Chromosphere

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不停地翻腾。

It is difficult to photograph the actual chromosphere .

拍摄实际的色球层很困难。

A possible mechanism of nonresonant heating of the chromosphere - corona transition zone

太阳色球-日冕过渡层非共振加热的可能机制

An observation study of the magnetic field on the solar-like chromosphere active star ε eri

类太阳色球活动星εEri磁场的观测研究

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。

The following results are revealed . 1 . For the first maximum , high energy electrons do not penetrate the chromosphere .

结果表明：1.耀斑的第一次极大，高能电子没有穿透到色球。

The rest escapes as sound waves , mechanical vibrations that heat the chromosphere , the middle layer of the sun 's atmosphere .

其余部分则以声波即机械振动的形式散逸，它们加热了太阳大气的中间一层，即色球层。

The chromosphere and corona can be seen from Earth when the sun is totally eclipsed by the moon .

当出现日全食时，从地球上可以看到太阳的色球层和电晕层。

This confirms the idea that the mechanical waves generated from the convection zone are not very effective in heating the chromosphere and corona .

这就证实了一些人认为的对流层机械波并不是一个对色球和日冕的有效加热机制的说法。

Colorant of naturally colored cotton fabric exists in the secondary cell wall of cellulose , the chromosphere is dependent on the carbonyl group .

天然彩棉的色素存在于纤维次生胞壁内，发色基团与羰基有关。

Solar-like Activities in Late-type Stars ( ⅱ): Active Chromosphere , Transition Region and Coronal Emissions , and Stellar Flares

晚型恒星中的类太阳活动（Ⅱ）：活动色球、过渡区和冕区发射、耀发活动

No , it was flare eruptions , which are the chromosphere and prominence on the landscape .

不，那是耀斑爆发，它与日珥都是色球层上的景观。

Center to limb observations show that the magnetic structures of small scale magnetic structures have not changed much when they extend from the solar photosphere to the chromosphere .

日面中心到边缘的观测表明，太阳宁静区中的小尺度磁结构在从光球到色球的扩展过程中变化不大。

Beyond the photosphere in the chromosphere and the extremely rarified corona , which extends millions of kilometres into space .

在光球层更外面的色球层以及极其稀薄的电晕，在空中延展几百万千米的范围。

Starting at the outside and going down into the Sun , the zones are the corona , chromosphere , photosphere . convection zone . and finally the core .

从太阳外部开始进入内部这些区域为：光环带、色球带、光球带、对流带，最终为核心带。

These observed results indicate that material evaporation occurs in the pre-flare phase , and violent variation of the chromospheric magnetic field probably is one of the reasons of causing chromosphere evaporation

这些现象清楚说明，物质沿磁力线的蒸发发生在耀斑前兆相，而且，色球磁场的剧烈变化可能是引起色球蒸发的原因之一

Axial Mixing and Gas Hold-Up of Gas-Liquid in Multistage Agitated Column The chromosphere is a frothy layer churned up by gases in the photosphere .

多级搅拌塔气液体系的轴向混合和气含率色球层在光球层气体的搅拌下是个多泡层。

The results indicate that the heating in the lower chromosphere and the upper photosphere , especially for large flares , can be caused neither by X-ray radiation nor by electron beam bombardment .

耀斑主相时，X线加热更能有效地平衡辐射损失.但是，尤其是对大耀斑来说，色球低层和光球上层的加热既不能用电子束轰击，也不能用X线的作用来解释；

Our conclusion is that we happened to observe an intensive short time-scale activity of the chromosphere of Arcturus characterized by mass outflow and outward motions of circumstellar matter .

分析认为我们观测到的是大角星的一次以天计的短时标色球剧烈活动，它伴随着物质的向外抛射，也引起星周物质的向外运动。

The chromospheric activity of II Peg is very strong , and exhibits an obvious rotational modulation phenomenon . The optical flare is happened In every rotational period , and it is through each layer of the chromosphere .

ⅡPeg的色球活动很强烈，有明显的自转调制现象，在我们观测的每个自转周里都有耀斑事件发生，且这样的耀斑事件是贯穿整个色球层的。

Solar spicules are rapidly evolving jets seen on the solar limb , extending from the bottom of the chromosphere to the corona . Spicule is the most common feature observed in the chromosphere .

太阳针状物是日面边缘上快速演化的喷流状结构，它可以从色球底部一直延伸到日冕，是色球层最普遍的观测现象之一。

During the major flare , the two-ribbon appearance , loop system formation , mass ejections and their flows back to the chromosphere had a good correspondance in time to the peaks of the 3.2 cm radio flux curve .

大耀斑爆发的Hα初始亮点，双带出现，环系形成，亮物质抛射和吸收冕珥等现象同3.2cm射电流量的变化在时间上有较好的对应关系。