Figure 1 from DIRECT OBSERVATION OF SOLAR CORONAL MAGNETIC FIELDS BY VECTOR TOMOGRAPHY OF THE CORONAL EMISSION LINE POLARIZATIONS

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DIRECT OBSERVATION OF SOLAR CORONAL MAGNETIC FIELDS BY VECTOR TOMOGRAPHY OF THE CORONAL EMISSION LINE POLARIZATIONS

Authors: M. Kramar, H. Lin, and S. Tomczyk

2016 The Astrophysical Journal Letters 819 L36.

Provider: AAS Journals

Caption: Figure 1.

Spherical cross-section of the reconstructed 3D electron temperature (top) and density (middle) at a heliocentric distance of ﹩1.17{R}_{\odot }﹩ obtained with EUVI Tomography, and an electron density map at ﹩2.0{R}_{\odot }﹩ obtained with STEREO/COR1 tomography (bottom).

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