Climate Dynamics 11:670:461 Alan Robock

Slides:



Advertisements
Similar presentations
Alan Robock Department of Environmental Sciences Rutgers University, New Brunswick, New Jersey USA
Advertisements

Alan Robock Department of Environmental Sciences Rutgers University, New Brunswick, New Jersey USA
Alan Robock Department of Environmental Sciences Rutgers University, New Brunswick, New Jersey USA
Energy Budget of the Earth-Atmosphere System
Alan Robock Department of Environmental Sciences Rutgers University, New Brunswick, New Jersey USA
Solar radiation and earth energy balance 1) Paul’s Demo 2) Magnitude of Solar Radiation ( Estimate of the power of Garden lights ) 2) Earth energy balance.
Energy Budget of the Earth- Atmosphere System. Energy Transfer Conduction -- direct molecular transfer Convection -- fluids; air or water –Sensible heat.
The Global Heat Budget Air-sea exchanges of heat (& freshwater) create deep water masses & drive the conveyor belt Heat source into the ocean is solar.
Climate Earth’s Radiation Balance. Solar Radiation Budget Life on earth is supported by energy from the sun Energy from the sun is not simply absorbed.
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.
1. weather or climate ? Annual mean temperature (red is warm, blue cold)
1. Introduction to the Climate System 1.1 Introduction 1.2 Overview of Midlatitude Climate 1.3 Overview of Tropical Climate Key Concepts from today’s Lecture:
5.7 PW5.9 PW The seasonal cycle of energy fluxes in the high latitudes Aaron Donohoe I.) How do the absorbed solar (ASR), outgoing longwave (OLR), and.
3. Climate Change 3.1 Observations 3.2 Theory of Climate Change 3.3 Climate Change Prediction 3.4 The IPCC Process.
Earth Systems Science Chapter 3 I. Global Energy Balance and the Greenhouse Effect: The Physics of the Radiation Balance of the Earth 1.Electromagnetic.
Thermohaline Circulation
1 Weather and Climate Bay Area Earth Science Institute (BAESI) Energy in the Atmosphere San Jose State University, January 24, 2004
Energy in the Ocean- Atmosphere Climate System SOEE3410 : Lecture 2 Dr Ian Brooks Room 1.64a Environment Building
What controls the total heat transport in CMIP3 models Aaron Donohoe AGU 2010 – 12/12/2010.
THE RADIATION BUDGET (Exercise) Exercise: Monitor radiation budget at 2 sites (urban rural) using instruments.
Incoming Solar Energy What affects the amount of incoming solar energy?
Lecture 1: Introduction to the planetary energy balance Keith P Shine, Dept of Meteorology,The University of Reading
Physical Geography by Alan Arbogast Chapter 5
Pat Arnott, ATMS 749 Atmospheric Radiation Transfer ATMS 749 Atmospheric Radiation Transfer.
Chapter 4 Atmosphere and Surface Energy Balances Robert W. Christopherson Charlie Thomsen.
South North East West Sunrise Sunset Azimuth Angle (From South) Altitude altitude angle horizontal surface perpendicular to surface zenith angle Sun Figure.
Solar Radiation and Energy Balance Unit 3: Weather and Climate Geo 12 Ms. Thind.
Radiation Group 3: Manabe and Wetherald (1975) and Trenberth and Fasullo (2009) – What is the energy balance of the climate system? How is it altered by.
On the Radiative and Dynamical Feedbacks over the Equatorial Pacific Cold Tongue De-Zheng Sun John Fasullo Tao Zhang Andres Roubicek J. Climate, 2003,
The Greenhouse Effect. What controls climate? Energy from the Sun – Radiation! Consider the 4 inner planets of the solar system: SUN 342 W m W.
Alan Robock Department of Environmental Sciences Rutgers University, New Brunswick, New Jersey USA
Advanced Hydrology Lecture 1: Water Balance 1:30 pm, May 12, 2011 Lecture: Pat YEH Special-appointed Associate Professor, OKI Lab., IIS (Institute of Industrial.
