17 March Good luck!

Size: px
Start display at page:

Download "17 March Good luck!"

Transcription

1 ! Midterm Exam 17 March 2005 Name:! SID:!! The mid-term has a maximum of 120 points: 60 points for a section with short essays, and 60 points for a section with qualitative/quantitative problems. Remember to carefully read the questions! Think simple and do not make unnecessary assumptions! Write clearly and use the provided space. Good luck! Remember to write clearly so that your instructor can read and understand your answers! Academic Integrity. The University Senate requires that students include the following signed statement on each examination: I pledge on my honor that I have not given or received any unauthorized assistance on this examination

2 Part I: Short Essays (4 * 15 pts. max = 60 pts. max) In this section I look for a brief answers and explanations of about one paragraph in length that answer the questions. Make sure that you include the most relevant aspects of the correct answer. Answer only 4 out of the 5 questions (pick your favorites)! 1. What is the atmospheric greenhouse effect? 2. What different roles does the expression P - E (precipitation - evaporation) play for the different components of the climate system?

3 3. Can the atmosphere transport heat only by a mean circulation (characterized by a mean wind speed), or are there also other possible means? 4. Which role does vegetation play for the surface energy- and water balance? Which terms are affected, and why are these affected by vegetation?

4 5. Is the sensible heat flux always directed from the surface to the atmosphere (i.e. cools the surface, heats the atmosphere), or can you imagine a situation in which the heat flux would be reversed? Where on Earth is this likely to be found?

5 Part II: Qualitative/Quantitative (3 * 20 pts. max = 60 pts. max) This section involves interpretation of diagrams and/or some simple calculations. Make sure that you show all your work of how you got to the answer. You may use a calculator for getting the final numerical value. Answer only 3 out of the 4 problems (pick your favorites)! 1. Energy Balance. The diagram shown below shows the global energy balance of Earth, with some numbers missing stratosphere 10 7 re- 21 emitted troposphere 335 emitted re- 17 SH LH surface 171 emitted -376 re- 304 heat fluxes 99 solar shortwave terrestrial longwave turbulent fluxes all units in W/m 2 a. Fill in the missing numbers! b. How strong is the atmospheric greenhouse (in terms of units) in the diagram?

6 2. Terrestrial water balance. The diagram below shows the mean seasonal course of precipitation (solid line) and potential evaporation (dotted line) for one location in the US. a. What would be the seasonal course of evaporation if storage of soil moisture is (a) negligible and (b) sufficiently large? Draw the two cases of evaporation into the diagram, mark them clearly, and briefly explain cm/month J F M A M J J A S O N D J b. What would be the seasonal cycle in soil moisture content in the case of a large storage capacity? During which months is soil moisture recharged and depleted and in which months would the maximum/ minimum in soil moisture be found? Draw the seasonal course of soil moisture into the empty diagram below and add a scale and a proper unit. Remember that the change in soil moisture is directly related to precipitation and evaporation (neglect the effect of runoff for simplicity). J F M A M J J A S O N D J

7 3. Radiative temperature. In 2004, scientists at Caltech and Yale discovered a tenth large object orbiting the Sun, which since has been named Sedna. Sedna orbits the Sun on a highly elliptical orbit far outside from Pluto s orbit (see figure on right). The closest distance of Sedna to the Sun is about 76 AU (1 AU = km, the mean distance of the Earth to Sun), at the farthest point of the orbit, Sedna is about 1000 AU away from the Sun. a. How much incoming solar radiation does Sedna receive at the perihelion? Orbit of Sedna in relation to the other 9 planets in our solar system. b. Assuming a planetary albedo of 20%, what would be the radiative temperature of Sedna at the perihelion?

8 4. Heat Transport. Calculate the surface temperatures of polar and tropical regions from a simple energy balance approach. Use QT = 300 W/m 2 and QP = 170 W/m 2 for the amount of solar radiation in the tropics and polar regions respectively, and use QTR = A + B * T for the emission of terrestrial radiation (for a temperature T in C) with A = 204 W/m 2 and B = 2.17 W/m 2 /K -1. Neglect turbulent heat fluxes. a. What would be the tropical and polar temperatures in the case of no heat transport? b. What is the global mean surface temperature? To calculate the mean absorption of solar radiation use the numbers from above and assume that the tropical and polar regions represent equal areas (so that the mean is given by (QT + QP)/2 ). How much heat transport would be required to be removed from the tropics for it to attain the global mean value?

