Kinetic studies of the gas phase
I2/O3 photochemistry
Juan Carlos Gomez Martin
IUP
27.05.2005, 13.00 c.t.
Room S3120
The evaluation of the relevance of tropospheric iodine chemistry in O3
depleting cycles and in aerosol formation requires a previous understanding of
the kinetics and mechanisms involved. In order to compile such information, the
chemical system generated by flash photolysis of I2 in the presence
of O3 has been studied by using multichannel time-resolved molecular
absorption spectroscopy and atomic resonance absorption spectroscopy.
This system was previously used to determine absolute absorption cross
sections of IO, IO*, OIO and higher iodine oxides (see Peter Spietz thesis), and
as a result of this work the time dependent concentration curves of relevant gas
phase species are known. These data have been analysed to derive a mechanism
which enables to explain:
-Pressure dependence of the branching ratios of the IO self reaction: the I and
OIO yields are relevant in order to determine the ozone destroying potential and
the particle formation potential of the IO self reaction.
-Fate of OIO and I2O2: the homogeneous aerosol nucleation
observed in the MBL. The reaction rates of the reactions considered are obtained
by integrating the corresponding set of differential rate equations and by
applying optimisation methods.
In this work the reactions IO+OIO+M->I2O3+M and
OIO+OIO->I2O4+M are proposed as the most plausible paths
to higher iodine oxides and aerosol formation. Modelling studies performed at
the UEA (Norwich) considering rate constants calculated in the context this work
are able to reproduce the ammounts of OIO and 'new particles' observed in Mace
Head. Theoretical calculations using RRKM Theory fit our experimentally
determined presure dependent branching ratios and rate constants very well.