1) magnetic activity
磁场活动
3) field magnetomotive force
磁场磁动势
4) Domain activities
磁畴活动
5) Geomagnetic activity
地磁活动
6) magnetic activity
磁活动
1.
Since RS CVn-type binary was defined by Hall in 1976, the solar-type activity(" chromospheric activity" or "magnetic activity") of contact binaries interests many astronomic researchers.
自从1976年，Hall明确地提出RS CVn型双星的定义以来，密近双星的类太阳活动(也叫“色球活动”或“磁活动”)性质就引起众多天文工作者的极大兴趣。
2.
Under this extreme physical conditions, RS CVn-type binaries show all features of solar activity: chromospheric emission lines (such as Hα, Hβ, CaII H&K), X-ray emission, spots, flare, mass loss due to star wind, magnetic activity, and orbital period variations.
在这种极端物理条件下,RS CVn型双星表现出了许多类似太阳的磁活动现象:色球活动(如Hα,Hβ,CaII H&K等谱线发射)、X射线发射、大面积的黑子活动、耀斑、星风损失以及轨道周期变化。
补充资料：安培环路定律(见磁场强度)
安培环路定律(见磁场强度)
Ampere's circuital law
A rlpe{h口。)11L一dingILJ安培环路定律(Amp之re’5 CirC。ital law)见磁场强度。
说明：补充资料仅用于学习参考，请勿用于其它任何用途。
参考词条