Radio spectral imaging of the Crab Nebula during solar conjunction shows that coronal scattering becomes more anisotropic closer to the Sun and reveals substructures linked to a coronal streamer.
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Probing the Turbulent Corona and Heliosphere Using Radio Spectral Imaging Observation during the Solar Conjunction of Crab Nebula
Radio spectral imaging of the Crab Nebula during solar conjunction shows that coronal scattering becomes more anisotropic closer to the Sun and reveals substructures linked to a coronal streamer.