| 书目名称 | Differential Rotation in Sun-like Stars from Surface Variability and Asteroseismology |
| 编辑 | Martin Bo Nielsen |
| 视频video | |
| 概述 | Nominated as an outstanding PhD thesis by University of Göttingen,Göttingen, Germany.Presents the first constraints on radial differential rotation in Sun-like stars.Employs a straightforward methodol |
| 丛书名称 | Springer Theses |
| 图书封面 |  |
| 描述 | In his PhD dissertation Martin Bo Nielsen performs observational studies of rotation in stars like the Sun. The interior rotation in stars is thought to be one of the driving mechanisms of stellar magnetic activity, but until now this mechanism was unconstrained by observational data..NASA’s Kepler space mission provides high-precision observations of Sun-like stars which allow rotation to be inferred using two independent methods: asteroseismology measures the rotation of the stellar interior, while the brightness variability caused by features on the stellar surface trace the rotation of its outermost layers. By combining these two techniques Martin Bo Nielsen was able to place upper limits on the variation of rotation with depth in five Sun-like stars. These results suggest that the interior of other Sun-like stars also rotate in much the same way as our own Sun.. |
| 出版日期 | Book 2017 |
| 关键词 | Stellar Rotation; Asteroseismology; Differential Rotation; Sun-like Stars; Photometric Variability; Keple |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-3-319-50989-1 |
| isbn_softcover | 978-3-319-84539-5 |
| isbn_ebook | 978-3-319-50989-1Series ISSN 2190-5053 Series E-ISSN 2190-5061 |
| issn_series | 2190-5053 |
| copyright | Springer International Publishing Switzerland 2017 |
发表于 2025-3-21 18:40:19
