Published June 16, 2000
| Version Published
Journal Article
Open
Intensity of the second and third OH overtones of H_2O_2, HNO_3, and HO_2NO_2
Abstract
The 3ν_(OH) and 4ν_(OH) of H_2O_2, HNO_3, and HO_2NO_2 have been observed. The band strengths of 3ν_(OH) are (7.0±1.8) × 10^(−20), (2.9±0.7) × 10^(−20), and (3.8±1.1) × 10^(−20) cm^2 molecules^(−1) cm^(−1) for H_2O_2, HNO_3, and HO_2NO_2, respectively. Those of 4ν_(OH) are (4.5± .6) × 10^(−21), (2.8± .0) × 10^(−21), and (3.0±1.8) × 10^(−21) cm^2 molecules^(−1) cm^(−1) for H_2O_2, HNO_3, and HO_2NO_2, respectively. The uncertainty is for one standard deviation. Assuming excitation of these modes by solar absorption is dissociative for HO_2NO_2, these measurements confirm that this process will play a small role in the atmospheric photochemistry of the lower stratosphere.
Additional Information
© 2000 American Geophysical Union. Received November 23, 1999; revised February 9, 2000; accepted February 11, 2000. Paper number 2000JD900118. This work is partly supported by NASA grant SA98-0055. We thank R.J. Salawitch for help on the HO_2NO_2 photolysis rate calculations. Useful communications with D. J. Donaldson are greatly appreciated.Attached Files
Published - jgrd7492.pdf
Files
jgrd7492.pdf
Additional details
Additional titles
- Alternative title
- Intensity of the second and third OH overtones of H2O2, HNO3, and HO2NO2
Identifiers
- Eprint ID
- 46496
- Resolver ID
- CaltechAUTHORS:20140625-075632457
Funding
- NASA
- SA98-0055
Dates
- Created
-
2014-06-25Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field
Caltech Custom Metadata
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)