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American Astronomical Society, Astrophysical Journal, 2(777), p. 167, 2013

DOI: 10.1088/0004-637x/777/2/167

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Establishing a Stereoscopic Technique for Determining the Kinematic Properties of Solar Wind Transients Based on a Generalized Self-Similarly Expanding Circular Geometry

This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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