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The centroid speed as a characteristic of the group speed of solar coronal fast magnetoacoustic wave trains (2023)

First Author: Kolotkov D

Attributed to: Fundamental plasma physics of the sun and heliosphere: Warwick CFSA Consolidated Grant Application funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2311.14512

Publication URI: https://arxiv.org/abs/2311.14512

Type: Preprint