Tipo de publicación: Sin árbitro

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    Introduction to the theory of stellar atmospheres
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    Introduction: under ancient Egyptian skies
    Not Available
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    Inverse problem approach in adaptive optics for the European-ELT
    Not Available
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    Inversion of Physical Parameters in Solar Atmospheric Seismology
    Magnetohydrodynamic (MHD) wave activity is ubiquitous in the solar atmosphere. MHD seismology aims to determine difficult to measure physical parameters in...
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    Inversion of Physical Parameters in Solar Coronal Magnetic Structures
    Magnetohydrodynamic seismology aims to determine difficult to measure physical parameters in the solar corona by a combination of observed and theoretical...
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    Inversion of Visible and IR Stokes Profiles in Sunspots
    We present an analysis of simultaneous observations of a sunspot in two different spectral ranges (630 nm and 1565 nm). The dataset was acquired with the...
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    Inversion Techniques Applied to Sunspot Spectropolarimetric Data
    Two inversion techniques are compared: the Unno-Rachkov-sky fitting method (UR) and the Stokes Inversion based on Response functions (SIR). Results with...
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    Inversion techniques: From observations to atmospheres
    Inversion techniques are presently the most powerful tools to deduce magnetic, dynamic, and thermal properties of the solar plasma from polarization line...
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    Inversions of L12-2 IMaX data of an emerging flux mantle
    We present the analysis of a flux emergence event observed with the IMaX magnetograph flown aboard the SUNRISE balloon. IMaX took a 15' sequence with cadence of...