Data and formulas at the end. Exam would be Weds. May 8, 2008

Data and formulas at the end. Exam would be Weds. May 8, 2008 ATMS 321: Science of Climate Practice Mid Term Exam - Spring 2008 page 1 Atmospheric Sciences 321 Science of Climate Practice Mid-Term Examination: Would be Closed Book Data and formulas at the end. Exam

More information

Data and formulas at the end. Real exam is Wednesday May 8, 2002

Data and formulas at the end. Real exam is Wednesday May 8, 2002 ATMS 31: Physical Climatology Practice Mid Term Exam - Spring 001 page 1 Atmospheric Sciences 31 Physical Climatology Practice Mid-Term Examination: Would be Closed Book Data and formulas at the end. Real

More information

Lecture 9: Climate Sensitivity and Feedback Mechanisms

Lecture 9: Climate Sensitivity and Feedback Mechanisms Lecture 9: Climate Sensitivity and Feedback Mechanisms Basic radiative feedbacks (Plank, Water Vapor, Lapse-Rate Feedbacks) Ice albedo & Vegetation-Climate feedback Cloud feedback Biogeochemical feedbacks

More information

Lecture 3: Global Energy Cycle

Lecture 3: Global Energy Cycle Lecture 3: Global Energy Cycle Planetary energy balance Greenhouse Effect Vertical energy balance Latitudinal energy balance Seasonal and diurnal cycles Solar Flux and Flux Density Solar Luminosity (L)

More information

Global Climate Change

Global Climate Change Global Climate Change Definition of Climate According to Webster dictionary Climate: the average condition of the weather at a place over a period of years exhibited by temperature, wind velocity, and

More information

Electromagnetic Radiation. Radiation and the Planetary Energy Balance. Electromagnetic Spectrum of the Sun

Electromagnetic Radiation. Radiation and the Planetary Energy Balance. Electromagnetic Spectrum of the Sun Radiation and the Planetary Energy Balance Electromagnetic Radiation Solar radiation warms the planet Conversion of solar energy at the surface Absorption and emission by the atmosphere The greenhouse

More information

Lecture 10: Climate Sensitivity and Feedback

Lecture 10: Climate Sensitivity and Feedback Lecture 10: Climate Sensitivity and Feedback Human Activities Climate Sensitivity Climate Feedback 1 Climate Sensitivity and Feedback (from Earth s Climate: Past and Future) 2 Definition and Mathematic

More information

Radiation, Sensible Heat Flux and Evapotranspiration

Radiation, Sensible Heat Flux and Evapotranspiration Radiation, Sensible Heat Flux and Evapotranspiration Climatological and hydrological field work Figure 1: Estimate of the Earth s annual and global mean energy balance. Over the long term, the incoming

More information

GEOG415 Mid-term Exam 110 minute February 27, 2003

GEOG415 Mid-term Exam 110 minute February 27, 2003 GEOG415 Mid-term Exam 110 minute February 27, 2003 1 Name: ID: 1. The graph shows the relationship between air temperature and saturation vapor pressure. (a) Estimate the relative humidity of an air parcel

More information

Radiative Equilibrium Models. Solar radiation reflected by the earth back to space. Solar radiation absorbed by the earth

Radiative Equilibrium Models. Solar radiation reflected by the earth back to space. Solar radiation absorbed by the earth I. The arth as a Whole (Atmosphere and Surface Treated as One Layer) Longwave infrared (LWIR) radiation earth to space by the earth back to space Incoming solar radiation Top of the Solar radiation absorbed

More information

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

Earth s Energy Budget: How Is the Temperature of Earth Controlled? 1 NAME Investigation 2 Earth s Energy Budget: How Is the Temperature of Earth Controlled? Introduction As you learned from the reading, the balance between incoming energy from the sun and outgoing energy

More information

1. Weather and climate.

1. Weather and climate. Lecture 31. Introduction to climate and climate change. Part 1. Objectives: 1. Weather and climate. 2. Earth s radiation budget. 3. Clouds and radiation field. Readings: Turco: p. 320-349; Brimblecombe:

More information

Torben Königk Rossby Centre/ SMHI

Torben Königk Rossby Centre/ SMHI Fundamentals of Climate Modelling Torben Königk Rossby Centre/ SMHI Outline Introduction Why do we need models? Basic processes Radiation Atmospheric/Oceanic circulation Model basics Resolution Parameterizations

More information

AT350 EXAM #1 September 23, 2003

AT350 EXAM #1 September 23, 2003 AT350 EXAM #1 September 23, 2003 Name and ID: Enter your name and student ID number on the answer sheet and on this exam. Record your answers to the questions by using a No. 2 pencil to completely fill

More information

5. General Circulation Models

5. General Circulation Models 5. General Circulation Models I. 3-D Climate Models (General Circulation Models) To include the full three-dimensional aspect of climate, including the calculation of the dynamical transports, requires

More information

Lecture 2: Light And Air

Lecture 2: Light And Air Lecture 2: Light And Air Earth s Climate System Earth, Mars, and Venus Compared Solar Radiation Greenhouse Effect Thermal Structure of the Atmosphere Atmosphere Ocean Solid Earth Solar forcing Land Energy,

More information

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

Name(s) Period Date. Earth s Energy Budget: How Is the Temperature of Earth Controlled? Name(s) Period Date 1 Introduction Earth s Energy Budget: How Is the Temperature of Earth Controlled? As you learned from the reading, the balance between incoming energy from the sun and outgoing energy

