The Layer Model of the Greenhouse Effect ATS 150 Spring 2015 Lecture 4 Please read Chapter 3 in Archer Textbook.

Slides:



Advertisements
Similar presentations
Causal Loop Diagrams. Exponential growth of a bank account. The two positive connections between Bank balance and interest added for a positive feedback.
Advertisements

Chapter 16: Weather Factors
Bare rock model Assumptions
Radiation Balance of the Earth-Atmosphere System In Balance: Energy flow in = Energy flow out PowerPoint 97 To download: Shift LeftClick Please respect.
MET 112 Global Climate Change
Chapter 2 Solar Heating. (Variations in) Solar Heating Power Weather Important Global and Seasonal Variations: Low latitudes receive more solar heating.
Chapter 2 Weather Factors
The atmosphere S6E4a: Demonstrate that land and water absorb and lose heat at different rates and explain the resulting effects on weather patterns.
Thermal Energy Transfer
16-1 Energy in Earth’s Atmosphere. (pages 542–545) 1
An improved energy balance model Goals: understand the effects of atmosphere and Greenhouse gases on the earth temperature.
Solar constant The solar constant is the amount of incoming solar radiation per unit area, measured on the outer surface of Earth's atmosphere, in a plane.
Climate Change and its consequences Bill Menke October 4, 2005.
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.
Chapter 2: Weather Factors
ENERGY FROM THE SUN Chapter 14.3 Pages Energy in the Atmosphere The sun is the source of ALL energy in our atmosphere. Three things that can.
1 BAESI - Global Warming: Food Climate Connections The Greenhouse Effect Dr. Eugene Cordero San Jose State University Outline  Greenhouse effect  Energy.
Lecture 1: Introduction to the planetary energy balance Keith P Shine, Dept of Meteorology,The University of Reading
EXPLAIN 2. Earth’s Energy Balance. Energy Balance Let the rate of energy flow from the Sun to the Earth be called F in Let the rate of energy flow from.
Earth-Atmosphere Energy Balance Earth's surface absorbs the 51 units of shortwave and 96 more of longwave energy units from atmospheric gases and clouds.
CH 24.3 Solar Radiation, Pressure, & Wind. Earth’s Energy Balance Input = Sun’s Energy = (Visible light + some UV) REFLECTED: ~ 25 % by clouds, dust,
The Greenhouse Effect Garver GEO 307. Take home points from Chapter 2  EMR carries energy through space  If an object can absorb energy, it can also.
Energy from the Sun Radiation is the transfer of energy by electromagnetic waves. Ninety-nine percent of the radiation from the Sun consists of visible.
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.
National Aeronautics and Space Administration The Energy Budget and the Greenhouse Effect Dr. Lin H. Chambers, NASA Langley Research Center.
Solar Radiation and Energy Balance Unit 3: Weather and Climate Geo 12 Ms. Thind.
AOS 100: Weather and Climate Instructor: Nick Bassill Class TA: Courtney Obergfell.
Transmission of Heat. Conduction n Heat transfer due to direct contact n Either between different materials in thermal contact or different parts of the.
Very Basic Climate Modeling Spring 2012, Lecture 5 1.
Solar Energy and Energy Balance in the Atmosphere.
Energy in the Atmosphere
Physics and Astronomy Outreach Program at the University of British Columbia Physics and Astronomy Outreach Program at the University of British Columbia.
Sun Controls Earth’s Climate System Earth has a global climate system that includes air, land, liquid water, ice, and living things.climate system The.
Energy Balance Chapter 18.
Earth’s Energy Budget Ch ways heat can be transferred: Conduction Conduction Convection Convection Radiation Radiation.
Heat Transfer in the Atmosphere Essential Question: How is heat transferred in the atmosphere?
 There are two common meanings of the term "greenhouse effect". There is a "natural" greenhouse effect that keeps the Earth's climate warm and habitable.
Please read Chapter 4 in Archer Textbook
Heat Transfer Conduction, Convection, Radiation. Three Main Processes of Heat Transfer  Conduction  Convection  Radiation.
Goals for Today 1.PREDICT the consequences of varying the factors that determine the (a) effective radiating temperature and (b) mean surface temperature.
Image: January 2004 Blue Marble Composite – Reto Stöckli, NASA Earth Observatory Energy, space, and Earth's effective temperature Unit 1 of Earth’s Thermostat.
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.
Heat Transfer, Albedo, and the Natural Greenhouse Effect.
Blackbody Radiation/ Planetary Energy Balance
1 Weather, Climate & Society ATMO 325 Global Energy Balance Greenhouse Effect.
How is Energy Transferred?. Radiation animations of heat transfer Emission and transfer of energy by means of electromagnetic waves Method of heat transfer.
CHAPTER 19 HEAT TRANSFER IN THE ATMOSPHERE. WHAT IS THE ATMOSPHERE? Earth’s atmosphere is heated by the transfer of energy from the sun. Some heat comes.
The Greenhouse Effect. A greenhouse is a building used to grow plants when the outside temperature is too low. The roof of the greenhouse prevents convection.
Energy from the Sun Radiation is the transfer of energy by electromagnetic waves. Ninety-nine percent of the radiation from the Sun consists of visible.
Energy Transfer in the Atmosphere
Climate Change: Simple, Serious, Solvable
Earth's Energy and Radiation By: May-Lynn Fortune & Maesey Phillips
Thermal radiation.
The Greenhouse Effect Garver GEO 307.
ENERGY IN THE BIOSPHERE
12: Greenhouses and the Earth System
The Sun Powers Earth’s Climate System
Energy Budget Subtitle.
Earth’s Energy Budget.
GLOBAL ENERGY BUDGET - 2 The Greenhouse Effect.
Energy transfer in the atmosphere
Journal #25 What is a greenhouse? What is the greenhouse effect?
Energy from the Sun.
The Transfer of Heat Chapter 13.
Energy and Heat Transfer in the Atmosphere
Climate Earth’s Energy Budget.
The Ins & Outs of Solar Radiation
The Sun is the source of energy for the Earth.
Unit 5 Earth’s Energy Budget.
Presentation transcript:

