搜索结果: 1-3 共查到“理学 COOL STARS”相关记录3条 . 查询时间(0.14 秒)
Non-radial modes in cool stars
Non-radial modes cool stars
font style='font-size:12px;'>
2011/9/29
In cool stars that oscillate like the Sun, non-radial modes become mixed as the stars evolve. The mixing is caused by the coupling between g-modes in the stellar core and p-modes in the envelope, whic...
MAGNETIC FIELDS IN COOL STARS
MAGNETIC FIELDS COOL STARS
font style='font-size:12px;'>
2009/4/23
MAGNETIC FIELDS IN COOL STARS。
Facular Structures on Cool Stars
Cool Stars Facular Structures dark spots
font style='font-size:12px;'>
2010/4/16
Activity has many manifestations, from dark spots to bright regions, to the presence of the heated chromosphere, to the superheated corona. Sunspots are extended, strongly magnetic regions on the Sun....