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Matching temporal signatures of solar features to their corresponding solar wind outflows (2021)

First Author: De Pablos D

Attributed to: How do weak shocks accelerate high energy particles? funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2103.09077

Publication URI: https://arxiv.org/abs/2103.09077

Type: Other