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تسجيل مستخدم جديدThermodynamic Structure of the Solar Corona: Tomographic Reconstructions and MHD Modeling
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We carry out a study of the global three-dimensional (3D) structure of the electron density and temperature of the quiescent inner solar corona ($r<1.25 R_odot$) by means of tomographic reconstructions and magnetohydrodynamic simulations. We use differential emission measure tomography (DEMT) and the Alfven Wave Solar Model (AWSoM), in their late
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