In 1780, the famous English chemist Joseph Priestley (right) found that plants could "restore air which has been injured by the burning of candles." He.

Slides:



Advertisements
Similar presentations
STRATOSPHERIC OZONE DISTRIBUTION Marion Marchand CNRS-UPMC-IPSL.
Advertisements

Copyright © 2010 R. R. Dickerson & Z.Q. Li 1 AOSC 620 The Ozone Hole R. Dickerson.
Chemistry in the Atmosphere Chapter 17 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
The Stratospheric Chemistry and The Ozone Layer
PowerPoint ® Lecture prepared by Gary A. Beluzo A REDUCTION IN ATMOSPHERIC OZONE Let the Sunshine In 14.
OZONE Stratospheric Tropospheric Summary Basics Issues ©2003, Perry Samson, University of Michigan The good, the bad & the ugly.
METO 621 CHEM Lesson 2. The Stratosphere We will now consider the chemistry of the troposphere and stratosphere. There are two reasons why we can separate.
CHAPTER 10: STRATOSPHERIC CHEMISTRY. THE MANY FACES OF ATMOSPHERIC OZONE Troposphere Stratosphere: 90% of total In stratosphere: UV shield In middle/upper.
In 1780, the famous English chemist Joseph Priestley (right) found that plants could "restore air which has been injured by the burning of candles."
Photosynthesis.  Chlorophyll is the molecule that absorbs sunlight and uses its energy to synthesize carbohydrates from CO 2 and water.  This process.
Copyright © 2010 R. R. Dickerson & Z.Q. Li 1 AOSC 620 Ozone in the Stratosphere R. Dickerson Note material on layers in general will be covered in AOSC.
METO 637 Lesson 15. Polar meteorology In the winter months the poles are in perpetual darkness. This causes extremely cold temperatures in the stratosphere.
METO 621 Lesson 21. The Stratosphere We will now consider the chemistry of the troposphere and stratosphere. There are two reasons why we can separate.
Stratospheric Chemistry EPS March – 04 April 2011 Polar Stratospheric Clouds.
Skin cancer In 1780, the famous English chemist Joseph Priestley (right) found that plants could "restore air which has been injured by the burning.
Bay Area Earth Science Institute (BAESI)
METO 637 Lesson 9. Man’s impact on the Stratosphere The concern over a loss of stratospheric ozone is that this will lead to an increase in ultraviolet.
LIGHT Special topics. 1.Greenhouse effect 2.Ozone hole.
Chemistry of Ozone in the Stratosphere. Levels of stratospheric ozone have been dropping NASA -
CALCULATION OF PHOTOLYSIS RATES k is the photolysis rate constant (also called photolysis frequency or J-value) quantum yield absorption x-section actinic.
PHOTONS IN CHEMISTRY OUT. PHOTONS IN CHEMISTRY OUT WHY BOTHER?
CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930) O O 3 O2O2 slow fast Odd oxygen family [O x ] = [O 3 ] + [O] R2 R3 R4 R1.
Meto 637 Lesson 11. The Ozone Hole Antarctic total ozone.
Typical mixing ratios for some compounds of environmental importance.
Solar and Terrestrial Radiation
Chapter 12a Chemical Reactions
The Ozone Layer. Importance Ozone, O 3, shields the earth’s surface from biologically harmful UV-B radiation, which damages the genetic information in.
QUESTIONS Based on the major source of OH described last class where do you expect OH formation to be high? 2. The  Chapman mechanism includes a fifth.
Stratospheric Ozone (con’t): Production, Destruction, & Trends Antarctic Ozone Hole: Sept. 12, 2012.
Copyright©2000 by Houghton Mifflin Company. All rights reserved. 1 Chemistry FIFTH EDITION Chapter 5 Gases.
Section  Area in the stratosphere where ozone is highly concentrated  Ozone: 3 atoms of oxygen (O3)  Absorbs most of the harmful ultraviolet.
QUESTIONS 1.Based on the major source of OH described last class where do you expect OH formation to be high? 2.Why don’t reactions of hydrocarbons deplete.
IV. Ozone Hole Observations Heterogeneous chemistry Decadal ozone loss.
Ozone Depletion. The Ozone “Hole” …What is it? Schematic of the North-to-South Ozone Depletion: courtesy NOAA equator.
CHEM /10/12 I.B. Stratospheric chemistry: Ozone - The Chapman Mechanism - cont. Embedded Fundamentals - Photochemistry  KEEP READING CH 1  HW#3.
© 2012 W. H. Freeman & Co.. Skin cancer © 2012 W. H. Freeman & Co.
Atmospheric Chemistry. Stratospheric Ozone 1) Absorbs solar radiation ( nm) 2) Three types of UV UV-A ( ) UV-A ( ) UV-B ( nm)
7. Ozone hole 1)Structure of the ozone layer 2) Chemistry of the natural ozone layer 3)Recent changes to the ozone layer 4)Effects of Chlorine on global.
1974 Sherwood Rowland & Mario Molina Calculated that CFCs were lowering the average concentration of Ozone in the stratosphere. Chemical Time Bomb: Spray.
Environmental chemistry
News _officials_urge_halving_of_phosphorous_levels_in_upper_middle_c harles_river/
Chapman Mechanism (~1930, Sidney Chapman) O 2 + h  O + O (

