Simulation of a flux emergence event and comparison with observations by Hinode

Astronomy and Astrophysics

Volumn 507, Issue 3, 2009, Pages

  Yelles Chaouche, L ^a,b   Cheung, M C M ^c   Solanki, S K ^a,d   Schussler M ^a   Lagg, A ^a  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^c LOCKHEED MARTIN   (United States)

^d Kyung Hee University   (South Korea)

Author keywords

Magnetohydrodynamics (MHD); Sun: magnetic fields; Sun: photosphere

Indexed keywords

ATMOSPHERIC PARAMETERS; BLUE SHIFT; FLUX EMERGENCE; FLUX TUBES; LARGE PARTS; MAGNETIZED PLASMAS; MAGNETOHYDRODYNAMICS SUNS; MHD SIMULATION; RADIATIVE COOLING; SOLAR ATMOSPHERE; SPECTRAL LINE; STOKES SPECTRA; SYNTHETIC DATA; SYNTHETIC SPECTRA; TYPE INVERSION;

ATMOSPHERIC STRUCTURE; FLUID DYNAMICS; MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; PHOTODEGRADATION; SPECTROSCOPY; SUN; UPPER ATMOSPHERE;

ATMOSPHERIC SPECTRA;

EID: 70849117978     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913181     Document Type: Article

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