Thin Plasmas
M3 - Journal article
VL - 638
SP - 1086
EP - 1100
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
ER -
ID: 1121248