More information

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

- matter-energy interactions. - global radiation balance. Further Reading: Chapter 04 of the text book. Outline. - shortwave radiation balance (1 of 12) Further Reading: Chapter 04 of the text book Outline - matter-energy interactions - shortwave radiation balance - longwave radiation balance - global radiation balance (2 of 12) Previously, we

More information

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

CLIMATE AND CLIMATE CHANGE MIDTERM EXAM ATM S 211 FEB 9TH 2012 V1 CLIMATE AND CLIMATE CHANGE MIDTERM EXAM ATM S 211 FEB 9TH 2012 V1 Name: Student ID: Please answer the following questions on your Scantron Multiple Choice [1 point each] (1) The gases that contribute to

More information

Understanding the Greenhouse Effect

Understanding the Greenhouse Effect EESC V2100 The Climate System spring 200 Understanding the Greenhouse Effect Yochanan Kushnir Lamont Doherty Earth Observatory of Columbia University Palisades, NY 1096, USA kushnir@ldeo.columbia.edu Equilibrium

More information

Observation: predictable patterns of ecosystem distribution across Earth. Observation: predictable patterns of ecosystem distribution across Earth 1.

Observation: predictable patterns of ecosystem distribution across Earth. Observation: predictable patterns of ecosystem distribution across Earth 1. Climate Chap. 2 Introduction I. Forces that drive climate and their global patterns A. Solar Input Earth s energy budget B. Seasonal cycles C. Atmospheric circulation D. Oceanic circulation E. Landform

More information

Chapter 2 Solar and Infrared Radiation

Chapter 2 Solar and Infrared Radiation Chapter 2 Solar and Infrared Radiation Chapter overview: Fluxes Energy transfer Seasonal and daily changes in radiation Surface radiation budget Fluxes Flux (F): The transfer of a quantity per unit area

More information

Lecture 3a: Surface Energy Balance

Lecture 3a: Surface Energy Balance Lecture 3a: Surface Energy Balance Instructor: Prof. Johnny Luo http://www.sci.ccny.cuny.edu/~luo Total: 50 pts Absorption of IR radiation O 3 band ~ 9.6 µm Vibration-rotation interaction of CO 2 ~

More information

Components of the Climate System. Lecture 2: Earth s Climate System. Pop Quiz. Sub-components Global cycles What comes in What goes out

Components of the Climate System. Lecture 2: Earth s Climate System. Pop Quiz. Sub-components Global cycles What comes in What goes out Lecture 2: Earth s Climate System Components of the Climate System terrestrial radiation Atmosphere Ocean solar radiation Land Energy, Water, and Biogeochemistry Cycles Sub-components Global cycles What

More information

Lecture 2: Earth s Climate System

Lecture 2: Earth s Climate System Lecture 2: Earth s Climate System terrestrial radiation solar radiation Atmosphere Ocean Solid Earth Land Energy, Water, and Biogeochemistry Cycles Sub-components Global cycles What comes in What goes

More information

FORCING ANTHROPOGENIC

FORCING ANTHROPOGENIC NATURAL CLIMATIC FORCING Earth-Sun orbital relationships, changing landsea distribution (due to plate tectonics), solar variability & VOLCANIC ERUPTIONS vs. ANTHROPOGENIC FORCING Human-Enhanced GH Effect,

More information

Chapter 02 Energy and Matter in the Atmosphere

Chapter 02 Energy and Matter in the Atmosphere Chapter 02 Energy and Matter in the Atmosphere Multiple Choice Questions 1. The most common gas in the atmosphere is. A. oxygen (O2). B. carbon dioxide (CO2). C. nitrogen (N2). D. methane (CH4). Section:

More information

Boundary layer equilibrium [2005] over tropical oceans

Boundary layer equilibrium [2005] over tropical oceans Boundary layer equilibrium [2005] over tropical oceans Alan K. Betts [akbetts@aol.com] Based on: Betts, A.K., 1997: Trade Cumulus: Observations and Modeling. Chapter 4 (pp 99-126) in The Physics and Parameterization

More information

Friday 8 September, :00-4:00 Class#05

Friday 8 September, :00-4:00 Class#05 Friday 8 September, 2017 3:00-4:00 Class#05 Topics for the hour Global Energy Budget, schematic view Solar Radiation Blackbody Radiation http://www2.gi.alaska.edu/~bhatt/teaching/atm694.fall2017/ notes.html

More information

( 1 d 2 ) (Inverse Square law);

( 1 d 2 ) (Inverse Square law); ATMO 336 -- Exam 3 120 total points including take-home essay Name The following equations and relationships may prove useful. F d1 =F d2 d 2 2 ( 1 d 2 ) (Inverse Square law);! MAX = 0.29 " 104 µmk (Wien's

More information

Atmospheric "greenhouse effect" - How the presence of an atmosphere makes Earth's surface warmer

Atmospheric greenhouse effect - How the presence of an atmosphere makes Earth's surface warmer Atmospheric "greenhouse effect" - How the presence of an atmosphere makes Earth's surface warmer Some relevant parameters and facts (see previous slide sets) (So/) 32 W m -2 is the average incoming solar

