Tests for coronal electron temperature signatures in suprathermal electron populations at 1 AU

The development of knowledge of how the coronal origin of the solar wind affects its in situ properties is one of the keys to understanding the relationship between the Sun and the heliosphere. <br><br> In this paper, we analyse ACE/SWICS and WIND/3DP data spanning  &gt; 12 years...

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Bibliographic Details
Main Authors: A. R. Macneil, C. J. Owen, R. T. Wicks
Format: Article
Language:English
Published: Copernicus Publications 2017-12-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/35/1275/2017/angeo-35-1275-2017.pdf