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Atmospheric chemistry Lecture 2: Photochemistry & kinetics Dr. David Glowacki University of Bristol,UK

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Presentation on theme: "Atmospheric chemistry Lecture 2: Photochemistry & kinetics Dr. David Glowacki University of Bristol,UK"— Presentation transcript:

1 Atmospheric chemistry Lecture 2: Photochemistry & kinetics Dr. David Glowacki University of Bristol,UK

2 Quick review of yesterday We discussed atmospheric structure Temperature & pressure gradients, as well as Coriolis forces are related to atmospheric transport Today… Well gain some insight into the relationship between atmospheric structure and atmospheric chemistry Atmospheric chemistry depends on sunlight, temperature, and pressure; Today well learn about Photochemistry Chemical kinetics

3 The Atmosphere is a low temperature chemical reactor Troposphere Stratosphere Tropopause -70 o C 14 km O 3 layer UV visible Urban Anthropogenic emissions Surface O 3 Regional and global biogenic emissions (CH 4 ) Important Chemistry : UV absorption by O 3 IR absorption by Greenhouse gases (H 2 O, CH 4, CO 2 ) Surface emissions resulting in O 3 and aerosol formation, and acid rain

4 Atmospheric Chemistry starts with sunlight E = hv Breaking chemical bonds requires energy Sunlight has energy If sufficient energy is deposited in the bond, then it will break O 3 has a bond energy of ~105 kJ mol -1 v = c/ Energy/kJ mol -1 Red700170 Orange620190 Yellow580210 Green530230 Blue470250 Violet420280 Near UV400-200300-600 Far UV200-50600-2400 visible

5 Photoexcitation gives excited molecules, A* Initial photoexcitation Dissociation Fluorescence Collisional relaxation Ionization Photoexcitation may result in a number of processes: Photochemistry depends on temperature, pressure, and the wavelength of the absorbed light *

6 Photoexcitation kinetics The rate of formation of A* is written: where j A is the photochemical rate constant Competition between subsequent processes is determined by the quantum yield, ϕ, for each process where: Dissociation yield =Φ 1 Fluorescence yield =Φ 2 Collisional relaxation yield =Φ 3 Ionization =Φ 4

7 Understanding the photolysis rate absorption cross section: number of photons absorbed by a molecule at a particular wavelength Spectral actinic flux: density of photons in the atmosphere at a particular wavelength Quantum yield: efficiency at which absorbed photons result in the molecular process of interest need to integrate over the entire wavelength range

8 Understanding photolysis rates Atmospheric actinic flux Photochemical processes depend on: temperature (absorption cross sections & quantum yields) Pressure (collisional relaxation) Altitude (actinic flux) O 3 absorption cross section

9 Atmospheric absorption of light Gases absorb light The absorption of light depends on the concentration of the gas, N, its absorption cross section, σ, & the path length, l, through the gas May be described by the Beer- Lambert law

10 Atmospheric absorption of light The Beer Lambert law: Explains the altititude dependence of actinic flux Is often used to measure atmospheric trace gas concentrations DOAS (differential optical absorption spectrometry) FTIR spectrometry

11 Chemical Kinetics

12 Kinetics depends on the potential energy surface (PES) What molecules do is determined by their potential energy landscapes – energy as a function of coordinates Stable molecules are minima on a PES Potential energy surfaces (PES) are multidimensional, but we usually think about their motion projected in one dimension T dependence of reaction rate coefficients well described by the Arrhenius equation:

13 First order Unimolecular kinetics

14 Mechanisms with more than one chemical reactions: exact solutions Coupled chemical reactions, often result in mechanisms of the sort: For this system we can write three rate equations, one for each species: A B k1k1 k2k2 B C In matrix form:

15 Chemical Mechanisms with Coupled Chemical Reactions: Coupled differential Equations Analytic solutions exist for this eigenvalue problem to solve for concentration vs. time If the initial concentration of every species but [A] is zero, the solutions are Concentration vs time when k 2 /k 1 =10 B changes a lot; Not low or constant Concentration vs time when k 2 /k 1 =0.5 B doesnt change much Low and ~constant

16 Consider again the following mechanism: Steady state approximation: assume the rate of change of intermediate B is zero A B k1k1 k2k2 B C Chemical Mechanisms with Coupled Chemical Reactions: Steady State Approximation Equivalent when k 2 >> k 1 making [B] low & ~constant Approximate Steady state solution Exact solution

17 Chemical Lifetimes Often we are interested in the average lifetime of a molecule before it reacts away Lifetime has units of time The interplay between chemical lifetimes and atmospheric mixing processes determines much of atmospheric chemistry A B k1k1 k2k2 B C

18 Collision Theory Molecules are constantly moving Molecular gases are constantly colliding with each other with a T & P dependent collision frequency Each collision has a particular amount of energy associated with it This energy may lead to chemical reaction Threshold energy

19 Bimolecular Kinetics Atmospheric chemistry involves both unimolecular and bimolecular processes Bimolecular kinetics depend on pressure, [M] A reasonable model for a bimolecular reaction is

20 Visualizing bimolecular pressure dependence: O + O 2 + M O 3 + M O + O 2 reaction coordinate O OO M M = O 2 or N 2 O3O3

21 Bimolecular Kinetics: The Low & High pressure Limits The total bimolecular process: Assume AB* is in steady state Solve for AB* and plug into the first equation Write rate equations for AB* We want to know the rate of AB formation

22 Bimolecular Kinetics: The Low & High pressure Limits Low Pressure Limit –[M] is very small –k 4 >> k 5 [M] –k 5 [M] goes to zero –Overall reaction rate depends linearly on [M] High Pressure Limit –[M] is very large –k 4 << k 5 [M] –k 4 goes to zero –Overall reaction rate is independent of [M] –Instantaneous stabilization

23 T & P dependent kinetic effects Laboratory measurements of rate coefficients give rise to T & P dependences which are well described by the kinetic master equation

24 Quick Summary Atmospheric chemistry dominated by photolysis Molecular motion on a potential energy surface (PES) determines reactivity In the atmosphere, simple reactions combine to form kinetic networks (i.e., coupled sets of important reactions) The steady state approximation is a useful simplification for short lifetimes Chemical reactions depend on both pressure & temperature, and are determined through a combination of experimental & theoretical approaches

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