WRAP UP: TOPIC #7 Atmospheric Structure & Composition

Similar documents
First some important preliminary business...

A few final review points to emphasize on: Topic #6 Atmospheric Structure & Composition...

Thursday Oct 2nd. A Study Session will be held from 4:30 5:30 pm Monday Oct 6th

Ready for some more SCIENCE Homer?

Ready for some more SCIENCE Homer?

Very Dynamic! Energy in the Earth s Atmosphere. How Does it Get Here? All Objects Radiate Energy!

Ready for some more SCIENCE Homer? ( Homer gives his brain a pep talk )

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 # 7 The RADIATION LAWS

The Kinetic Theory of Matter. Temperature. Temperature. Temperature. Temperature. Chapter 6 HEAT

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

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

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

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

Global Energy Balance: Greenhouse Effect

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

SIT IN YOUR GROUP AREA TODAY!

ATS150 Global Climate Change Spring 2019 Candidate Questions for Exam #1

Energy, Temperature, & Heat. Energy, Temperature, & Heat. Temperature Scales 1/17/11

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

Layer Protection Glossary

Temperature Scales

Bernoulli s Principle. Application: Lift. Bernoulli s Principle. Main Points 3/13/15. Demo: Blowing on a sheet of paper

Today. Events. Terrestrial Planet Geology - Earth. Terrestrial Planet Atmospheres. Homework DUE next time

AT 350 EXAM #1 February 21, 2008

Earth s Energy Budget: How Is the Temperature of Earth Controlled?

Greenhouse Effect. Julia Porter, Celia Hallan, Andrew Vrabel Miles, Gary DeFrance, and Amber Rose

Energy: Warming the earth and Atmosphere. air temperature. Overview of the Earth s Atmosphere 9/10/2012. Composition. Chapter 3.

Chapter 14 Temperature and Heat

Today. Events. Terrestrial Planet Atmospheres (continued) Homework DUE. Review next time? Exam next week

Lecture 2-07: The greenhouse, global heat engine.

CHEM 103: Chemistry in Context

Topic # 10 THE EARTH S GLOBAL ENERGY BALANCE

Investigating Planets Name: Block: E1:R6

ESS15 Lecture 7. The Greenhouse effect.

Period 13 Solutions: Earth as an Energy System

TOPIC # 6 The RADIATION LAWS

Name(s) Period Date. Earth s Energy Budget: How Is the Temperature of Earth Controlled?

To begin, enter your Footprint in Earths with you clicker...

Assessment Schedule 2017 Earth and Space Science: Demonstrate understanding of processes in the atmosphere system (91414)

Today. Work, Energy, Power loose ends Temperature Second Law of Thermodynamics

10/31/2017. Calculating the temperature of earth (The greenhouse effect) IR radiation. The electromagnetic spectrum

Mon Oct 20. Today: radiation and temperature (cont) sun-earth geometry energy balance >> conceptual model of climate change Tues:

Energy and Radiation. GEOG/ENST 2331 Lecture 3 Ahrens: Chapter 2

Agenda. Chapter 10, Problem 26. All matter is made of atoms. Atomic Structure 4/8/14. What is the structure of matter? Atomic Terminology

Academic Year First Term. Science Revision sheets PHYSICS

Conduction. Heat Transfer Methods. Conduction. Conduction

Recap. There are 3 different temperature scales: Celsius, Kelvin, and Fahrenheit

Table of Contents. Chapter: Atmosphere. Section 1: Earth's Atmosphere. Section 2: Energy Transfer in the Atmosphere. Section 3: Air Movement

PHYS:1200 LECTURE 18 THERMODYNAMICS (3)

Kinds of Energy. Defining Energy is Hard! EXPLAIN: 1. Energy and Radiation. Conservation of Energy. Sco; Denning CSU ESMEI ATS 1

Lecture 3: Light and Temperature

Archimedes Principle

Temperature. Temperature Scales. Temperature (cont d) CHAPTER 14 Heat and Temperature

Topic 6: Insolation and the Seasons


Planetary Atmospheres (Chapter 10)

Core Concepts. PowerPoint Lectures to accompany Physical Science, 8e. Chapter 4 Heat and Temperature. New Symbols for this Chapter 2/14/2011

Chapter: Heat and States

The last 2 million years.

