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