Due to the implication of iodine chemistry in stratospheric ozone
depletion, an accurate atmospheric lifetime
of methyl iodide has recently become of interest. To calculate
this lifetime, a reliable temperature-dependent
UV photodissociation cross section, in the region that overlaps with
available solar light, is vital. Unfortunately,
measurement of this cross section is complicated by the fact that, at
typical laboratory pressures, methyl
iodide readily forms dimers whose ultraviolet absorption differs from
that of the monomer and that dimer
formation is also temperature-dependent. We use a combination of
theory and experiment to separate the
changes in the absorption due to the temperature dependence of dimer
formation from the narrowing of the
absorption band that results from rotational and vibrational cooling of
isolated methyl iodide molecules.
Calculation of the predicted absorption cross section shows that
the valence band absorption spectrum narrows
only slightly upon cooling from 25 to −73 °C (200 K).
Absorption spectra were also measured experimentally
at a range of pressures from 0.1 to 2.4 Torr and a range of
temperatures from −22 to 100 °C. The temperature-dependent cross section measured at 0.1 Torr agrees well with the
calculated temperature dependence. The
spectra at higher pressures show strong pressure as well as temperature
dependence. This pressure dependence
allowed us to constrain the temperature-dependent equilibrium constant
for dimer formation.