1 Characteristics of the Atmosphere

ATOC 3500/CHEM 3151 Air Pollution Chemistry Lecture 1

Chapter 2. Heating Earth's Surface & Atmosphere

Tuesday Sep 9th ANNOUNCEMENTS. Assignment I-1 is due tonight before midnight (11:59 pm)

HEAT AND TEMPERATURE Vikasana-Bridge Course 2012

Directed Reading. Section: Solar Energy and the Atmosphere RADIATION. identical point on the next wave. waves

,Solar Energy, Greenhouse effect, Convection.notebook October 31, 2016

Chapter 9. Preview. Objectives Defining Temperature. Thermal Equilibrium. Thermal Expansion Measuring Temperature. Section 1 Temperature and

Chapter 2: The global ledger of radiation and heat

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.

Section 1: The Science of Energy¹

Chapter 21: Temperature, Heat and Expansion

What Is Air Temperature?

18.13 Review & Summary

The Earth is surrounded by a blanket of air, which we call the atmosphere. It reaches over 560 kilometers

Lecture 3. - Global Sulfur, Nitrogen, Carbon Cycles - Short-term vs. Long-term carbon cycle - CO 2 & Temperature: Last 100,000+ years

Section 2: The Atmosphere

Temperature, Heat, and Expansion

Chapter 14 Heat and Temperature Notes

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

* Defining Temperature * Temperature is proportional to the kinetic energy of atoms and molecules. * Temperature * Internal energy

Build Your Own Planet Lesson 4: Atmosphere

Atmosphere, Weather & Climate Review for Unit Assessment (Can be taken on Study Island Due Mon., 11/26/12)

Lecture 2: Zero law of thermodynamics

Climate Change Lecture Notes

International Conference on Climate Change natural greenhouse effect radiative transfer model

Introduction to Electromagnetic Radiation and Radiative Transfer

Earth s Atmosphere. Energy Transfer in the Atmosphere. 3. All the energy from the Sun reaches Earth s surface.

Radiative Balance and the Faint Young Sun Paradox

Everything in the universe can be classified as either matter or energy. Kinetic Energy Theory: All particles of matter are in constant motion.

12 The Laws of Thermodynamics

Table of Contents. Chapter: Atmosphere. Section 1: Earth's Atmosphere. Section 2: Energy Transfer in the Atmosphere. Section 3: Air Movement

Study Guide Unit 3 Chapter 6 DRAFT

ASTROVENTURE Extend Lesson Concept Activities

All objects emit radiation. Radiation Energy that travels in the form of waves Waves release energy when absorbed by an object. Earth s energy budget

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.

Mon April 17 Announcements: bring calculator to class from now on (in-class activities, tests) HW#2 due Thursday

OBJECTIVES FOR TODAY S CLASS:

Thermodynamics. Thermodynamics1.notebook. December 14, Quality vs Quantity of Energy

CLIMATE AND CLIMATE CHANGE MIDTERM EXAM ATM S 211 FEB 9TH 2012 V1

Transcription:

WRAP UP: TOPIC #7 Atmospheric Structure & Composition

SUMMARY OF KEY CONCEPTS: short version 1. Four gases N 2, O 2, Ar, & CO 2 comprise about 99% of the volume but minor trace Greenhouse Gases are extremely important. Which one is a GHG? 2. Most of the MASS of the atmosphere is in the bottom few kilometers (i.e. the Toposphere!) 3. Different gases are abundant at certain levels in the atmosphere & where radiation is absorbed by these gases, leads to: vertical temperature profile... 4.... which leads to the vertical structure of the atmosphere: p 41

Most Abundant Greenhouse Gases: GAS Symbol % by volume Water Vapor H 2 O 0.00001 (South Pole) to 4.0 (Tropics) % in ppm 0.1-40,000 Carbon Dioxide CO 2 0.0390 (and rising!) 360 (in 1997) 390 ++! Greenhouse Gases! Review p 40

Two other Important Greenhouse Gases: GAS Symbol % by volume % in ppm Methane CH 4 0.00017 1.7 Nitrous Oxide N 2 O 0.00003 0.3 Ozone O 3 0.0000004 0.01 CFCs (Freon-11) CFCs (Freon-12) CCl 3 F 0.000000026 0.00026 CCl 2 F 2 0.000000047 0.00047 Review p 40

CARBON DIOXIDE: Trends Data from ice cores

METHANE: Trends

NITROUS OXIDE: Trends

Since 0 A.D.! p 40

Updated figures from Dire Predictions p 33 CH 4 CO 2 N 2 O Since 10,000 years ago!

