Topic # 15 OZONE DEPLETION IN THE STRATOSPHERE. see pp in Class Notes

Similar documents
Topic # 14 OZONE DEPLETION IN THE STRATOSPHERE

Topic # 13 (cont.) OZONE DEPLETION IN THE STRATOSPHERE Part II

Average Temperature Readings at Various Altitudes

Science 1206 Unit 2: Weather Dynamics Worksheet 8: Layers of the Atmosphere

Today s AZ Daily Star has 2 interesting articles: one on our solar future & the other on an issue re: our state-mandated energy-efficiency plan

Topic # 6 ATMOSPHERIC STRUCTURE & CHEMICAL COMPOSITION Part II. Plus wrap up of some other topics

SIT IN YOUR GROUP AREA TODAY!

WRAP UP OF TOPIC #6. Fire up your CLICKERS for some questions to solidify the concepts from the last few classes:

The gases: gases: H2O O and What What are The two two most most abundant gases The The two two most most abundant abundant Greenhouse

TOPIC # 7 The RADIATION LAWS

Ozone: Earth s shield from UV radiation

Introduction to Electromagnetic Radiation and Radiative Transfer

CHEM/ENVS 380 S14, Midterm Exam ANSWERS 1 Apr 2014

We re about to play: PSUEDO-JEOPARDY!!!!! (Aka The Answer Is... ) It will refresh your memories about some of the key concepts we ve covered.

- matter-energy interactions. - global radiation balance. Further Reading: Chapter 04 of the text book. Outline. - shortwave radiation balance

Monday Sep 21st SIT ANYWHERE TODAY! Wrap-Up of Topic #5 on the Radiation Laws and start of Topic # 6 Atmospheric & Structure & Composition

OBJECTIVES: By the end of today s lesson, you will be able to. SWBAT list the layers of the atmosphere and describe the characteristics of each one.

Wednesday, September 8, 2010 Infrared Trapping the Greenhouse Effect

Atmospheric Structure

GE510 Physical Principles of the Envt

The Study of the Atmosphere

OZONE AND ULTRAVIOLET RADIATION

ATOC 3500/CHEM 3151 Air Pollution Chemistry Lecture 1

The Atmosphere. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems

Layers of the Atmosphere

GC 170A1 INTRO TO GLOBAL CHANGE MIDTERM STUDY GUIDE Fall 2014

Radiative equilibrium and vertical temperature profile

Lecture 14 - Radiative equilibrium and the atmospheric greenhouse effect

Common Elements: Nitrogen, 78%

Ozone in the Atmosphere

Chapter 2: Protecting the Ozone Layer

STRATOSPHERIC OZONE DEPLETION. Adapted from K. Sturges at MBHS

Lecture # 04 January 27, 2010, Wednesday Energy & Radiation

Our Atmosphere as seen from the bottom of it near Grand Pre, NS. Info modified from various sources by TWebb HHS

Spectrum of Radiation. Importance of Radiation Transfer. Radiation Intensity and Wavelength. Lecture 3: Atmospheric Radiative Transfer and Climate

Lecture 3: Atmospheric Radiative Transfer and Climate

Name Period Date L.O: SWBAT DESCRIBE THE PROPERTIES OF THE ATMOSPHERE.(

Topic # 13 (cont.) OZONE DEPLETION IN THE STRATOSPHERE Part II

Earth s Energy Balance and the Atmosphere

Radiation and the atmosphere

Let s Create a Little Atmosphere

WRAP UP OF TOPIC #5... ELECTROMANGETIC RADAITAION & THE ELECTROMAGNETIC SPECTRUM

Heating the Atmosphere (Chapter 14, with material from Chapter 2)

1. Radiative Transfer. 2. Spectrum of Radiation. 3. Definitions

Section 2: The Atmosphere

Unique nature of Earth s atmosphere: O 2 present photosynthesis

Lecture Outlines PowerPoint. Chapter 16 Earth Science 11e Tarbuck/Lutgens

Chapter 2 Protecting the Ozone Layer. The Ozone Hole

TOPIC # 6 The RADIATION LAWS

Atmosphere & Heat Transfer Basics Notes

Characteristics of the Atmosphere

Earth s Atmosphere. Composition

Characteristics of the Atmosphere

LECTURE 6 - THE EARTH'S ATMOSPHERE

AST 105 Intro Astronomy The Solar System

Tananyag fejlesztés idegen nyelven

ATM 507 Lecture 5. Text reading Chapter 4 Problem Set #2 due Sept. 20 Today s topics Photochemistry and Photostationary State Relation

