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日落科学。二、一张有用的图表。

Sunset Science. II. A useful diagram.

作者信息

Young A T, Kattawar G W

出版信息

Appl Opt. 1998 Jun 20;37(18):3785-92. doi: 10.1364/ao.37.003785.

Abstract

We present diagrams that show how layers in atmospheric thermal structure are related to the altitudes at which they are seen tangentially. These dip diagrams show that the inferior mirage greatly magnifies the apparent angular size of the lowest few centimeters of atmosphere. Conversely, inversion layers below eye level are compressed-even to zero apparent thickness, in ducts. The diagrams show that, even when distant objects are miraged, the ray crossings occur beyond the lowest point on each ray where the line of sight is tangent to a horizontal surface in the atmosphere. Therefore the apparent altitudes of these tangent points are a monotonic function of their actual heights in the atmosphere. This monotonicity explains an apparent paradox in low-Sun images.

摘要

我们展示了一些图表,这些图表显示了大气热结构中的各层与它们被切线观测时的高度之间的关系。这些倾角图表表明,下蜃景会极大地放大大气最底层几厘米的视在角大小。相反,低于视线水平的逆温层会被压缩——在管道中甚至会被压缩到视在厚度为零。这些图表表明,即使远处的物体出现了海市蜃楼现象,光线交叉点也出现在每条光线的最低点之后,在该点视线与大气中的水平面切线相切。因此,这些切点的视在高度是它们在大气中实际高度的单调函数。这种单调性解释了低太阳角度图像中一个明显的悖论。

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