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气球搭载的红外羟基气辉光谱观测。

Balloon-borne spectroscopic observation of the infrared hydroxyl airglow.

作者信息

Lowe R P, Lytle E A

出版信息

Appl Opt. 1973 Mar 1;12(3):579-83. doi: 10.1364/AO.12.000579.

Abstract

A balloon-borne grating spectrometer has been used to study the spectrum of the airglow between 1.8 microm and 3.6 microm and its diurnal variation. The principal features identified are the bands of the Deltaupsilon = 2 and Deltaupsilon = 1 sequences of the vibration-rotation spectrum of OH. The brightness of the 1-0 band at night was measured to be in the range 270-400 kR on two flights. A sudden decrease in the intensity of the hydroxyl bands occurred in morning twilight at a solar depression of 4 degrees and is ascribed to the photodissociation of ozone. The temperature, as indicated by the Q/R branch ratio, rose from 170 K at night to 255 K at noon indicating a reduction in the height of the emitting layer during the day.

摘要

一台气球搭载的光栅光谱仪被用于研究1.8微米至3.6微米之间气辉的光谱及其日变化。识别出的主要特征是OH振动-转动光谱中Δυ = 2和Δυ = 1序列的谱带。在两次飞行中,夜间1-0谱带的亮度测量值在270 - 400 kR范围内。在早晨曙光中,当太阳高度角为4度时,羟基谱带的强度突然下降,这归因于臭氧的光解。由Q/R分支比表示的温度从夜间的170 K上升到中午的255 K,表明白天发射层的高度降低。

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