chromosphere造句

• It is difficult to photograph the actual chromosphere .
  拍摄实际的色球层很困难。
• The chromosphere is a frothy layer churned up by gases in the photosphere .
  色球层在光球层气体的搅拌下是个多泡层。
• Acoustic waves are a primary candidate for supplying the energy necessary to heat the solar chromosphere and corona .
  声波是供给太阳色球和日冕加热所需能量的主要候选能源。
• Active chromosphere binary
  活动色球双星
• Hybrid - chromosphere star
  混合色球星
• Active chromosphere star
  活动色球星
• White chromosphere one
  白色球粒
• Is the outermost layer of the sun . similar to the chromosphere , usually it is only visible during total solar eclipse
  是太阳大气的最外层，和色球层相类，亦是通常只能在日全食时才看得见。
• K . we still cannot completely explain why the temperature of the chromosphere and corona can be higher than the photosphere
  度。为甚么日冕和色球层的温度可以比光球层更高，仍是天文学上一个未解之谜。
• As shown in the photo below are eruptions of the gas trapped in the magnetic fields in the chromosphere . usually , they are about a few times the size of the earth
  如下图所示是被太阳磁场困著的表面气体爆发，很多时可以喷发至数个地球大小的高度。
• Those inflexion are brought by the energy balance and heating mechanism in stellar chromosphere and corona . using large samples , we gain several credible numeric relation between different magnetic activity index and rotational parameters
  我们通过对大样本恒星的统计分析分别得到了晚型主序星磁活动与恒星自转参量间以及磁活动与恒星色指数之间更广泛意义的数值关系。
• This phenomenon farther surport our conclusion in the analysis of evolution stars , i . e . the difference of stellar chromosphere and corona activity of evolution stars is bred by the energy balance and heating mechanism in stellar chromosphere and corona
  M型主序星在演化恒星的冕球活动与色球活动行为的差异则是由于m型主序星的色球与冕球间存在的能量平衡和转移过程产生的。