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Measurement of rate constant for quenching CO2(0110) by atomic oxygen at low temperatures : Reassessment of the population of CO 2(0110) and the CO215-μm emission cooling in the lower thermosphere. / Shved, Gustav M.; Khvorostovskaya, Lyudmila E.; Potekhin, Igor Yu; Ogibalov, Vladimir P.; Uzyukova, Tatyana V.

In: Proceedings of SPIE - The International Society for Optical Engineering, Vol. 4882, 01.12.2002, p. 106-116.

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Author

Shved, Gustav M. ; Khvorostovskaya, Lyudmila E. ; Potekhin, Igor Yu ; Ogibalov, Vladimir P. ; Uzyukova, Tatyana V. / Measurement of rate constant for quenching CO2(0110) by atomic oxygen at low temperatures : Reassessment of the population of CO 2(0110) and the CO215-μm emission cooling in the lower thermosphere. In: Proceedings of SPIE - The International Society for Optical Engineering. 2002 ; Vol. 4882. pp. 106-116.

BibTeX

@article{3deb228736d34e75ae077269f4f93403,
title = "Measurement of rate constant for quenching CO2(0110) by atomic oxygen at low temperatures: Reassessment of the population of CO 2(0110) and the CO215-μm emission cooling in the lower thermosphere",
abstract = "The paper presents the first laboratory measurement of the rate constant for quenching the CO2(0110) state during collisions of CO2 molecules with O atoms at temperatures realized near the Earth's mesopause. The measurement was carried out with a hollow-cathode glow discharge in the temperature range 206-358 K. The measured values are significantly smaller than those commonly used in solving the non-LTE CO2 problem for the vibrational states of the mode v2 in the atmospheres of the Earth, Venus, and Mars. The measured temperature dependence of the rate constant is approximated by a simple relation, which is recommended for solving the above problem. The value of this rate constant is absolutely critical to remotely sense temperature, and hence also constituent densities, in the upper mesosphere and lower thermosphere of the Earth. The use of the new values of the rate constant significantly decreased the rate of cooling by the CO 2 15-μm emission in the terrestrial lower thermosphere as compared to the previous estimates obtained for this rate. Over the most area of the Earth's surface, the maximum cooling rate occurs at an altitude of about 110 km and amounts to about 20 K/day.",
keywords = "Atmospheric infrared emission, Hollow-cathode glow discharge, Non-LTE, V-T collisional transfer",
author = "Shved, {Gustav M.} and Khvorostovskaya, {Lyudmila E.} and Potekhin, {Igor Yu} and Ogibalov, {Vladimir P.} and Uzyukova, {Tatyana V.}",
year = "2002",
month = dec,
day = "1",
doi = "10.1117/12.463371",
language = "English",
volume = "4882",
pages = "106--116",
journal = "Proceedings of SPIE - The International Society for Optical Engineering",
issn = "0277-786X",
publisher = "SPIE",
note = "Remote Sensing of Clouds and the Atmosphere VII ; Conference date: 24-09-2002 Through 27-09-2002",

}

RIS

TY - JOUR

T1 - Measurement of rate constant for quenching CO2(0110) by atomic oxygen at low temperatures

T2 - Remote Sensing of Clouds and the Atmosphere VII

AU - Shved, Gustav M.

AU - Khvorostovskaya, Lyudmila E.

AU - Potekhin, Igor Yu

AU - Ogibalov, Vladimir P.

AU - Uzyukova, Tatyana V.

PY - 2002/12/1

Y1 - 2002/12/1

N2 - The paper presents the first laboratory measurement of the rate constant for quenching the CO2(0110) state during collisions of CO2 molecules with O atoms at temperatures realized near the Earth's mesopause. The measurement was carried out with a hollow-cathode glow discharge in the temperature range 206-358 K. The measured values are significantly smaller than those commonly used in solving the non-LTE CO2 problem for the vibrational states of the mode v2 in the atmospheres of the Earth, Venus, and Mars. The measured temperature dependence of the rate constant is approximated by a simple relation, which is recommended for solving the above problem. The value of this rate constant is absolutely critical to remotely sense temperature, and hence also constituent densities, in the upper mesosphere and lower thermosphere of the Earth. The use of the new values of the rate constant significantly decreased the rate of cooling by the CO 2 15-μm emission in the terrestrial lower thermosphere as compared to the previous estimates obtained for this rate. Over the most area of the Earth's surface, the maximum cooling rate occurs at an altitude of about 110 km and amounts to about 20 K/day.

AB - The paper presents the first laboratory measurement of the rate constant for quenching the CO2(0110) state during collisions of CO2 molecules with O atoms at temperatures realized near the Earth's mesopause. The measurement was carried out with a hollow-cathode glow discharge in the temperature range 206-358 K. The measured values are significantly smaller than those commonly used in solving the non-LTE CO2 problem for the vibrational states of the mode v2 in the atmospheres of the Earth, Venus, and Mars. The measured temperature dependence of the rate constant is approximated by a simple relation, which is recommended for solving the above problem. The value of this rate constant is absolutely critical to remotely sense temperature, and hence also constituent densities, in the upper mesosphere and lower thermosphere of the Earth. The use of the new values of the rate constant significantly decreased the rate of cooling by the CO 2 15-μm emission in the terrestrial lower thermosphere as compared to the previous estimates obtained for this rate. Over the most area of the Earth's surface, the maximum cooling rate occurs at an altitude of about 110 km and amounts to about 20 K/day.

KW - Atmospheric infrared emission

KW - Hollow-cathode glow discharge

KW - Non-LTE

KW - V-T collisional transfer

UR - http://www.scopus.com/inward/record.url?scp=0041730196&partnerID=8YFLogxK

U2 - 10.1117/12.463371

DO - 10.1117/12.463371

M3 - Conference article

AN - SCOPUS:0041730196

VL - 4882

SP - 106

EP - 116

JO - Proceedings of SPIE - The International Society for Optical Engineering

JF - Proceedings of SPIE - The International Society for Optical Engineering

SN - 0277-786X

Y2 - 24 September 2002 through 27 September 2002

ER -

ID: 39862527