N 2 O The grey bars show the ranges of natural variability for the past 650,000 years! CO 2 CH 4 These graphs go WAY back in time: 20,000 years ago! Radiative Forcing

Other Important Greenhouse Gases: GAS Symbol % by volume % in ppm Methane CH 4 0.00017 1.7 Nitrous Oxide N 2 O 0.00003 0.3 Ozone O 3 0.0000004 0.01 CFCs (Freon-11) CFCs (Freon-12) CCl 3 F 0.000000026 0.00026 CCl 2 F 2 0.000000047 0.00047 Greenhouse Gases! Review p 40

CO 2 Amount in Atmosphere = 386,000 ppb From pp 29-29 in Dire Predictions

Name that GAS!!! MYSTERY GHG # 4

CFCs: Trends FREON-11 Human-made -- didn t exist before 1950! FREON-12

CFCs (Freon-11 & Freon-12) * Human-made CFCs (didn t exist in atmosphere prior to 1950s) * Have increased at rates faster than any other greenhouse gas; used in refrigerants, fire retardants, some aerosol propellants & foam blowing agents * Absorb at different wavelengths than H 2 O and CO 2 (in 8 12 μm WINDOW part of spectrum), hence a single molecule can have great effect ( high Global Warming Potential ) MONTREAL (and subsequent) PROTOCOLS have reduced CFCs! Table p 40

CFCs: Trends Montreal Protocol signed in 1987 to phase out CFCs FREON-11 Called for 50% reduction over 10 years Human-made -- didn t exist before 1950! FREON-12

Q1 Why do you think the concentration of CFC s didn t begin dropping immediately after the Montreal Protocol in 1987? 1. Because it was an international agreement only and the nations of the world never followed through. 2. Because it called for only a 50% reduction of CFC s over 10 years and had to be followed by more stringent protocols later. 3. Because CFC s are very stable molecules and don t break down easily once they are in the atmosphere.

Q1 Why do you think the concentration of CFC s didn t begin dropping immediately after the Montreal Protocol in 1987? 1. Because it was an international agreement only and the nations of the world never followed through. 2. Because it called for only a 50% reduction of CFC s over 10 years and had to be followed by more stringent protocols later. 3. Because CFC s are very stable molecules and don t break down easily once they are in the atmosphere.

24 Sep 2011 http://www.nytimes.com/2011/09/25/business/energy-environment/recyclers-extract-coolant-from-oldrefrigerators.html?_r=1&scp=1&sq=robots%20extract%20coolant%20from%20old%20refrigeratros&st=cse

Companies can use credits from the proper destruction of refrigerants to cover part of their annual emissions, said Gary Gero, president of Climate Action Reserve in Los Angeles, which certifies projects that reduce greenhouse gas emissions and issues offset credits.

NOTE: There are other GHG s (esp. human-made) Some examples: Hydrofluorocarbons (HFCs) Perfluorocarbons (PFCs) Sulfur Hexafluoride (SF 6 ) Like CFCs, some of these are especially harmful because they have high Global Warming Potential (GWP) A high GWP depends on: a large infrared absorption in the right wavelengths and a long atmospheric lifetime.

Now on to today s topic....

TOPIC # 8 LAWS OF THERMODYNAMICS: Keys to Energy Transfer & Conservation The Next Piece in the Puzzle to Understand Global Changes Featuring.... CLASS NOTES: pp 45-49

OUR QUOTE OF THE DAY... In this house, we obey the LAWS of THERMODYNAMICS!... is from HOMER SIMPSON

THERMODYNAMICS (def) = The study of the general properties of ENERGY. Thermal energy plays a central role in understanding these properties, hence the study of energy can also be called thermodynamics.