The Layer Model of the Greenhouse Effect ATS 150 Spring 2015 Lecture 4 Please read Chapter 3 in Archer Textbook

What is a Model? Models represent reality in a simplified or idealized way Used to understand or predict Doesn’t have to be realistic to be useful

Generalized mathematical formulation with adjustable coefficients Combinations of – polynomials – exponential growth & decay – Periodic sines and cosines Coefficients fit to data (e.g., least squares) Interpolation or extrapolation Empirical Models

Deterministic Models Formulated as “cause and effect” Common in physics and chemistry Usually take the form of differential equations Initial & boundary- value problems May still have adjustable coefficients

Energy Balance Let the rate of energy flow from the Sun to the Earth be called F in Let the rate of energy flow from the Earth to outer space be called F out Energy In = Energy Out

Energy Balance Assume both Sun and Earth are blackbodies (  =1), so F =  T 4 F in = absorbed sunlight x daylight area F out =  T earth 4 x total area F in = F out

Energy Balance F in = F out F in = Solar brightness x (1 – albedo) x (area of Earth’s shadow) F out =  (T earth ) 4 x (area of Earth’s surface)

30% reflected by clouds, air, dust, and surface 30% reflected by clouds, air, dust, and surface 19% absorbed by the atmosphere (mostly clouds) 19% absorbed by the atmosphere (mostly clouds) 51% absorbed at the surface 51% absorbed at the surface Solar Radiation

Energy Balance F in = F out F in = Solar brightness x (1 –  ) x  r 2 F out =  (T e ) 4 x 4  r 2

Energy Balance F in = F out

Energy Balance F in = F out But the observed surface temperature is about 288 K

Both are almost perfect blackbodies! The hot sun radiates at shorter (visible) wavelengths that carry more energy Energy absorbed by the cooler earth is then re- radiated at longer (thermal infrared) wavelengths Thermal Emission SUN EARTH 255 K

Works for Other Planets Too F in = F out Experiment!

Bare Rock Model If sunlight were the only source of energy, the surface of the Earth would be way too cold for life! 255 °K = -18 °C = -1 °F Surface Sunlight F surface F in = F out

Two-Layer Model Now imagine a layer of glass above the solid rock Glass is transparent to sunlight Glass is opaque to “Earthlight” (thermal IR) Glass Surface Sunlight F glass F surface

Two-Layer Model Sun shines right through transparent glass layer Glass layer emits both upward and downward Glass layer “feels” both space and surface Surface “feels” both Sun and glass Glass Surface Glass boundary Boundary F in = F out

Seen from Above Both models: Absorb the same sunshine Reflect the same amount of sunlight back out Emit the same amount of Earthlight Glass Surface Sunlight F glass F surface Sunlight F surface boundary

Two-Layer Model Use balance at boundary to space to find temperature of the glass Since energy in from Sun and energy out from glass are same as bare rock model, temperature is too! glass surface boundary Boundary F in = F out Glass 255 K = T glass

Two-Layer Model Recall from boundary balance that S(1-  )/4 =  T glass 4 Substitute this into surface balance glass surface boundary F in = F out Surface Find that surface is much warmer under glass! 303 °K = 30 °C = 86 °F

Summary Layer models are not meant to be accurate or predictive, just to help us understand how the world works Energy balance of “bare rock” model is way too cold to support life! Adding a layer of glass makes the surface nice and toasty Where did the heat come from?

Bathtub Analogy If faucet runs faster than drain, level rises And vice versa Drain runs faster when water is deep Adding glass to layer model acts like a clog in the drain Water rises until drainage = inflow again Faucet ~ Sun Drain ~ Thermal emission Water level ~ temperature

Three Layers Top boundary (“skin”) temperature is always the same As we add layers, the surface gets hotter (bathtub drain gets slower)

Ten Layers Top boundary (“skin”) temperature is always the same As we add layers, the surface gets hotter (bathtub drain gets slower)

100 Layers! Top boundary (“skin”) temperature is always the same As we add layers, the surface gets hotter (bathtub drain gets slower)