More information

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

Topic # 6 ATMOSPHERIC STRUCTURE & CHEMICAL COMPOSITION Part II. Plus wrap up of some other topics Topic # 6 ATMOSPHERIC STRUCTURE & CHEMICAL COMPOSITION Part II Plus wrap up of some other topics THE POWER OF COLLABORATIVE LEARNING! Individual Test Class mean REMEMBER: Your group is there to HELP YOU

More information

Lecture 2: Global Energy Cycle

Lecture 2: Global Energy Cycle Lecture 2: Global Energy Cycle Planetary energy balance Greenhouse Effect Vertical energy balance Solar Flux and Flux Density Solar Luminosity (L) the constant flux of energy put out by the sun L = 3.9

More information

Lecture 11: Meridonal structure of the atmosphere

Lecture 11: Meridonal structure of the atmosphere Lecture 11: Meridonal structure of the atmosphere September 28, 2003 1 Meridional structure of the atmosphere In previous lectures we have focussed on the vertical structure of the atmosphere. Today, we

More information

9/5/16. Section 3-4: Radiation, Energy, Climate. Common Forms of Energy Transfer in Climate. Electromagnetic radiation.

9/5/16. Section 3-4: Radiation, Energy, Climate. Common Forms of Energy Transfer in Climate. Electromagnetic radiation. Section 3-4: Radiation, Energy, Climate Learning outcomes types of energy important to the climate system Earth energy balance (top of atm., surface) greenhouse effect natural and anthropogenic forcings

More information

Earth is tilted (oblique) on its Axis!

Earth is tilted (oblique) on its Axis! MONDAY AM Radiation, Atmospheric Greenhouse Effect Earth's orbit around the Sun is slightly elliptical (not circular) Seasons & Days Why do we have seasons? Why aren't seasonal temperatures highest at

More information

Introduction to Climate ~ Part I ~

Introduction to Climate ~ Part I ~ 2015/11/16 TCC Seminar JMA Introduction to Climate ~ Part I ~ Shuhei MAEDA (MRI/JMA) Climate Research Department Meteorological Research Institute (MRI/JMA) 1 Outline of the lecture 1. Climate System (

More information

Lecture 3a: Surface Energy Balance

Lecture 3a: Surface Energy Balance Lecture 3a: Surface Energy Balance Instructor: Prof. Johnny Luo http://www.sci.ccny.cuny.edu/~luo Surface Energy Balance 1. Factors affecting surface energy balance 2. Surface heat storage 3. Surface

More information

Earth Systems Science Chapter 3

Earth Systems Science Chapter 3 Earth Systems Science Chapter 3 ELECTROMAGNETIC RADIATION: WAVES I. Global Energy Balance and the Greenhouse Effect: The Physics of the Radiation Balance of the Earth 1. Electromagnetic Radiation: waves,

More information

Climate Modeling Dr. Jehangir Ashraf Awan Pakistan Meteorological Department

Climate Modeling Dr. Jehangir Ashraf Awan Pakistan Meteorological Department Climate Modeling Dr. Jehangir Ashraf Awan Pakistan Meteorological Department Source: Slides partially taken from A. Pier Siebesma, KNMI & TU Delft Key Questions What is a climate model? What types of climate

More information

Climate Roles of Land Surface

Climate Roles of Land Surface Lecture 5: Land Surface and Cryosphere (Outline) Climate Roles Surface Energy Balance Surface Water Balance Sea Ice Land Ice (from Our Changing Planet) Surface Albedo Climate Roles of Land Surface greenhouse

More information

G109 Midterm Exam (Version A) October 10, 2006 Instructor: Dr C.M. Brown 1. Time allowed 50 mins. Total possible points: 40 number of pages: 5

G109 Midterm Exam (Version A) October 10, 2006 Instructor: Dr C.M. Brown 1. Time allowed 50 mins. Total possible points: 40 number of pages: 5 G109 Midterm Exam (Version A) October 10, 2006 Instructor: Dr C.M. Brown 1 Time allowed 50 mins. Total possible points: 40 number of pages: 5 Part A: Short Answer & Problems (12), Fill in the Blanks (6).

More information

Lecture 4: Global Energy Balance

Lecture 4: Global Energy Balance Lecture : Global Energy Balance S/ * (1-A) T A T S T A Blackbody Radiation Layer Model Greenhouse Effect Global Energy Balance terrestrial radiation cooling Solar radiation warming Global Temperature atmosphere

More information

Lecture 4: Global Energy Balance. Global Energy Balance. Solar Flux and Flux Density. Blackbody Radiation Layer Model.