Forms of Energy - Review Kinetic (KE ) = energy of motion or the ability of a mass to do work. (related to mass and velocity) Potential (PE) = energy a system possesses if it is capable of doing work, but is not doing work now Includes: gravitational, elastic, chemical, electrical, magnetic... and electromagnetic review

Thermal Energy Thermal energy (def) = the grand total of all energies inside a substance: the kinetic energy of the molecules in the substance! Internal Energy -- specifically: a measure of the quantity of atomic kinetic & potential energy contained in every object p 43

Thermal Energy Atoms and molecules are constantly jiggling in some sort of back-and-forth vibratory motion. The greater this molecular kinetic energy is in a substance, the hotter the substance is. p 43

Thermal Energy & Temperature Temperature = tells how warm or cold a body is with respect to some standard (e.g., Fahrenheit ( F), Celsius ( C), or Kelvin (K) standard scales). Temperature is a measure of the average kinetic energy of each molecule in a body. p 43

If a body has a high temperature, each of its molecules has, on the average, a large amount of kinetic energy. e.g. water vapor -- H 2 O molecule at high temperatures p 43

if a body has a low temperature, each molecule on the average has a small amount of kinetic energy. e.g. water vapor molecule H 2 O at lower temperature (and if atoms lose all their kinetic energy, they reach the "absolute zero" of temperature) p 43

Thermal Energy Flow (Transfer) In which direction will THERMAL ENERGY be transferred? Thermal energy flow = HEAT p 43

Thermal Energy vs. Heat Heat = the thermal energy that is transferred from one body to another because of a temperature difference. Heat will always pass from a substance of higher temperature to a substance of lower temperature, until both come to a common temperature. Higher T Lower T p 43

Heat will always pass from a substance of higher temperature to a substance of lower temperature, until both come to a common temperature. p 43

Reaches equilibrium Will not spontaneously return to previous condition! http://jersey.uoregon.edu/vlab/thermodynamics/index.html p 43

Skip to p 44 THE LAWS! Everything that happens can be described as energy transformations (a repeat quote) Was discussed earlier under ENERGY (p 24) THE FIRST LAW OF THERMODYNAMICS (stated as the Law of Conservation of Energy ) The total energy of all the participants in any process must remain unchanged throughout the process. There are no known exceptions. Energy can be transformed (changed from one form to another), but the total amount always remains the same.

An Energy Flow Diagram Energy flow for a falling book, with air resistance. 1 st Law of Thermodynamics p 44

FIRST LAW OF THERMODYNAMICS (another way of saying it) In an isolated system the total amount of energy (including heat energy) is conserved, although energy may change from one form to another over and over again. p 44

SECOND LAW OF THERMODYNAMICS (stated as the Law of Heating ) Heat will not flow spontaneously from a cold to a hot body. Thermal energy flows spontaneously (without external assistance) from a higher temperature object to a lower-temperature object. It will not spontaneously flow the other way! Example from p 43 p 44

The 2nd Law stated another way: Energy flow diagram for a heat engine. 2 nd Law = Any process that uses thermal energy as input to do the work must also have thermal energy output -- or exhaust! WHAT TO REMEMBER: heat engines are always less than 100 % efficient! IMPROVED ENERGY EFFICIENCY IS A KEY ASPECT OF GREEN TECHNOLOGIES! p 44

The 2nd Law stated a THIRD way: Energy of all kinds in our material world disperses or dissipates if it is not hindered from doing so! Entropy = the quantitative measure of this kind of spontaneous dissipating process: i.e., how much energy has flowed from being constricted or concentrated to being more widely spread out (at the temperature of the process) p 44

Irreversibility: Once a system creates thermal energy, that system will never by itself (spontaneously) be able to return to its previous condition. There is an irreversibility about any process that creates thermal energy. p 44

Got all that Homer? boring....!

CLICKER SELF-TEST TIME!!!.... Channel 32

Q2 - Which way is heat being transferred? 1. From the cold beer can into Homer s warmer beer belly 2. From Homer s beer belly to the colder beer can 3. From BOTH the beer can to Homer and Homer to the beer can

Q2 - Which way is heat being transferred? 1. From the cold beer can into Homer s warmer beer belly 2. From Homer s beer belly to the colder beer can 3. From BOTH the beer can to Homer and Homer to the beer can

Explanation for answer to Q2: The 2 nd Law of Thermodynamics! Heat will always pass from a substance of higher temperature to a substance of lower temperature, until both come to a common temperature.

Can I go now???? NO! It s time for a Sustainability Segment!!!

The last segment of: http://www.pbs.org/wgbh/nova/solar/

Can I go now???? YES!! But don t forget RQ-4 on Wednesday before class!!