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单词 Limb darkening
释义

Limb darkening

中文百科

周边昏暗

周边昏暗的太阳-以可见光观察的太阳影像,因为密度向边缘逐渐降低而在太阳盘面的外缘显示出周边昏暗的效应。
周边昏暗的理想状况。半径的最外缘是来自恒星向外辐射的光子不再被吸收的区域,L 是光深度为1单位的距离。由A处辐射出的高温光子和由B处辐射出的低温光子都正好在可以逃脱的距离上。
An image of the Sun in visible light showing the limb-darkening effect as a drop in intensity towards the edge or limb of the solar disk. The image was taken during the 2012 transit of Venus (seen here as the dark disk at the upper right).

周边昏暗是恒星因为密度由中心向边缘逐渐降低而呈现出影像向边缘的强度减少。周边昏暗是两种效应造成的结果:

光深度的观念是了解周边昏暗的关键想法。光深度在光学上的1单位是由吸收气体能逃逸出来的比率达到1/e光子数量的厚度。这是为何定义了恒星可见的边缘之后,在光深度为1单位之处恒星就会变得不透明的原因。到达我们的辐射非常接近恒星释放出的能量沿着视线方向朝向我们,直至光深度为1单位处点的总量。当我们观察恒星的边缘时,我们不能看见如同观察中心一样的光深度,因为当观测边缘时,视线是以倾斜的角度在恒星的气体中行进。换言之,当我们观察太阳时,1光深度单位对应的长度在移向边缘时会逐渐增加。

英语百科

Limb darkening 周边昏暗

An image of the Sun in visible light showing the limb-darkening effect as a drop in intensity towards the edge or limb of the solar disk. The image was taken during the 2012 transit of Venus (seen here as the dark disk at the upper right).
An idealized case of limb darkening. The outer boundary is the radius at which photons emitted from the star are no longer absorbed. L is a distance for which the optical depth is unity. High-temperature photons emitted at A will just barely escape from the star, as will the low-temperature photons emitted at B. Note that for a typical star, this drawing is not to scale. E.g., for the Sun, L would be only a few hundred km.
周边昏暗的太阳-以可见光观察的太阳影像,因为密度向边缘逐渐降低而在太阳盘面的外缘显示出周边昏暗的效应。

Limb darkening is an optical effect seen in stars (including the Sun), where the center part of the disk appears brighter than the edge or limb of the image. Its understanding offered early solar astronomers an opportunity to construct models with such gradients. This encouraged the development of the theory of radiative transfer.

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更新时间:2025/6/20 23:23:06