Lecture 4: Global Energy Balance. Global Energy Balance. Solar Flux and Flux Density. Blackbody Radiation Layer Model. Lecture : Global Energy Balance Global Energy Balance S/ * (1-A) terrestrial radiation cooling Solar radiation warming T S Global Temperature Blackbody Radiation ocean land Layer Model energy, water, and

More information

MIDTERM PRACTICE EXAM ANSWERS

MIDTERM PRACTICE EXAM ANSWERS MIDTERM PRACTICE EXAM ANSWERS 1. (2) Location B shows that the altitude of the noon Sun increases between Dec 21. and June 21. Location B also shows that the Dec. 21 noon Sun is at an altitude of approximately

More information

Energy Systems, Structures and Processes Essential Standard: Analyze patterns of global climate change over time Learning Objective: Differentiate

Energy Systems, Structures and Processes Essential Standard: Analyze patterns of global climate change over time Learning Objective: Differentiate Energy Systems, Structures and Processes Essential Standard: Analyze patterns of global climate change over time Learning Objective: Differentiate between weather and climate Global Climate Focus Question

More information

Features of Global Warming Review. GEOG/ENST 2331 Lecture 23 Ahrens: Chapter 16

Features of Global Warming Review. GEOG/ENST 2331 Lecture 23 Ahrens: Chapter 16 Features of Global Warming Review GEOG/ENST 2331 Lecture 23 Ahrens: Chapter 16 The Greenhouse Effect 255 K 288 K Ahrens, Fig. 2.12 What can change the global energy balance? Incoming energy Solar strength

More information

Atmospheric Sciences 321. Science of Climate. Lecture 14: Surface Energy Balance Chapter 4

Atmospheric Sciences 321. Science of Climate. Lecture 14: Surface Energy Balance Chapter 4 Atmospheric Sciences 321 Science of Climate Lecture 14: Surface Energy Balance Chapter 4 Community Business Check the assignments HW #4 due Today, HW#5 is posted Quiz Today on Chapter 3, too. Mid Term

More information

Lecture 2 Global and Zonal-mean Energy Balance

Lecture 2 Global and Zonal-mean Energy Balance Lecture 2 Global and Zonal-mean Energy Balance A zero-dimensional view of the planet s energy balance RADIATIVE BALANCE Roughly 70% of the radiation received from the Sun at the top of Earth s atmosphere

More information

The Study of the Atmosphere

The Study of the Atmosphere 1 The Study of the Atmosphere Learning Goals After studying this chapter, students should be able to distinguish between weather and climate (pp. 2 5); describe how the various components of the climate

More information

Lecture 5: Greenhouse Effect

Lecture 5: Greenhouse Effect /30/2018 Lecture 5: Greenhouse Effect Global Energy Balance S/ * (1-A) terrestrial radiation cooling Solar radiation warming T S Global Temperature atmosphere Wien s Law Shortwave and Longwave Radiation

More information

Lecture 3. Background materials. Planetary radiative equilibrium TOA outgoing radiation = TOA incoming radiation Figure 3.1

Lecture 3. Background materials. Planetary radiative equilibrium TOA outgoing radiation = TOA incoming radiation Figure 3.1 Lecture 3. Changes in planetary albedo. Is there a clear signal caused by aerosols and clouds? Outline: 1. Background materials. 2. Papers for class discussion: Palle et al., Changes in Earth s reflectance

More information

Lecture 2: Global Energy Cycle

Lecture 2: Global Energy Cycle Lecture 2: Global Energy Cycle Planetary energy balance Greenhouse Effect Selective absorption Vertical energy balance Solar Flux and Flux Density Solar Luminosity (L) the constant flux of energy put out

More information

Solar Flux and Flux Density. Lecture 2: Global Energy Cycle. Solar Energy Incident On the Earth. Solar Flux Density Reaching Earth

Solar Flux and Flux Density. Lecture 2: Global Energy Cycle. Solar Energy Incident On the Earth. Solar Flux Density Reaching Earth Lecture 2: Global Energy Cycle Solar Flux and Flux Density Planetary energy balance Greenhouse Effect Selective absorption Vertical energy balance Solar Luminosity (L) the constant flux of energy put out

More information

ATMS 321 Problem Set 1 30 March 2012 due Friday 6 April. 1. Using the radii of Earth and Sun, calculate the ratio of Sun s volume to Earth s volume.

ATMS 321 Problem Set 1 30 March 2012 due Friday 6 April. 1. Using the radii of Earth and Sun, calculate the ratio of Sun s volume to Earth s volume. ATMS 321 Problem Set 1 30 March 2012 due Friday 6 April 1. Using the radii of Earth and Sun, calculate the ratio of Sun s volume to Earth s volume. 2. The Earth-Sun distance varies from its mean by ±1.75%

More information

Lecture 5: Greenhouse Effect

Lecture 5: Greenhouse Effect Lecture 5: Greenhouse Effect S/4 * (1-A) T A 4 T S 4 T A 4 Wien s Law Shortwave and Longwave Radiation Selected Absorption Greenhouse Effect Global Energy Balance terrestrial radiation cooling Solar radiation

More information

COURSE CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION

COURSE CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION COURSE CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION DATE 4 JUNE 2014 LEADER CHRIS BRIERLEY Course Outline 1. Current climate 2. Changing climate 3. Future climate change 4. Consequences 5. Human

