Science. 1975 Aug 15;189(4202):547-9. doi: 10.1126/science.189.4202.547.
The NO(2) abundance in the stratosphere has been determined from ground-based spectra of the rising and setting sun and moon and of the twilight sky near 4500 angstroms. The spectra were taken at the Fritz Peak Observatory, at an altitude of 3 kilometers in the Colorado mountains. Separation of the stratospheric contribution requires observations at a relatively unpolluted site; direct measurement of the tropospheric absorption in the Colorado mountains often yields an upper limit on the tropospheric mixing ratio of 0.1 part per billion. The stratospheric NO(2) abundance is two to three times greater at night than during the day and increases significantly during the course of a sunlit day; these changes are related to photolytic decomposition of NO(2) and N(2)O(5) in the daytime stratosphere. Absorption by NO(3) was sought but not found; the results set an upper limit of 2 percent on the nighttime abundance ratio of NO(3) to NO(2) in the stratosphere.
平流层中的 NO(2)丰度是通过对日出和日落时的地面太阳和月球光谱以及近 4500 埃处的曙光天空光谱进行测量来确定的。这些光谱是在科罗拉多山脉海拔 3 公里的弗里茨峰观测站拍摄的。要分离平流层的贡献,需要在相对未受污染的地点进行观测;在科罗拉多山脉直接测量对流层吸收,通常对流层混合比的上限为 0.1 十亿分之一。夜间平流层中的 NO(2)丰度比白天高两到三倍,并在白天的阳光照射过程中显著增加;这些变化与白天平流层中 NO(2)和 N(2)O(5)的光解分解有关。虽然寻找了但没有发现 NO(3)的吸收;这些结果对平流层中 NO(3)与 NO(2)的夜间丰度比设定了 2%的上限。