What is the Greenhouse Effect?. Review of last lecture – The two basic motions of the Earth – What causes the four seasons: the Earth’s tilt and the 3.

Slides:



Advertisements
Similar presentations
2.1 Energy in the Atmosphere
Advertisements

Chapter 3 Energy Balance and Temperature. Atmospheric gases, particulates, and droplets all reduce the intensity of solar radiation (insolation) by absorption,
The Earth’s Energy Budget Chapter 3 Objectives Trace the flow of energy through the atmosphere.
MET 112 Global Climate Change
22.2 Solar Energy and the Atmosphere. What happens to incoming solar radiation? 1.Scattered 2.Reflected 3.Absorbed.
Earth’s Energy Exchange GPH 111. Insolation at Earth’s Surface Average annual solar radiation receipt on a horizontal surface at ground level in watts.
Earth’s Global Energy Balance Overview
Chapter 3 – Energy Balance and Temperature. The Fate of Solar Radiation We owe it all to the sun… 3 things can happen to solar (and all) radiation: 1)
Part 1. Energy and Mass Chapter 3. Energy Balance and Temperature.
Part 1. Energy and Mass Chapter 3. Energy Balance and Temperature.
ATS Lecture 2 Energy & Radiation Surface Maps.
What happens to solar energy ? 1.Absorption (absorptivity=  ) Results in conduction, convection and long-wave emission 2.Transmission (transmissivity=
1 MET 112 Global Climate Change MET 112 Global Climate Change - Lecture 2 The Earth’s Energy Balance Dr. Craig Clements San José State University Outline.
Handout (yellow) Solar Energy and the Atmosphere Standard 3 Objective 1 Indicators a, b, and c Standard 3 Objectives 1, 2, and 3 Workbook Pages 3,
Chapter 2: Weather Factors
1 BAESI - Global Warming: Food Climate Connections The Greenhouse Effect Dr. Eugene Cordero San Jose State University Outline  Greenhouse effect  Energy.
GY205 Weather and Climate Lecture 2 (Please turn in homework on the table.)
Surface air temperature. Review of last lecture Earth’s energy balance at the top of the atmosphere and at the surface. What percentage of solar energy.
Solar Energy & the Atmosphere
Solar Energy and the Atmosphere
Atmospheric temperature
Chapter 3 Energy Balance and Temperature. Atmospheric gases, particulates, and droplets all reduce the intensity of solar radiation (insolation) by absorption,
Visualizing Physical Geography Copyright © 2008 John Wiley and Sons Publishers Inc. Chapter 2 The Earth’s Global Energy Balance.
1 MET 112 Global Climate Change MET 112 Global Climate Change - Lecture 2 The Earth’s Energy Balance Dr. Eugene Cordero San Jose State University Outline.
1 Met 10 Weather Processes Jeff Gawrych Temperature, Heat Transfer and Earth’s Energy Balance.
Ozone Creation. Chapter 4 Atmosphere and Surface Energy Balances Geosystems 6e An Introduction to Physical Geography Robert W. Christopherson Charles.
Energy: Warming the earth and Atmosphere
Radiation in the Atmosphere (Cont.). Cloud Effects (2) Cloud effects – occur only when clouds are present. (a) Absorption of the radiant energy by the.
Objectives Explain how radiant energy reaches Earth.
Midterm #1 - Wednesday!!! Bring a scantron sheet!!!!! No OH’s this week again (last time – I promise) Midterm Review Tonight Broida Hall1610 starting 6:30!!
Chapter 10, Section 2 Chapter 22, Section 2. Solar Energy Key Terms: Create a flashcard for each. The words can be found starting on page 555 or use the.
Solar Radiation and Insolation Incoming solar radiation:
Ch3: Energy Balance and Temperature. 1.About the first in-class assignment 2.About reading the textbook.
ESS 111 – Climate & Global Change Lecture 3 Greenhouse Effect El Nino – Southern Oscillation.
Energy: Warming the Earth & the Atmosphere
Welcome Back Write down the 4 layers of the atmosphere (in order) and 1 fact about each.
AOS February 19/21 Energy Transfer. Four mechanisms of transfer Conduction Convection Advection Radiation.
Ch Solar Energy and the Atmosphere
AOSC Lesson 2. Temperature Scales Temperature scales are defined by upper and lower calibration points (fixed points) In the Fahrenheit temperature scale.
Chapter 4 Atmosphere and Surface Energy Balances Robert W. Christopherson Charlie Thomsen.
Solar Energy and Energy Balance in the Atmosphere.
Copyright © 2013 Pearson Education, Inc. The Atmosphere: An Introduction to Meteorology, 12 th Lutgens Tarbuck Lectures by: Heather Gallacher, Cleveland.
The Atmosphere: Energy Transfer & Properties Weather Unit Science 10.
Energy in the Atmosphere
Energy Balance Chapter 18.
Surface energy balance (2). Review of last lecture –What is energy? 3 methods of energy transfer –The names of the 6 wavelength categories in the electromagnetic.
What is the Greenhouse Effect?. Review of last lecture – What is energy? 3 methods of energy transfer – The names of the 6 wavelength categories in the.
Lecture 3: Radiation and Earth’s Atmosphere EarthsClimate_Web_Chapter.pdfEarthsClimate_Web_Chapter.pdf, p. 1-5 For more advanced reading materials, please.
Incoming & Outgoing of Energy of the Earth. The Earth’s Energy Balance The Earth's average temperature remains fairly constant from year to year. Therefore,
Solar Energy and the Atmosphere
1 MET 112 Global Climate Change MET 112 Global Climate Change - Lecture 3 The Earth’s Energy Balance Dr. Eugene Cordero San Jose State University Outline.
Chapter 4 Atmosphere and Surface Energy Balances Geosystems 6e An Introduction to Physical Geography Robert W. Christopherson Charles E. Thomsen.
Atmosphere-ocean interactions Exchange of energy between oceans & atmosphere affects character of each In oceans –Atmospheric processes alter salinity.
Energy = the ability to do work Two Energy Categories: 1. Kinetic Energy (energy of motion) Types: – Electromagnetic energy (from our Sun) – Light energy.
Journal #27 What were your results from yesterday? Why did you get the results you did?
Radiation Balance.
Unit 9 Section 2: Solar Energy and the Atmosphere
Radiation Balance. Radiation Balance In atmosphere, radiation can be… transmitted absorbed reflected.
Global energy balance SPACE
Lecture 4: Heat Transfer and Energy Balance
Solar Energy and the Atmosphere
Radiation Balance.
Section 2: Solar Energy and the Atmosphere
“Energy in Earth Processes”
AOSC Lesson 4.
Journal #25 What is a greenhouse? What is the greenhouse effect?
The Earth’s Energy Budget/ Heat Balance
Climate Earth’s Energy Budget.
Heat in the Atmosphere.
Solar Energy and the Atmosphere
Presentation transcript:

What is the Greenhouse Effect?

Review of last lecture – The two basic motions of the Earth – What causes the four seasons: the Earth’s tilt and the 3 ways it affects the solar insolation (change of length of the day, beam spreading, beam depletion) – Change of the Earth’s orbit at longer time scales (Milankovitch cycles): eccentricity, axial tilt, and precession

Satellite Measurements of the Earth’s Radiation Budget NASA’s Earth Radiation Budget Satellite (ERBS)

Earth’s energy budget (averaged over the whole globe and over a long time) At the top of the atmosphere: At the top of the atmosphere: Incoming shortwave = Reflected Shortwave + Emitted longwave Incoming shortwave = Reflected Shortwave + Emitted longwave At the surface: At the surface: Incoming shortwave = Reflected shortwave + Net emitted longwave (emitted - incoming) Incoming shortwave = Reflected shortwave + Net emitted longwave (emitted - incoming) + Latent heat flux + sensible heat flux + Latent heat flux + sensible heat flux Sensible heat 7% Latent heat 23% Net Longwave 21% Yellow: shortwave Red: longwave

Atmospheric influences on radiation ReflectionScattering Absorption (absorber warms)

Reflection reflection – redirection of energy w/o absorption reflection – redirection of energy w/o absorption all objects reflect visible light  effectiveness varies all objects reflect visible light  effectiveness varies albedo – % of visible light reflected albedo – % of visible light reflected There are two types of reflection (solid surface): There are two types of reflection (solid surface): –Specular: light is reflected with equal intensity (e.g. mirror) –Diffuse reflection OR scattering: light is reflected in multiple directions, weakly (e.g. snow)