13-2 The Ozone Shield Page 335.
Copyright © 2010 R. R. Dickerson & Z.Q. Li 1 AOSC 620 Ozone in the Stratosphere R. Dickerson Note material on layers in general will be covered in AOSC.
Damaging the Ozone Layer
History of Ozone Discovered in 1840 by Christian Friedrich Schönbein. In the 1920’s Gordon Dobson made the first O 3 column measurements. 1 DU = 1x10 -3.
Atmosphere Layers. Vertical Structure of the Earth’s Atmosphere Vertical temperature (T) profile: troposphere stratosphere mesosphere Thermosphere (contains.
News _officials_urge_halving_of_phosphorous_levels_in_upper_middle_c harles_river/
Atmospheric Chemistry of the Ozone Layer. Levels of Atmospheric Ozone have been Dropping NASA -
Biogeochemical Rx in Troposphere Trace biogenic gases (NO, NO 2, N 2 O, CH 4, SO 2 ) more Rx than major constituents (N 2, O 2, Ar) NITROGEN & SULFUR Ozone.
Chapter 1 Ingredients of Change: Functions and Models.
Chapter 26 Ozone Depletion. Ozone A form of oxygen in which three atoms of oxygen occur together. Chemically active and has a short average lifetime in.
News mix/TNjKKIEJaaKm6ZNwwDxqhN/story.html
Ozone depletion today – introduction and ozone chemistry
Chloromonoxide
Advanced Placement Environmental Science Teacher
ATS 621 Fall 2012 Lecture 11.
ATS 621 Fall 2012 Lecture 9.
Chemistry of Ozone in the Stratosphere.
Zumdahl Zumdahl DeCoste
ATS 621 Fall 2012 Lecture 10.
A tour of the ozone hole Courtesy of the Centre for Atmospheric Sciences, Cambridge University and plus Claire Cosgrove and Peter Webster.
Spectroscopy and Photochemistry
Chemistry in the Atmosphere
Spectroscopy Copyright © Houghton Mifflin Company. All rights reserved.
The Ozone Shield 13.2.
The Ozone Shield 13.2.
mass of the atmosphere: 5 x kg <0.1% <1%
Chemistry in the Atmosphere
Presentation transcript:

In 1780, the famous English chemist Joseph Priestley (right) found that plants could "restore air which has been injured by the burning of candles." He used a mint plant, and placed it into an upturned glass jar in a vessel of water for several days. He then found that "the air would neither extinguish a candle, nor was it all inconvenient to a mouse which I put into it". In other words, he discovered that plants produce oxygen. A few years later, in 1794, the French chemist Antoine Lavoisier (left), discovered the concept of oxidation, but soon after was executed during the French Revolution for being a Monarchist sympathiser. The judge who pronounced sentence said "The Republic has no need for scientists".

mass of the atmosphere: 5 x kg

Fast vertical mixing Mixing across tropopause is slow Fast vertical mixing Direct interface with surface T  w/ altitude (adiabatic lapse rate) Rapid vertical mixing High T because of: high E of bomb. radiation Slow vertical mixing T  w/ altitude because of h abs. by O 3 T  w/ altitude because h abs. by O 3 less important

© 2012 W. H. Freeman & Co.

