17 March Good luck!
|
|
- Elisabeth Higgins
- 6 years ago
- Views:
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
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 informationData 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 informationLecture 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 informationLecture 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 informationGlobal 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 informationElectromagnetic 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 informationLecture 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 informationRadiation, 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 informationGEOG415 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 informationRadiative 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 informationEarth 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 information1. 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 informationTorben 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 informationAT350 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 information5. 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 informationLecture 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 informationName(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
(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 informationCLIMATE 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 informationUnderstanding 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 informationObservation: 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 informationChapter 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 informationLecture 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 informationComponents 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 informationLecture 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 informationFORCING 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 informationChapter 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 informationBoundary 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 informationFriday 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);
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 informationAtmospheric "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 informationTopic # 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 informationLecture 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 informationLecture 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 information9/5/16. 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 informationEarth 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 informationIntroduction 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 informationLecture 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 informationEarth 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 informationClimate 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 informationClimate 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 informationG109 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 informationLecture 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 informationLecture 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 informationMIDTERM 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 informationEnergy 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 informationFeatures 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 informationAtmospheric 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 informationLecture 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 informationThe 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 informationLecture 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 informationLecture 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 informationLecture 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 informationSolar 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 informationATMS 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 informationLecture 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 informationCOURSE 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 information14 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 informationTopic # 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 informationCourse 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 informationLight 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 informationSatellite 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 informationSolar 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 informationESE / 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
(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 informationThe 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 informationI 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 informationTemperature 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 informationLearning 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 informationMIDTERM 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 informationThe 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 informationAtmospheric "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 informationG109 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 informationPTYS 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 informationSun 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 informationNATURAL 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 informationTopic # 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 informationClimate 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 informationChapter 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 informationClimate 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 informationLecture 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 informationATMS 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 informationFactors 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 informationThe 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 informationAtmospheric 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 informationRadiative-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 informationThe 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 informationLecture 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 informationSurface 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 informationGlobal 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 informationAgronomy 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 information9/1/14. 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 informationEarth 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 informationInsolation 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 informationThe 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 informationLecture 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 informationRadiative 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 informationRadiation 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 informationPlanetary 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 informationPrentice 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