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Abstract: The introduction to this review summarizes chromosphere observation in twofigures. The first part showcases the historical emphasis on the eclipsechromosphere in the development of NLTE line formation theory and criticizes 1Dmodeling. The second part advertises recent breakthroughs after many decades ofstandstill. The third part discusses what may or should come next.



Autor: Robert J. Rutten

Fuente: https://arxiv.org/







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