太阳光球

最后对太阳光球型大气（见表3），计算了以一个氢粒子为单位的连续吸收系数ac（T，lgPe）。

Lastly , the continuous absorption coefficients a_c ( T , lgP_e ) of a H particle are calculated for the atmosphere of the solar photosphere type ( see Table 3 ) .

活动日冕，作为由电磁场和粒子组成的系统，其唯一的开场表面是太阳光球。

For an active corona , a system consisting of the electromagnetic field and particles , the only open surface is the solar photosphere .

太阳光球层磁重联的直接证据

Direct Evidence of Magnetic Reconnection in Photospheric Layer on the Sun

大地震事件的一个可能的天文因素&太阳光球磁场

A possible astronomical factor for major seismic events & the photospheric magnetic field

本文讨论了从太阳光球向日冕传输磁能和磁复杂性的过程。

A discussion on the transport of magnetic energy and complexity to the corona is given in this paper .

食既：太阳与月球第一次内切，太阳光球刚完全被月球掩蔽的时刻。

Fresh both : the sun and the moon within the first cut , sun-moon has just been totally masking the moment .

生光：太阳与月球第二次内切，太阳光球刚从月球西面露出来的时刻。

Health : the sun and the moon , the second cut , sun-exposed just west of the moon moment .

初亏：太阳与月球第一次外切，太阳光球西面刚切入月球东面的时刻。

Early losses : the sun and the moon , the first cut , just west of the sun-Cut east of the moon moment .