More information

14 Heating and Cooling of Planets AND Daytime Observations

14 Heating and Cooling of Planets AND Daytime Observations Name: Date: 14 Heating and Cooling of Planets AND Daytime Observations 14.1 Heating and Cooling Introduction With this lab exercise we will investigate the ability of the radiant energy from the Sun to

More information

Topic # 12 How Climate Works

Topic # 12 How Climate Works Topic # 12 How Climate Works A Primer on How the Energy Balance Drives Atmospheric & Oceanic Circulation, Natural Climatic Processes pp 63-68 in Class Notes How do we get energy from this........ to drive

More information

Course Outline CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION. 1. Current climate. 2. Changing climate. 3. Future climate change

Course Outline CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION. 1. Current climate. 2. Changing climate. 3. Future climate change COURSE CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION DATE 4 JUNE 2014 LEADER CHRIS BRIERLEY Course Outline 1. Current climate 2. Changing climate 3. Future climate change 4. Consequences 5. Human

More information

Light Up Your World Adapted from Reflecting on Reflectivity,

Light Up Your World Adapted from Reflecting on Reflectivity, Climate Change I m Supposed To Know What That Is? Light Up Your World Adapted from Reflecting on Reflectivity, http://www.climatechangenorth.ca Overview: Students often confuse global warming and the depletion

More information

Satellite Observations and Climate Modeling: What They Can and Cannot Reveal About Future Climate

Satellite Observations and Climate Modeling: What They Can and Cannot Reveal About Future Climate Satellite Observations and Climate Modeling: What They Can and Cannot Reveal About Future Climate INCOSE Chesapeake Chapter JHU/APL March 21, 2012 Albert Arking Dept of Earth and Planetary Sciences Johns

More information

Solar Radiation and Environmental Biophysics Geo 827, MSU Jiquan Chen Oct. 6, 2015

Solar Radiation and Environmental Biophysics Geo 827, MSU Jiquan Chen Oct. 6, 2015 Solar Radiation and Environmental Biophysics Geo 827, MSU Jiquan Chen Oct. 6, 2015 1) Solar radiation basics 2) Energy balance 3) Other relevant biophysics 4) A few selected applications of RS in ecosystem

More information

ESE / GE 148a: Introduction to Climate. Organizational Details - I

ESE / GE 148a: Introduction to Climate. Organizational Details - I ESE / GE 148a: Introduction to Climate Organizational Details - I TA: Tim Merlis and Zhihong Tan Tim is a graduate student in Environmental Science and Engineering and is currently working on climate dynamics

More information

- continental vs. marine regimes

- continental vs. marine regimes (1 of 14) Further Reading: Chapter 05 of the text book Outline - continental vs. marine regimes - temperature structure of the atmosphere - seasonal variations - urban heat island (2 of 14) Introduction

More information

The inputs and outputs of energy within the earth-atmosphere system that determines the net energy available for surface processes is the Energy

The inputs and outputs of energy within the earth-atmosphere system that determines the net energy available for surface processes is the Energy Energy Balance The inputs and outputs of energy within the earth-atmosphere system that determines the net energy available for surface processes is the Energy Balance Electromagnetic Radiation Electromagnetic

More information

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

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 Word Search Directions: Below are definitions of vocabulary terms. Figure out each term and then find and circle it in the puzzle. Words may appear horizontally, vertically, or diagonally. K E M I S S

More information

Temperature Scales

Temperature Scales TEMPERATURE is a measure of the internal heat energy of a substance. The molecules that make up all matter are in constant motion. By internal heat energy, we really mean this random molecular motion.

More information

Learning goals. Good absorbers are good emitters Albedo, and energy absorbed, changes equilibrium temperature

Learning goals. Good absorbers are good emitters Albedo, and energy absorbed, changes equilibrium temperature Greenhouse effect Learning goals Good absorbers are good emitters Albedo, and energy absorbed, changes equilibrium temperature Wavelength (color) and temperature related: Wein s displacement law Sun/Hot:

More information

MIDTERM PRACTICE EXAM

MIDTERM PRACTICE EXAM MIDTERM PRACTICE EXAM PART I Multiple Choice Answer all questions in this part [60 pts] Directions (1-30): For each statement of question, select the word or expression that best completes the statement

More information

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

The Atmosphere. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems The Atmosphere 1 How big is the atmosphere? Why is it cold in Geneva? Why do mountaineers need oxygen on Everest? 2 A relatively thin layer of gas over the Earths surface Earth s radius ~ 6400km Atmospheric

More information

Atmospheric "greenhouse effect" - How the presence of an atmosphere makes Earth's surface warmer

Atmospheric greenhouse effect - How the presence of an atmosphere makes Earth's surface warmer Atmospheric "greenhouse effect" - How the presence of an atmosphere makes Earth's surface warmer Some relevant parameters and facts (see previous slide sets) (So/) 32 W m -2 is the average incoming solar

More information

G109 Alternate Midterm Exam October, 2004 Instructor: Dr C.M. Brown

G109 Alternate Midterm Exam October, 2004 Instructor: Dr C.M. Brown 1 Time allowed 50 mins. Answer ALL questions Total possible points;50 Number of pages:8 Part A: Multiple Choice (1 point each) [total 24] Answer all Questions by marking the corresponding number on the

More information

PTYS 214 Spring Announcements. Midterm 3 next Thursday!

