Figure 4 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 4.

STEREO-B/EUVI image taken on 2011 July 20, when CoMP POS was at the longitude of 33°. Central meridian of the EUVI image is located at 33°. White dots show a carrington coordinate grid for every 30°.

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