3 Types of Scattering: 1.Raleigh 2.Mie 3.Non-Selective Atmospheric Scattering A discussion of each type follows…

involves gases smaller than insolation wavelength scatters light in all directions most effective at short wavelengths (violet, blue)… hence, blue sky Rayleigh Scattering The Earth has an atmosphere. So it has Rayleigh scattering and its sky appears blue The Moon has no atmosphere. So it has no Rayleigh scattering and its sky appears dark

Rayleigh scattering also explains reddish-orange sunsets when light travels through thick slice of atmosphere

Monet: Impressions, Sunrise

Grainstacks at different time of the day

2) Mie scattering –involves aerosols (e.g. dust, smoke) larger than gas molecules –forward scatter –equally effective across visible spectrum –explains hazy, gray days

3) Non-selective scattering –Happens when atmospheric particles are much larger than the wavelength of incoming radiation (e.g. water droplets in clouds) –Act like lenses; scatter all wavelengths equally to create a white appearance –That’s why clouds appear white

Video: The greenhouse effect Mk Mk Mk Mk

Atmospheric Absorption - The Greenhouse Effect Transparent to solar (shortwave) radiation Opaque to earth’s (longwave) radiation Major GH gases: CO 2, H 2 0 (v), CH 4

The importance of methane (CH 4 ) 23 times more powerful as a greenhouse gas than CO 2 23 times more powerful as a greenhouse gas than CO 2 The livestock sector is a major player, which accounts for 35-40% global anthropogenic emissions of methane (their burps!) The livestock sector is a major player, which accounts for 35-40% global anthropogenic emissions of methane (their burps!) The livestock sector is responsible for 18% of total greenhouse gas emissions The livestock sector is responsible for 18% of total greenhouse gas emissions Therefore, consuming less meat can help reducing global warming than not driving cars. Therefore, consuming less meat can help reducing global warming than not driving cars.

Seasonal variation of surface radiation

Surface “Sensible” and “Latent” heat transfers 1. Conduction –This is how excess heat in ground is transferred to the atmosphere via an extremely thin layer of air in contact with the surface 2. Convection –Once the heat is transferred from the surface to the air via conduction, convection takes over from here via “sensible” and “latent” heat transfers First, recall 2 other methods of energy transfer in addition to radiation:

Sensible Heat Heat energy which is readily detected Heat energy which is readily detected Magnitude is related to an object’s specific heat Magnitude is related to an object’s specific heat –The amount of energy needed to change the temperature of an object a particular amount in J/kg/K Related to mass Related to mass –Higher mass requires more energy for heating Sensible heat transfer occurs from warmer to cooler areas (i.e., from ground upward) Sensible heat transfer occurs from warmer to cooler areas (i.e., from ground upward)

Latent Heat Energy required to induce changes of state in a substance Energy required to induce changes of state in a substance In atmospheric processes, invariably involves water In atmospheric processes, invariably involves water When water is present, latent heat of evaporation redirects some energy which would be used for sensible heat When water is present, latent heat of evaporation redirects some energy which would be used for sensible heat –Wet environments are cooler relative to their insolation amounts Latent heat of evaporation is stored in water vapor Latent heat of evaporation is stored in water vapor –Released as latent heat of condensation when that change of state is induced Latent heat transfer occurs from regions of wetter-to-drier Latent heat transfer occurs from regions of wetter-to-drier

Seasonal variation of surface energy budget Storage change = net radiation - latent heat flux - sensible heat flux

Summary Earth’s energy balance at the top of the atmosphere and at the surface. What percentage of solar energy is absorbed by the surface? Earth’s energy balance at the top of the atmosphere and at the surface. What percentage of solar energy is absorbed by the surface? Atmospheric influences on radiation (3 ways) Atmospheric influences on radiation (3 ways) The three types of atmospheric scattering. What causes the blue sky? Why causes the reddish-orange sunsets? The three types of atmospheric scattering. What causes the blue sky? Why causes the reddish-orange sunsets? What cause the greenhouse effect? What are the major greenhouse gases? Why is methane important? What cause the greenhouse effect? What are the major greenhouse gases? Why is methane important? Sensible heat flux (dry flux from warm to cold regions) and latent heat flux (wet flux from wet to dry regions) Sensible heat flux (dry flux from warm to cold regions) and latent heat flux (wet flux from wet to dry regions)