The photodissociation of nitric oxide in the mesosphere and stratosphere

M. Nicolet; S. Cieslik

doi:10.1016/0032-0633(80)90107-5

The photodissociation of nitric oxide in the mesosphere and stratosphere

M. Nicolet
, S. Cieslik

Research output › peer-review

Abstract

A detailed calculation of the nitric oxide photodissoeiation rate has been made for application to mesospheric and stratospheric photochemistry. It takes into account a new determination of the oscillator strengths of the NO bands and is based on a critical analysis of the solar flux. Moreover it entails a complete determination of the molecular oxygen attenuation allowing for the rotational fine structure including the Voight profile of the Schumann-Runge bands.

Original language	English
Pages (from-to)	105-115
Number of pages	11
Journal	Planetary and Space Science
Volume	28
Issue number	1
DOIs	https://doi.org/10.1016/0032-0633(80)90107-5
State	Published - Jan 1980

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1016/0032-0633(80)90107-5

Cite this

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title = "The photodissociation of nitric oxide in the mesosphere and stratosphere",

abstract = "A detailed calculation of the nitric oxide photodissoeiation rate has been made for application to mesospheric and stratospheric photochemistry. It takes into account a new determination of the oscillator strengths of the NO bands and is based on a critical analysis of the solar flux. Moreover it entails a complete determination of the molecular oxygen attenuation allowing for the rotational fine structure including the Voight profile of the Schumann-Runge bands.",

author = "M. Nicolet and S. Cieslik",

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AU - Cieslik, S.

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AB - A detailed calculation of the nitric oxide photodissoeiation rate has been made for application to mesospheric and stratospheric photochemistry. It takes into account a new determination of the oscillator strengths of the NO bands and is based on a critical analysis of the solar flux. Moreover it entails a complete determination of the molecular oxygen attenuation allowing for the rotational fine structure including the Voight profile of the Schumann-Runge bands.

UR - https://www.scopus.com/pages/publications/0007818177

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DO - 10.1016/0032-0633(80)90107-5

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JO - Planetary and Space Science

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