英语释义

• the intensely luminous surface of a star (especially the sun)

片语

quiet photosphere[天]

photosphere U色球层

extended photosphere[天]

rarefaction photosphere疏松光团

model photosphereThe photosphere denotes those solar or stellar surface layers from which optical radiation escape These stellar outer layers can be modeled by different computer program

Photosphere E光球

solar photosphere太阳光球

英汉例句

• photosphere means light sphere, 「 which is the brightest layer of the sun」s atmosphere.

  光球层意味着「发光的球面」，是太阳大气层最明亮的一层。

• the photosphere is the lowest layer of the sun「s atmosphere, and emits the light we see.

  光球是太阳大气的最底层，我们看到的光线就是从它发出的。

• the material in the arched sheet comes mainly from the transition region and the photosphere and is further cooled by radiation, giving rise to a low-temperature prominence loop.

  拱形电流片物质主要来自过渡层和光球层，并通过辐射损失进一步冷却，形成低温日珥环；

• detailed studies on magnetic field topology above photosphere have been done.

  人们对磁场拓扑结构进行了深入的研究。

• from about 200 km above the photosphere outward extension of the height of 100 km area.

  从光球之上约200公里的高度向外延伸100公里的区域。

• her hopes mingled with the sunshine in an ideal photosphere which surrounded her as she bounded along against the soft south wind.

  迎着温柔的南风，她一路跳跃着向前走去，她的希望同阳光融合在一起，似乎幻化成了一道环绕着她的光环。

• i learnt from him many of the songs in his repertoire and these were in even greater request than my talks about the photosphere of the sun or the many moons of saturn.

  我从他身上学到了许多歌曲。这些歌曲可比我对太阳这个发光体和土星上的卫星的有关讲述，更受人欢迎。

• some people investigate magnetic topology by analyzing magnetic field of photosphere directly.

  或者直接利用观测的光球矢量场来研究磁场拓扑。

• temperatures in the dark centers of sunspots drop to about 3700 k (compared to 5700 k for the surrounding photosphere ).

  太阳黑子的温度在黑暗的中心，下降至约3700度（5700k中比周围光球）。

• the cause of filament destabilization is interpreted as steady cancellationreconnection in the photosphere layer.

  我们把暗条失稳的原因解释为光球层中稳定的对消重联。

• the interaction of velocity and magnetic fields on the photosphere is the primary cause of transporting the magnetic energy and complexity to the corona;

  光球层 等离子体的运动和磁场的相互作用，是造成磁能和磁复杂性向日冕传播的主要根源；

• the brightness of the photosphere prevents people from seeing the outer layer of the sun」s atmosphere.

  光球层的亮度阻止了人们看到太阳大气层的外层。

• it turns out that zinc, gallium, and copper are very difficult to measure precisely in the solar photosphere so our measurements of the sun may not be quite right.

  其结果是在太阳光球层中的锌、镓、铜恰好是很难测定的，那么我们对太阳的测量 方法可能不是很正确。