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The relation between stellar magnetic field geometry and chromospheric activity cycles I: The highly variable field of Epsilon Eridani at activity minimum (2017)

First Author: Jeffers S

Attributed to: Astronomy and Planetary Sciences at the Open University (APSOU) funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1710.09227

Publication URI: https://arxiv.org/abs/1710.09227

Type: Other