Temperature Change. Heat (Q) Latent Heat. Latent Heat. Heat Fluxes Transfer of heat in/out of the ocean Flux = Quantity/(Area Time) Latent heat

Similar documents
Global Climate Change

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

Lecture 4: Global Energy Balance

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

1. Weather and climate.

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

HEAT, TEMPERATURE, AND ATMOSPHERIC CIRCULATION

The Ocean-Atmosphere System II: Oceanic Heat Budget

Lecture 9: Climate Sensitivity and Feedback Mechanisms

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

Lecture 5: Greenhouse Effect

Lecture 5: Greenhouse Effect

1) The energy balance at the TOA is: 4 (1 α) = σt (1 0.3) = ( ) 4. (1 α) 4σ = ( S 0 = 255 T 1

Energy Balance and Temperature. Ch. 3: Energy Balance. Ch. 3: Temperature. Controls of Temperature

Energy Balance and Temperature

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

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

Understanding the Greenhouse Effect

COURSE CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION

Earth s Energy Balance and the Atmosphere

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

Earth s Heat Budget. What causes the seasons? Seasons

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?

Course Outline. About Me. Today s Outline CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION. 1. Current climate. 2.

Torben Königk Rossby Centre/ SMHI

Boundary layer equilibrium [2005] over tropical oceans

Earth Systems Science Chapter 3

Glaciology HEAT BUDGET AND RADIATION

Earth s Heat Budget. What causes the seasons? Seasons

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

Lecture 3: Global Energy Cycle

Chapter 2 Solar and Infrared Radiation

Lecture 7: The Monash Simple Climate

Lecture 4: Heat, and Radiation

Lecture 2: Global Energy Cycle

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

Lecture 2 Global and Zonal-mean Energy Balance

Lecture 10: Climate Sensitivity and Feedback

Lecture 2: Global Energy Cycle

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

THE EXOSPHERIC HEAT BUDGET

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

Composition, Structure and Energy. ATS 351 Lecture 2 September 14, 2009

Climate Change: Past and Future ERTH 303, 3 December, 2009

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

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

Earth: the Goldilocks Planet

Lecture 3a: Surface Energy Balance

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

Radiative Balance and the Faint Young Sun Paradox

PTYS 214 Spring Announcements. Midterm 3 next Thursday!

Chapter 9 External Energy Fuels Weather and Climate

Energy. Kinetic and Potential Energy. Kinetic Energy. Kinetic energy the energy of motion

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

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

GEO1010 tirsdag

Radiative equilibrium Some thermodynamics review Radiative-convective equilibrium. Goal: Develop a 1D description of the [tropical] atmosphere

Lecture 4: Radiation Transfer

Climate System. Sophie Zechmeister-Boltenstern

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

CHAPTER 1 - GEOPHYSICAL PERSPECTIVE

2/18/2013 Estimating Climate Sensitivity From Past Climates Outline

Chapter 11 Lecture Outline. Heating the Atmosphere

Radiation in climate models.

Climate Dynamics (PCC 587): Clouds and Feedbacks

Chapter 3. Multiple Choice Questions

The Planck Blackbody Equation and Atmospheric Radiative Transfer

Radiation, Sensible Heat Flux and Evapotranspiration

Climate Roles of Land Surface

Atmospheric Radiation

MAPH & & & & & & 02 LECTURE

Earth s Heat Budget. What causes the seasons?

- global radiative energy balance

Lecture 2: Light And Air

Chapter 3- Energy Balance and Temperature

ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY. Lecture 19. Learning objectives: develop a physical understanding of ocean thermodynamic processes

Let s make a simple climate model for Earth.

