Intensity contrast from MHD simulations and HINODE observations

Astronomy and Astrophysics

Volumn 526, Issue 15, 2011, Pages

  Afram, N ^a   Unruh, Y C ^a   Solanki, S K ^b,c   Schussler M ^b   Lagg, A ^b   Vogler A ^d  

^a IMPERIAL COLLEGE LONDON   (United Kingdom)

^b MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^c Kyung Hee University   (South Korea)

^d UTRECHT UNIVERSITY   (Netherlands)

Author keywords

Sun: activity; Sun: surface magnetism

Indexed keywords

1-D MODELS; BROAD BANDS; DEFOCUS; EARTH'S CLIMATE; FLUX TUBES; INTENSITY DISTRIBUTION; LONG-TERM CHANGES; MAGNETIC ELEMENTS; MAGNETIC FLUX TUBE; MHD SIMULATION; SCATTERED LIGHT; SOLAR ATMOSPHERE; SOLAR DISK; SOLAR SPECTRAL IRRADIANCE; SOLAR SURFACES; SPACE OBSERVATIONS; SPECTRAL IRRADIANCE; SPECTRAL SYNTHESIS; SUN: ACTIVITY; THEORETICAL POINTS; VERTICAL MAGNETIC FIELDS; VISIBLE CONTINUUM; WAVELENGTH COVERAGE;

EARTH (PLANET); HARMONIC ANALYSIS; MAGNETIC FIELDS; MAGNETIC FLUX; MAGNETIC STRUCTURE; OPTICAL SYSTEMS; OPTICAL TELESCOPES; SPECTROSCOPY;

THREE DIMENSIONAL;

EID: 78651306105     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015582     Document Type: Article

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