Three-dimensional Radiative Transfer Simulations of the Scattering Polarization of the Hydrogen Lyalpha Line in a Magnetohydrodynamic Model of the Chromosphere-Corona Transition Region

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F15%3A00444747" target="_blank" >RIV/67985815:_____/15:00444747 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1088/0004-637X/803/2/65" target="_blank" >http://dx.doi.org/10.1088/0004-637X/803/2/65</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1088/0004-637X/803/2/65" target="_blank" >10.1088/0004-637X/803/2/65</a>

Result language
angličtina
Original language name
Three-dimensional Radiative Transfer Simulations of the Scattering Polarization of the Hydrogen Lyalpha Line in a Magnetohydrodynamic Model of the Chromosphere-Corona Transition Region
Original language description
Probing the magnetism of the upper solar chromosphere requires measuring and modeling the scattering polarization produced by anisotropic radiation pumping in UV spectral lines. Here we apply PORTA (a novel radiative transfer code) to investigate the hydrogen Ly alpha line in a three-dimensional model of the solar atmosphere resulting from a state of the art magnetohydrodynamic (MHD) simulation.
Czech name
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Czech description
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Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Project
<a href="/en/project/GPP209%2F12%2FP741" target="_blank" >GPP209/12/P741: Spectropolarimetric modeling and diagnostics of magnetic fields in the upper atmosphere of the quiet Sun</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2015
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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