Skin cancer

© 2012 W. H. Freeman & Co.

14a–13

(wavelength) x (frequency) = speed λν = c [3x10 8 m/s]

E = h ν h = 6.6 x J.s Light as particles or photons With energy, E, proportional to frequency, ν

=

~ nm Take 500 nm

Copyright © Houghton Mifflin Company. All rights reserved. 14a–23 Electromagnetic spectrum λ ν

E = h ν

Chapman Mechanism (~1930, Sidney Chapman) O 2 + h  O + O 498 kJ/mol  <242.4 nm O + O 2 + M  O 3 + M O 3 + h  O + O kJ/mol  <280 nm

Chapman Mechanism (~1930, Sidney Chapman) O 2 + h  O + O 498 kJ/mol  <242.4 nm O + O 2 + M  O 3 + M O 3 + h  O + O kJ/mol  <280 nm

Chapman Mechanism (~1930, Sidney Chapman) O 2 + h  O + O 498 kJ/mol  <242.4 nm O + O 2 + M  O 3 + M O 3 + h  O + O kJ/mol  <280 nm

Chapman Mechanism (~1930, Sidney Chapman) O 2 + h  O + O 498 kJ/mol  <242.4 nm O + O 2 + M  O 3 + M O 3 + h  O + O kJ/mol  <280 nm O + O 3  2O 2 O + O + M  O 2 + M

Ozone production λ ≤ 240 nm λ ≤ 280 nm h h Ozone destruction

© 2012 W. H. Freeman & Co.

λ ≥ 280 nm

1 Dobson unit (DU) is: 0.01 mm of pure O 3 at 1 atm. and 0 o C NB: what does 300 DU expand to at atm?

Ozone production Photochemical kinetics λ ≤ 240 nm λ ≤ 280 nm h h WRONG EQUILIBRIUM: TOO MUCH OZONE

Chlorine reservoirs © 2012 W. H. Freeman & Co.

Chlorine reservoirs © 2012 W. H. Freeman & Co.

Recipe for ozone loss: 1.POLAR WINTER  Polar vortex  Isolates air 2.LOW TEMPERATURE  PSC (=Polar Stratospheric Clouds) (=Nitric acid – HNO 3 ) 3.SURFACE CHEMISTRY  Cl 2 (+denoxification) 4.LIGHT RETUNS  Cl*  Catalytic destruction of O 3

Catalytic Decomposition of Ozone X + O 3  XO + O 2 XO + O  X + O 2 _____________________________ O 3 + O  2O 2 X = HO x (  H,  OH, HOO  ) NO x (NO ,  NO 2 ) ClO x (  Cl, ClO  )

CHAPTER 02: Figure 2.1 © 2012 W. H. Freeman & Co.

CHAPTER 02: Figure 2.2 © 2012 W. H. Freeman & Co.

NASA projections of stratospheric ozone concentrations if chlorofluorocarbons had not been banned.

Mount manitoba, June 1991

CHAPTER 02: Figure 2.10 © 2012 W. H. Freeman & Co.

PrefixMeaningAtoms in the Molecule CFCchlorofluorocarbonCl, F, C HCFChydrochlorofluorocarbonH, Cl, F, C HBFChydrobromofluorocarbonH, Br, F, C HFChydrofluorocarbonH, F, C HChydrocarbonH, C PFCperfluorocarbonF, C HalonN/A Br, Cl (in some but not all), F, H (in some but not all), C

© 2012 W. H. Freeman & Co.