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Published June 2006 | Published + Supplemental Material
Journal Article Open

On the stratospheric chemistry of hydrogen cyanide

Abstract

HCN profiles measured by solar occultation spectrometry during 10 balloon flights of the JPL MkIV instrument are presented. The HCN profiles reveal a compact correlation with stratospheric tracers. Calculations with a 2D-model using established rate coefficients for the reactions of HCN with OH and O(^1D) severely underestimate the measured HCN in the middle and upper stratosphere. The use of newly available rate coefficients for these reactions gives reasonable agreement of measured and modeled HCN. An HCN yield of ∼30% from the reaction of CH_3CN with OH is consistent with the measurements.

Additional Information

© 2006 American Geophysical Union. Received 9 February 2006; revised 30 March 2006; accepted 24 April 2006; article first published online 3 June 2006. We would like to thank the various launch crews for conducting the balloon flights, and D. Petterson and J. Landeros of JPL for their excellent support prior and during the measurement campaigns. Work at AER was supported by the NASA ACMAP program. Work at Georgia Tech was supported by the NASA UARP program. Work at Jet Propulsion Laboratory, California Institute of Technology, was performed under a contract with the National Aeronautics and Space Administration. Please note: Wiley Blackwell is not responsible for the content or functionality of any supporting information supplied by the authors. Any queries (other than missing content) should be directed to the corresponding author for the article.

Attached Files

Published - grl21441.pdf

Supplemental Material - grl21441-sup-0001-readme.txt

Supplemental Material - grl21441-sup-0002-ts01.txt

Supplemental Material - grl21441-sup-0003-fs01.eps

Supplemental Material - grl21441-sup-0004-fs02.eps

Supplemental Material - grl21441-sup-0005-t01.txt

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Additional details

Created:
August 22, 2023
Modified:
October 26, 2023