2. What does a mercury barometer measure? Describe this device and explain how it physically works.

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

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

Spectrum of Radiation. Importance of Radiation Transfer. Radiation Intensity and Wavelength. Lecture 3: Atmospheric Radiative Transfer and Climate

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

Lecture 3: Atmospheric Radiative Transfer and Climate

Climate Models & Climate Sensitivity: A Review

The Arctic Energy Budget

Climate Change 2007: The Physical Science Basis

Climate Dynamics (PCC 587): Feedbacks & Clouds

GE510 Physical Principles of the Envt

ATOC OUR CHANGING ENVIRONMENT Class 19 (Chp 6) Objectives of Today s Class: The Cryosphere [1] Components, time scales; [2] Seasonal snow

Equation for Global Warming

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

Radiation in the atmosphere

Thursday, November 1st.

Northern New England Climate: Past, Present, and Future. Basic Concepts

Take away concepts. What is Energy? Solar Radiation Emission and Absorption. Energy: The ability to do work

Climate Modeling Dr. Jehangir Ashraf Awan Pakistan Meteorological Department

Earth s Climate Patterns

Chapter 7: Thermodynamics

Monitoring Climate Change from Space

Transcription:

Heat (Q) 1 calorie = 4.18 Joule Heat : Total Kinetic Energy Temperature: Average Kinetic Energy Heat that causes a change in temperature: Sensible Heat Temperature Change ΔQ = m c water ΔT Q in Joules c water = 4186 J/kg C m = mass. Per unit volume: m/vol = density of the water ΔQ = ρ c water ΔT vol The heat absorbed or released in the change of phase of water. Latent heat of fusion = 80cal/gm Latent heat of evaporation= 540 cal/gm The 1 gm ice cube is 0 C. What happens if it absorbs 5 cal of heat? Latent heat Transfer of heat in/out of the ocean Flux = Quantity/(Area Time) Heat Flux = Joule /(m 2 s) 1 Watt = 1 Joule/s Heat Flux = W/m 2 1

Transfer of heat in/out of the ocean surface Heat In - One Heat Flux Shortwave Radiation or Insolation (Qs) Heat Out - Three Longwave or Back Radiation (Qb) These are the 2 heat fluxes involving Radiation Transfer of heat in/out of the ocean surface Shortwave Radiation or Insolation (Qs) Longwave or Back Radiation (Qb) Flux (Qe) Sensible Heat Flux (Qh) Heat In = Heat Out Heat In = Heat Out is not true for the short-term Smaller Region of Ocean Sept: Measurements show Qs = Qb + Qe +Qh. What happens to the Bay s temperature? June: Measurements show Qs > Qb + Qe +Qh. What happens to the Bay s temperature? June: Measurements show the Bay s temperature was constant. How?? Advective Heat Flux Qv Qv is the only heat flux that does not transfer heat in and out of the ocean (through the surface) Qv transfers heat in and out of a region 20 200 180 Bay +/- = 0 2

Qs - Qb - Qe - Qh Heating by Latitude Cooling Annual Average Unequal Surface Heating/Cooling Produces: Wind Driven Circulation (surface currents) Pump heat poleward Thermohaline Circulation (deep currents) Pump cold water equatorward Oceans circulate to redistribute heat, caused by the unequal heating/cooling at the surface. Transfer of heat in/out of the ocean surface Shortwave Radiation or Insolation (Qs) Longwave or Back Radiation (Qb) Flux (Qe) Sensible Heat Flux (Qh) Heat In = Heat Out Stefan-Boltzmann Law Q (W/m 2 ) = ct 4 ( K) C =5.67 x 10-8 W/m 2 K 4 EM Spectrum 3

Wien s Law 2897.8µ m λ ( µ m) =! T( K) Energy Spectra What gives off longer wavelength energy, the Earth (10 C) or the Sun (6000 C)? Shortwave Radiation Once the Sun s radiation reaches Earth: A certain % is reflected away A certain % is absorbed in the atmosphere and is converted to heat The remainder is absorbed by the land/ ocean (Qs) Shortwave Budget Albedo + + Transmissivity = 100% Albedo Qs Absorptivity Transmissivity Annual Global Average Radiative Budget 4

