z-logo
open-access-imgOpen Access
Temperature dependence of UV absorption cross sections and atmospheric implications of several alkyl iodides
Author(s) -
Roehl Coleen M.,
Burkholder James B.,
Moortgat Geert K.,
Ravishankara A. R.,
Crutzen Paul J.
Publication year - 1997
Publication title -
journal of geophysical research: atmospheres
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/97jd00530
Subject(s) - absorption spectroscopy , photodissociation , absorption (acoustics) , analytical chemistry (journal) , solar zenith angle , alkyl , spectral line , chemistry , bromine , zenith , reaction rate constant , wavelength , materials science , photochemistry , optics , physics , kinetics , atmospheric sciences , optoelectronics , organic chemistry , astronomy , composite material , chromatography , quantum mechanics
The ultraviolet absorption spectra of a number of alkyl iodides which have been found in the troposphere, CH 3 I, C 2 H 5 I, CH 3 CH 2 CH 2 I, CH 3 CHICH 3 , CH 2 I 2 , and CH 2 ClI, have been measured over the wavelength range 200–380 nm and at temperatures between 298 and 210 K. The absorption spectra of the monoiodides CH 3 I, C 2 H 5 I, CH 3 CH 2 CH 2 I, and CH 3 CHICH 3 are nearly identical in shape and magnitude and consist of single broad bands centered near 260 nm. The addition of a chlorine atom in CH 2 ClI shifts its spectrum to longer wavelengths (σ max at 270 nm). The spectrum of CH 2 I 2 is further red‐shifted, reaching a maximum of 3.85×10 −18 cm 2 molecule −1 at 288 nm and exhibiting strong absorption in the solar actinic region, λ>290 nm. Atmospheric photolysis rate constants, J values, have been calculated assuming quantum efficiencies of unity for different solar zenith angles as a function of altitude using the newly measured cross sections. Surface photolysis rate constants, calculated from the absorption cross sections measured at 298 K, range from 3×10 −6 s −1 for CH 3 I to 5×10 −3 s −1 for CH 2 I 2 at a solar zenith angle of 40°.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom