Ultra-violet absorption cross sections of isotopically substituted nitrous oxide species: <sup>14</sup>N<sup>14</sup>NO, <sup>15</sup>N<sup>14</sup>NO, <sup>14</sup>N<sup>15</sup>NO and <sup>15</sup>N<sup>15</sup>NO
The isotopically substituted nitrous oxide species <sup>14</sup>N<sup>14</sup>NO, <sup>15</sup>N<sup>14</sup>NO, <sup>14</sup>N<sup>15</sup>NO and <sup>15</sup>N<sup>15</sup>NO were investigated by ultra-...
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doaj-6fe41deebf494940ae0c8e356d169f0b2020-11-24T21:20:01ZengCopernicus PublicationsAtmospheric Chemistry and Physics1680-73161680-73242004-01-014512371253Ultra-violet absorption cross sections of isotopically substituted nitrous oxide species: <sup>14</sup>N<sup>14</sup>NO, <sup>15</sup>N<sup>14</sup>NO, <sup>14</sup>N<sup>15</sup>NO and <sup>15</sup>N<sup>15</sup>NOP. von HessbergJ. KaiserJ. KaiserM. B. EnghoffC. A. McLindenS. L. SorensenT. RöckmannM. S. JohnsonThe isotopically substituted nitrous oxide species <sup>14</sup>N<sup>14</sup>NO, <sup>15</sup>N<sup>14</sup>NO, <sup>14</sup>N<sup>15</sup>NO and <sup>15</sup>N<sup>15</sup>NO were investigated by ultra-violet (UV) absorption spectroscopy. High precision cross sections were obtained for the wavelength range 181 to 218nm at temperatures of 233 and 283K. These data are used to calculate photolytic isotopic fractionation constants as a function of wavelength. The fractionation constants were used in a three-dimensional chemical transport model in order to simulate the actual fractionation of N<sub>2</sub>O in the stratosphere, and the results were found to be in good agreement with field studies.http://www.atmos-chem-phys.net/4/1237/2004/acp-4-1237-2004.pdf |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
P. von Hessberg J. Kaiser J. Kaiser M. B. Enghoff C. A. McLinden S. L. Sorensen T. Röckmann M. S. Johnson |
spellingShingle |
P. von Hessberg J. Kaiser J. Kaiser M. B. Enghoff C. A. McLinden S. L. Sorensen T. Röckmann M. S. Johnson Ultra-violet absorption cross sections of isotopically substituted nitrous oxide species: <sup>14</sup>N<sup>14</sup>NO, <sup>15</sup>N<sup>14</sup>NO, <sup>14</sup>N<sup>15</sup>NO and <sup>15</sup>N<sup>15</sup>NO Atmospheric Chemistry and Physics |
author_facet |
P. von Hessberg J. Kaiser J. Kaiser M. B. Enghoff C. A. McLinden S. L. Sorensen T. Röckmann M. S. Johnson |
author_sort |
P. von Hessberg |
title |
Ultra-violet absorption cross sections of isotopically substituted nitrous oxide species: <sup>14</sup>N<sup>14</sup>NO, <sup>15</sup>N<sup>14</sup>NO, <sup>14</sup>N<sup>15</sup>NO and <sup>15</sup>N<sup>15</sup>NO |
title_short |
Ultra-violet absorption cross sections of isotopically substituted nitrous oxide species: <sup>14</sup>N<sup>14</sup>NO, <sup>15</sup>N<sup>14</sup>NO, <sup>14</sup>N<sup>15</sup>NO and <sup>15</sup>N<sup>15</sup>NO |
title_full |
Ultra-violet absorption cross sections of isotopically substituted nitrous oxide species: <sup>14</sup>N<sup>14</sup>NO, <sup>15</sup>N<sup>14</sup>NO, <sup>14</sup>N<sup>15</sup>NO and <sup>15</sup>N<sup>15</sup>NO |
title_fullStr |
Ultra-violet absorption cross sections of isotopically substituted nitrous oxide species: <sup>14</sup>N<sup>14</sup>NO, <sup>15</sup>N<sup>14</sup>NO, <sup>14</sup>N<sup>15</sup>NO and <sup>15</sup>N<sup>15</sup>NO |
title_full_unstemmed |
Ultra-violet absorption cross sections of isotopically substituted nitrous oxide species: <sup>14</sup>N<sup>14</sup>NO, <sup>15</sup>N<sup>14</sup>NO, <sup>14</sup>N<sup>15</sup>NO and <sup>15</sup>N<sup>15</sup>NO |
title_sort |
ultra-violet absorption cross sections of isotopically substituted nitrous oxide species: <sup>14</sup>n<sup>14</sup>no, <sup>15</sup>n<sup>14</sup>no, <sup>14</sup>n<sup>15</sup>no and <sup>15</sup>n<sup>15</sup>no |
publisher |
Copernicus Publications |
series |
Atmospheric Chemistry and Physics |
issn |
1680-7316 1680-7324 |
publishDate |
2004-01-01 |
description |
The isotopically substituted nitrous oxide species <sup>14</sup>N<sup>14</sup>NO, <sup>15</sup>N<sup>14</sup>NO, <sup>14</sup>N<sup>15</sup>NO and <sup>15</sup>N<sup>15</sup>NO were investigated by ultra-violet (UV) absorption spectroscopy. High precision cross sections were obtained for the wavelength range 181 to 218nm at temperatures of 233 and 283K. These data are used to calculate photolytic isotopic fractionation constants as a function of wavelength. The fractionation constants were used in a three-dimensional chemical transport model in order to simulate the actual fractionation of N<sub>2</sub>O in the stratosphere, and the results were found to be in good agreement with field studies. |
url |
http://www.atmos-chem-phys.net/4/1237/2004/acp-4-1237-2004.pdf |
work_keys_str_mv |
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