PTYS 214 Spring Announcements. Midterm 3 next Thursday! PTYS 214 Spring 2018 Announcements Midterm 3 next Thursday! 1 Previously Habitable Zone Energy Balance Emission Temperature Greenhouse Effect Vibration/rotation bands 2 Recap: Greenhouse gases In order

More information

Sun and Earth s Climate

Sun and Earth s Climate Kevin E Trenberth Sun and Earth s Climate BAMS cover March 2009 NCAR Here comes the sun So where does all that solar radiation go? If the sun keeps shining why don t we continue to get warmer? Aaagh! But

More information

NATURAL CLIMATIC FORCING Part II

NATURAL CLIMATIC FORCING Part II TOPIC #12 NATURAL CLIMATIC FORCING Part II (p 72 in Class Notes) Today we will focus on the third main driver of NATURAL CLIMATIC FORCING: 1) ATRONOMICAL FORCING 2) SOLAR FORCING 3) VOLCANIC FORCING VOLCANIC

More information

Topic # 12 Natural Climate Processes

Topic # 12 Natural Climate Processes Topic # 12 Natural Climate Processes A Primer on How the Energy Balance Drives Atmospheric & Oceanic Circulation, Natural Climatic Processes pp 63-68 in Class Notes RADIATION / ENERGY BALANCE Radiation

More information

Climate Change a review

Climate Change a review a review AIChE Dallas Local Section September 2017 Page 2 AIChE Dallas Local Section September 2017 Page 3 AIChE Dallas Local Section September 2017 Page 4 How will it affect me What do we know Sun Earth

More information

Chapter 3. Multiple Choice Questions

Chapter 3. Multiple Choice Questions Chapter 3 Multiple Choice Questions 1. In the case of electromagnetic energy, an object that is hot: a. radiates much more energy than a cool object b. radiates much less energy than a cool object c. radiates

More information

Climate and the Atmosphere

Climate and the Atmosphere Climate and Biomes Climate Objectives: Understand how weather is affected by: 1. Variations in the amount of incoming solar radiation 2. The earth s annual path around the sun 3. The earth s daily rotation

More information

Lecture 7: Natural Climate Change. Instructor: Prof. Johnny Luo.

Lecture 7: Natural Climate Change. Instructor: Prof. Johnny Luo. Lecture 7: Natural Climate Change Instructor: Prof. Johnny Luo http://www.sci.ccny.cuny.edu/~luo Final Exam: May 23 1-3:15pm at MR O44 Outlines (Chapter 11, Edition 1) 1. Variation in solar luminosity

More information

ATMS 321: Sci. of Climate Final Examination Study Guide Page 1 of 4

ATMS 321: Sci. of Climate Final Examination Study Guide Page 1 of 4 ATMS 321: Sci. of Climate Final Examination Study Guide Page 1 of 4 Atmospheric Sciences 321: Final Examination Study Guide The final examination will consist of similar questions Science of Climate Multiple

More information

Factors That Affect Climate

Factors That Affect Climate Factors That Affect Climate Factors That Affect Climate Latitude As latitude (horizontal lines) increases, the intensity of solar energy decreases. The tropical zone is between the tropic of Cancer and

More information

The Atmosphere. Importance of our. 4 Layers of the Atmosphere. Introduction to atmosphere, weather, and climate. What makes up the atmosphere?

The Atmosphere. Importance of our. 4 Layers of the Atmosphere. Introduction to atmosphere, weather, and climate. What makes up the atmosphere? The Atmosphere Introduction to atmosphere, weather, and climate Where is the atmosphere? Everywhere! Completely surrounds Earth February 20, 2010 What makes up the atmosphere? Argon Inert gas 1% Variable

More information

Atmospheric Sciences 321. Science of Climate. Lecture 13: Surface Energy Balance Chapter 4

Atmospheric Sciences 321. Science of Climate. Lecture 13: Surface Energy Balance Chapter 4 Atmospheric Sciences 321 Science of Climate Lecture 13: Surface Energy Balance Chapter 4 Community Business Check the assignments HW #4 due Wednesday Quiz #2 Wednesday Mid Term is Wednesday May 6 Practice

More information

Radiative-Convective Models. The Hydrological Cycle Hadley Circulation. Manabe and Strickler (1964) Course Notes chapter 5.1

Radiative-Convective Models. The Hydrological Cycle Hadley Circulation. Manabe and Strickler (1964) Course Notes chapter 5.1 Climate Modeling Lecture 8 Radiative-Convective Models Manabe and Strickler (1964) Course Notes chapter 5.1 The Hydrological Cycle Hadley Circulation Prepare for Mid-Term (Friday 9 am) Review Course Notes

