3D temperatures and densities of the solar corona via multi-spacecraft EUV tomography: Analysis of prominence cavities
Three-dimensional (3D) tomographic analysis of extreme ultraviolet (EUV) images is used to place empirical constraints on the corona's temperature and density structure. The input data are images taken by the EUVI instrument on STEREO A and B spacecraft for Carrington Rotation 2069 (16 April to...
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Autores principales: | Vásquez, A.M., Frazin, R.A., Kamalabadi, F. |
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Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00380938_v256_n1-2_p73_Vasquez |
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