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Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Comparison of a Global Magnetic Evolution Model with Observations of Coronal Mass Ejections

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Comparison of Convective Overshooting Models and Their Impact on Abundances from Integrated Light Spectroscopy of Young ($<$ 3 Gyr) Star Clusters

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Comparison of Energies Between Eruptive Phenomena and Magnetic Field in AR 10930

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Comparison of Fe and Ni opacity calculations for a better understanding of pulsating stellar envelopes

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Comparison of Hinode/XRT and RHESSI detection of hot plasma in the non-flaring solar corona

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Comparison of limb-darkening laws from plane-parallel and spherically-symmetric model stellar atmospheres

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Comparison of seismic signatures of flares obtained by SOHO/MDI and GONG instruments

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Comparison of synthetic maps from truncated jet-formation models with YSO jet observations

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Comparison of synthetic maps from truncated jet-formation models with YSO jet observations. II. The effect of varying inclinations

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Comparison of the sidereal angular velocity of subphotospheric layers and small bright coronal structures during the declining phase of solar cycle 23

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Comparison of the thin flux tube approximation with 3D MHD simulations

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Comparison of Two Solar Minima: Narrower Streamer Stalk Region and Conserved Open Magnetic Flux in the Region Outside of Streamer Stalk

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Comparisons and Comments on Electron and Ion Impact Profiles of Spectral Lines

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Comparisons of Supergranule Characteristics During the Solar Minima of Cycles 22/23 and 23/24

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Competitive Accretion in Sheet Geometry and the Stellar IMF

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Complete calculation of evaluated Maxwellian-averaged cross sections and their uncertainties for s-process nucleosynthesis

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Complex asteroseismology of the $β$ Cep/SPB pulsator $ν$ Eridani: constraints on opacities

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Complex asteroseismology of the B-type main sequence pulsators

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Complex asteroseismology of the hybrid B-type pulsator $γ$ Pegasi: a test of stellar opacities

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