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Coronal hole boundaries evolution at small scales II. XRT view. Can small-scale outflows at CHBs be a source of the slow solar wind? (2010)

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/200913624

Publication URI: http://dx.doi.org/10.1051/0004-6361/200913624

Type: Journal Article/Review

Parent Publication: Astronomy and Astrophysics