UNIVERSITY OF VICTORIA CHEMISTRY 102 Midterm Test 1 January 31, pm (60 minutes) DISPLAY YOUR STUDENT ID CARD ON THE TOP OF YOUR DESK NOW

OBJECTIVES FOR TODAY S CLASS:

Radiation in the atmosphere

Atmospheric Layers. Ionosphere. Exosphere. Thermosphere. Mesosphere. Stratosphere. Troposphere. mi (km) above sea level 250 (400) 50 (80) 30 (50)

Thursday, November 1st.

Fundamentals of Atmospheric Radiation and its Parameterization

Ozone. In the upper atmosphere. At the surface pollution (not discussed)

Outline. Chemical lifetime. Photochemistry. Ozone chemistry Chapman model Catalytic cycles Ozone hole. Institute of Applied Physics University of Bern

Earth: the Goldilocks Planet

Lecture 5: Greenhouse Effect

TOPIC # 5 ELECTROMAGNETIC

General Astronomy (29:61) Fall 2012 Lecture 28 Notes, November 7, 2012

Lecture 5: Greenhouse Effect

Chapter 2: Protecting the Ozone Layer

I T A T I O N H B I T B T V A O C J K M R S A T M O S P H E R E

Outline. Stock Flow and temperature. Earth as a black body. Equation models for earth s temperature. Balancing earth s energy flows.

Atmospheric Radiation

Unit 3 Review Guide: Atmosphere

Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.

The greenhouse effect

Lecture 2 Global and Zonal-mean Energy Balance

Understanding the Greenhouse Effect

Discuss Yesterday s Lab. What Do We Know? Funny Ozone Video. Ozone Layer Defined! Ozone Layer. Warm-Up 3/3/2015

January 23, Lecture 3. The Ozone Chemistry.

EARTH'S ATMOSPHERE. 1. The graph below shows the average concentration of ozone in Earth's atmosphere over Arizona during 4 months of the year.

Chapter 2 Protecting the Ozone Layer

Topic # 10 THE EARTH S GLOBAL ENERGY BALANCE

5.5 (AIR PRESSURE) WEATHER

1. The frequency of an electromagnetic wave is proportional to its wavelength. a. directly *b. inversely

Teaching the Greenhouse Effect. Brian Hornbuckle and Ray Arritt

2. Sketch a plot of R vs. z. Comment on the shape. Explain physically why R(z) has a maximum in the atmospheric column.

Bring a printed copy of this lab to your lab section. We will answer the lettered questions in class.

). It is a gas produced naturally in the stratosphere where it strongly absorbs incoming

Planetary Atmospheres

Planetary Atmospheres

General Comments about the Atmospheres of Terrestrial Planets

ATMOSPHERE M E T E O R O LO G Y

LAB 3: Atmospheric Pressure & Moisture

Solar Variability and the Effects on the Earth s Atmosphere James Brenton Jerry Harder, Peter Pilewskie, Erik Richard Laboratory for Atmospheric and

Outline. Planetary Atmospheres. General Comments about the Atmospheres of Terrestrial Planets. General Comments, continued

Beer-Lambert (cont.)

Chapman Cycle. The cycle describes reactions of O 2 and O 3 in stratosphere

On Stationary state, also called steady state. Lifetimes and spatial scales of variability

Transcription:

Topic # 15 OZONE DEPLETION IN THE STRATOSPHERE see pp 81-85 in Class Notes

[ The Ozone Treaty is ] the first truly global treaty that offers protection to every single human being. ~ Mostofa K. Tolba, Director of the UN Environment Programme

OZONE STORY = A very interesting illustration of the scientific process! The THEORY that the ozone layer in the stratosphere might be damaged by human intervention PRECEDED the actual OBSERVATION of the ozone hole. Yet, when the hole WAS observed (via satellite) it was almost missed because it wasn t expected... But let s begin with the stratospheric ozone layer itself...... Key Concept

WHERE IS THE OZONE LAYER? SGC Fig. 3-11 Stratosphere Ozone Concentration (ppm)

OZONE: Sources Ozone is produced naturally in photochemical reactions in the stratospheric ozone layer -- good ozone -- is decreasing! However, ozone has increased in troposphere due to photochemical smog reactions -- bad ozone review