More information

The Structure and Motion of the Atmosphere OCEA 101

The Structure and Motion of the Atmosphere OCEA 101 The Structure and Motion of the Atmosphere OCEA 101 Why should you care? - the atmosphere is the primary driving force for the ocean circulation. - the atmosphere controls geographical variations in ocean

More information

Lecture 10. Surface Energy Balance (Garratt )

Lecture 10. Surface Energy Balance (Garratt ) Lecture 10. Surface Energy Balance (Garratt 5.1-5.2) The balance of energy at the earth s surface is inextricably linked to the overlying atmospheric boundary layer. In this lecture, we consider the energy

More information

Surface Processes and the Hydrosphere Unit Heating the Earth s Atmosphere Chapter 11 (pg )

Surface Processes and the Hydrosphere Unit Heating the Earth s Atmosphere Chapter 11 (pg ) Name: Block: Surface Processes and the Hydrosphere Unit Heating the Earth s Atmosphere Chapter 11 (pg. 352 385) 11.1: Focus on the Atmosphere: Weather and Climate What is the difference between the weather

More information

Global Energy Balance. GEOG/ENST 2331: Lecture 4 Ahrens: Chapter 2

Global Energy Balance. GEOG/ENST 2331: Lecture 4 Ahrens: Chapter 2 Global Energy Balance GEOG/ENST 2331: Lecture 4 Ahrens: Chapter 2 Solstices and Equinoxes Winter Solstice was on December 21 last year 8 hours 22 minutes of daylight March (Vernal) Equinox: March 20 this

More information

Agronomy 406 World Climates January 11, 2018

Agronomy 406 World Climates January 11, 2018 Agronomy 406 World Climates January 11, 2018 Greenhouse effect quiz. Atmospheric structure and Earth's energy budget. Review for today: Online textbook: 2.1.1 The heat balance at the top of the atmosphere.

More information

9/1/14. Chapter 2: Heating Earth s Surface and Atmosphere. The Atmosphere: An Introduction to Meteorology, 12 th. Lutgens Tarbuck

9/1/14. Chapter 2: Heating Earth s Surface and Atmosphere. The Atmosphere: An Introduction to Meteorology, 12 th. Lutgens Tarbuck Chapter 2: Heating Earth s Surface and Atmosphere The Atmosphere: An Introduction to Meteorology, 12 th Lutgens Tarbuck Lectures by: Heather Gallacher, Cleveland State University! Earth s two principal

More information

Earth s orbit. 2.2 Celestial mechanics. Earth s orbit. Earth s orbit. Variation of eccentricity over Earth s history. 0 e 1

Earth s orbit. 2.2 Celestial mechanics. Earth s orbit. Earth s orbit. Variation of eccentricity over Earth s history. 0 e 1 around the un:. Celestial mechanics Earth's orbit is an ellipse and the sun is located in one of its focal points. Definition Ellipse: The sum of the distances from any point on the ellipse to the two

More information

Insolation and Temperature variation. The Sun & Insolation. The Sun (cont.) The Sun

Insolation and Temperature variation. The Sun & Insolation. The Sun (cont.) The Sun Insolation and Temperature variation Atmosphere: blanket of air surrounding earth Without our atmosphere: cold, quiet, cratered place Dynamic: currents and circulation cells June 23, 2008 Atmosphere important

More information

The Climate in a World without Ozone

The Climate in a World without Ozone The Climate in a World without Ozone Frank Selten, Richard Bintanja, Dewi Le Bars, Hylke de Vries, Michiel van Weele (KNMI) Aarnout van Delden (Univ. Utrecht) QOS 2016, 5-9 September 2016, Edinburgh Study

More information

Lecture notes: Interception and evapotranspiration

Lecture notes: Interception and evapotranspiration Lecture notes: Interception and evapotranspiration I. Vegetation canopy interception (I c ): Portion of incident precipitation (P) physically intercepted, stored and ultimately evaporated from vegetation

More information

Radiative Balance and the Faint Young Sun Paradox

Radiative Balance and the Faint Young Sun Paradox Radiative Balance and the Faint Young Sun Paradox Solar Irradiance Inverse Square Law Faint Young Sun Early Atmosphere Earth, Water, and Life 1. Water - essential medium for life. 2. Water - essential

More information

Radiation in climate models.

Radiation in climate models. Lecture. Radiation in climate models. Objectives:. A hierarchy of the climate models.. Radiative and radiative-convective equilibrium.. Examples of simple energy balance models.. Radiation in the atmospheric

More information

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

Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc. Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning: What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric properties

More information

Prentice Hall EARTH SCIENCE

Prentice Hall EARTH SCIENCE Prentice Hall EARTH SCIENCE Tarbuck Lutgens Chapter 21 Climate 21.1 Factors That Affect Climate Factors That Affect Climate Latitude As latitude increases, the intensity of solar energy decreases. The

More information