The solar minimum corona from differential emission measure tomography
We present results derived from a dual-spacecraft tomographic reconstruction of the solar corona's three-dimensional (3D) extreme ultraviolet (EUV) emissivity. We use simultaneously taken STEREO A and B spacecraft EUVI images from Carrington rotation 2077 (UT 2008 November 20 06:56 through UT D...
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2010
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v715_n2_p1352_Vasquez http://hdl.handle.net/20.500.12110/paper_0004637X_v715_n2_p1352_Vasquez |
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