Here s a different version of the figure Shows 2 peaks, a major peak in O 3 density in the stratosphere, a smaller secondary peak in the lower troposphere Ozone Density (10 17 molecules / m 3) p 82

Bulk of ozone produced at ~ 25 km & drifts downward 22 km altitude peak Another lesser peak at ground level First we ll focus on the GOOD ozone located in the STRATOSPHERE (the ozone that is being depleted leading to an ozone hole )

THE OZONE LAYER IN THE STRATOSPHERE -- WHY IT'S THERE Due to: the natural Chapman Mechanism (a series of photochemical reactions)

THE CHAPMAN MECHANISM (first proposed in 1930s) ozone is continuously produced and destroyed through PHOTOCHEMICAL REACTIONS in the stratosphere involves oxygen (O 2 ), molecular oxygen (O), photons of UV radiation, and OZONE (O 3 ). Key Concept

The Chapman Mechanism [Go to movie clip] p 81

In theory: a balance of ozone is established over time > prevents much of the harmful UV radiation from reaching the earth's surface. Leads to an Equilibrium or Steady State Key Concept

STEADY STATE = a condition in which the STATE of a system component (e.g. reservoir) is CONSTANT over time.

Steady state can be achieved in a reservoir: a) if there are no inflows or outflows, or b) if the rate of inflow = the rate of outflow. Stratospheric ozone under steady state natural conditions Ozone reservoir Any imbalance in these rates leads to a change in the level of the reservoir.

FLOW DIAGRAM OF A STEADY STATE Inflow Ozone being formed via natural Chapman mechanism Reservoir of STRATOSPHERIC OZONE Outflow Ozone being destroyed via natural Chapman mechanism Where have we seen something like this before?

Review: Why stratospheric ozone is Good : Black areas = radiation absorbed Ozone has the property of being a very strong absorber of ultraviolet radiation nearly total absorption of wavelengths less than 0.3 m remember this absorption curve? p 81

Q4 What is the CORRECT completion to this sentence: The global change issue usually referred to as Stratospheric Ozone Depletion is related to the part of the absorption curve that is labeled. (1) X or (2) Y

Q4 What is the CORRECT completion to this sentence: The global change issue usually referred to as Stratospheric Ozone Depletion is related to the part of the absorption curve that is labeled. (1) X or (2) Y

Q5. Ok, X is right, but Why? 1.... because X represents UV radiation being absorbed -- hence if ozone is depleted, MORE ultraviolet radiation will reach the Earth s surface. 2.... because X represents terrestrial longwave radiation being absorbed -- and hence serves as a catalyst in the Chapman mechanism. 3....because X represents easy transmission of wavelengths of terrestrial longwave radiation out to space which then disappear through the atmospheric window also known as the ozone hole.

Q5. Ok, X is right, but Why? 1.... because X represents UV radiation being absorbed -- hence if ozone is depleted, MORE ultraviolet radiation will reach the Earth s surface. 2.... because X represents terrestrial longwave radiation being absorbed -- and hence serves as a catalyst in the Chapman mechanism. 3....because X represents easy transmission of wavelengths of terrestrial longwave radiation out to space which then disappear through the atmospheric window also known as the ozone hole.

From p. 40 in Class Notes: Temperature graph Ozone Density graph First sketch in tropopause & stratopause Now roughly sketch the temperature line from this graph onto the ozone graph p 82

TEMPERATURE [ increases / decreases ] with increasing altitude in the stratosphere WHY??? p 82

Q6. Why is there an increase in temperature with altitude in the STRATOSPHERE? 1. It is the closest layer to the sun, hence it is closest to the solar heat source. 2. It receives large amounts of UV radiation from the sun PLUS it has a high concentration of ozone to absorb this UV. 3. It is the layer which contains most of the GH gases that absorb IR radiation emitted by the Earth s surface.

Q6. Why is there an increase in temperature with altitude in the STRATOSPHERE? 1. It is the closest layer to the sun, hence it is closest to the solar heat source. 2. It receives large amounts of UV radiation from the sun PLUS it has a high concentration of ozone to absorb this UV. 3. It is the layer which contains most of the GH gases that absorb IR radiation emitted by the Earth s surface.

This is about where we ended... We ll finish up on THURSDAY before TEST #4!