Flux (W/m 2 ) Q e = E L ρ E - evaporation rate L - latent heat of evaporation (540 cal/gm) ρ - density Q e = c e (q s - q a )W c e = 1.5 x 10-3 q s = saturation vapor pressure (mb) q a = actual vapor pressure (mb) W = wind speed (m/s) Vapor Pressure Vapor Pressure - the air pressure produced by all the water vapor in the air (a portion of the total air pressure). It is a measure of how much water is in the air. Unit is millibar. Saturation Vapor Pressure - the maximum amount of water vapor that can be in the air (i.e. when humidity is 100%). Its value depends on the air temperature Actual Vapor Pressure - the actual amount of water vapor in the air Sat. Vapor Pressure When humidity = 90% is (qs - qa) a large or small value?. Saturation (q s ) Qe = c(q s - q a )W When (q s - q a ) is small, air is close to saturation, humidity is high, evaporation is small. Unsaturated When (q s - q a ) is large, air is dry, humidity is low, easy to evaporate (q s - q a ) is the opposite of humidity Qe and Temperature Temp and Humidity Late at night the temperature in Conway suddenly plummets. What happens to the latent heat flux? Why? T down, qs qa down, humidity up, Qs down The latent heat flux IS dependent on temperature, although temperature is not in the equation. 5

Sensible Heat Flux (conduction/convection) Q h = c h (T s - T a )W c h = 1.2 x 10-3 T s = sea temperature T a = air temperature W = wind speed When Ts > Ta, the sensible heat flux represents cooling Bowen s Ratio B = Q h /Q e (Global Annual Averages) For every 100 units of Energy that reach Earth: 7 units leave the oceans as Qh Radiative Budget 22 7 For every 100 units of Energy that reach Earth: (Global Annual Averages) 22 units leave the oceans as Qe Radiative Budget 7 units leave the oceans as Qh (smallest of the 3 cooling terms) These fluxes do not transfer energy in/out of Earth system, but transfer energy from the oceans to the atmosphere. Calculating Back Radiation (Qb) Radiation leaving ocean (W/m 2 )= c sb T( K) 4 K = C + 273 Need to know the % that returns to Earth (or escapes & becomes heat) to estimate Qb Qb = Radiation leaving ocean - radiation returned to ocean Global Heat Budget Heat In = Heat Out Qs = Qe + Qb + Qh On average: Qs= (44%)Qe + (42%)Qb + (14%)Qh (W/m 2 ) 6

Temperature Increase The global average temperature rose 1 C in the 20th century. The global average temperature rose.7 C in the last 3 decades. This is the fastest warming rate in the last 1000 years. 15 out of 16 of warmest years on record have occurred since 2005. Mauna Loa Co2 CO2 Concentrations CO2 Long term 401 ppm 7

Co2 CO2 Future The observed warming last century could be largely due to natural variability, alternatively emissions of greenhouse gases from human activities may be enhancing greenhouse warming. 1st IPCC Assessment Report, 1990 Although both natural forcings and changes in the Sun s output might be contributing to climate change, the balance of evidence suggests a discernable human influence on climate. 2nd IPCC Assessment Report, 1995 The 1990 s were the warmest decade on record and the recent climate change is partly attributable to human activities. 3rd IPCC Assessment Report, 2001 Warming of the climate system is unequivocal. Concentrations of greenhouse gases have increased markedly as a result of human activities. The understanding of human impact on climate has improved since the 3rd report, leading to a 90% likelihood that the observed warming has been due to human activity. 4th IPCC Assessment Report, 2007 8

Greenland Ice Mass 2002-2014 Sea Level Change Spring Maid Pier, S.C. 5.2 mm/year (1.7 feet/century) Last century in S.C. sea level rose at 2-3 x the global average Average: ~ 2 mm/yr Current: 3 mm/yr 9