Changes in the sensitivity of solar p-mode frequency shifts to activity over three solar cycles (2018)
Attributed to:
Asteroseismology and Helioseismology at Birmingham and Queen Mary
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1807.01504
Publication URI: https://arxiv.org/abs/1807.01504
Type: Other