Chapter 3 Atmospheric Energy and Global Temperatures.
ATMOSPHERE HEATING RATE: CLOUD FREE ATMOSPHERE. Words and Equation from Petty: Radiative Heating Rate.
Lecture 3 read Hartmann Ch.2 and A&K Ch.2 Brief review of blackbody radiation Earth’s energy balance TOA: top-of-atmosphere –Total flux in (solar or SW)=
Climate: It’s All About the Sun!!! Or, Is It? Chris Fairall, NOAA ESRL Introduction, background on climate system Black body radiation basics The sun vs.
Surface energy balance (2). Review of last lecture –What is energy? 3 methods of energy transfer –The names of the 6 wavelength categories in the electromagnetic.
Chapter 3 Atmospheric Energy and Global Temperatures
The Radiation Budget and the Greenhouse Effect SNC2D.
© Oxford University Press, All rights reserved. 1 Chapter 3 CHAPTER 3 THE GLOBAL ENERGY SYSTEM.
Global-mean energy balance. Spatial Radiation Imbalance Distribution of solar forcing as function of latitude.
Introduction to Climate and Environmental Physics HS 2014 Lecture II Christoph Raible, Markus Leuenberger, Fortunat Joos and Thomas Stocker.
Alan Robock Department of Environmental Sciences Rutgers University, New Brunswick, New Jersey USA
The Greenhouse Effect. Natural heating of earth’s surface caused by greenhouse gases –CO 2 (Carbon Dioxide) –CH 3 (Methane) –N 2 O (Nitrous Oxide) –H.
The Atmosphere: One component of the climate system Composition / Structure Radiative transfer Vertical and latitudinal heat transport Atmospheric circulation.
Alan Robock Department of Environmental Sciences Rutgers University, New Brunswick, New Jersey USA
A Little Climate Physics Kerry is this your original? If not, something selected from
1. Introduction to the Climate System
BAESI - Global Warming: Food Climate Connections
Planetary albedo (a) is the average reflectivity of the Earth = 107/342  0.3 Earth’s global, annual mean energy balance.
Natural Environments: The Atmosphere
Global energy balance SPACE
Natural Environments: The Atmosphere
Climate Dynamics 11:670:461 Alan Robock
Lecture 6: Energy balance and temperature (Ch 3)
Solar energy drives the world’s climate…
Climate Dynamics 11:670:461 Alan Robock
Climate Dynamics 11:670:461 Alan Robock
ATOC 4720 class29 1. How the energy balance is achieved in the earth-atmosphere system 2. The energy balance of the upper atmosphere 3. The energy balance.
Energy Balance and Circulation Systems
Climate Dynamics 11:670:461 Alan Robock
Earth’s Energy Budget.
GLOBAL ENERGY BUDGET - 2 The Greenhouse Effect.
Climate Dynamics 11:670:461 Alan Robock
Climate Dynamics 11:670:461 Alan Robock
Sun Earth Sun: shortwave radiation Earth: longwave radiation.
ATM OCN Fall 2000 LECTURE 8 ATMOSPHERIC ENERGETICS: RADIATION & ENERGY BUDGETS A. INTRODUCTION: What maintains life? How does Planet Earth maintain.
Climate Dynamics 11:670:461 Alan Robock
1. Introduction to the Climate System
Unit 5 Earth’s Energy Budget.
Presentation transcript:

Climate Dynamics 11:670:461 Alan Robock robock@envsci.rutgers.edu Lecture 9, 10/3/13 Climate Dynamics 11:670:461 Alan Robock Department of Environmental Sciences Rutgers University, New Brunswick, New Jersey USA robock@envsci.rutgers.edu http://envsci.rutgers.edu/~robock

Fig. 5.3

Climatological annual mean energy budget for 2000–2005 (W/m2) Climatological annual mean energy budget for 2000–2005 (W/m2). (Trenberth & Fasullo, 2011) https://climatedataguide.ucar.edu/climate-data/budgets-mass-moisture-energy

Global, annual average heat balance (W/m2) Fig. 5.4

Planetary albedo (a) is the average reflectivity of the Earth = 102/341 = 0.30 Climatological annual mean energy budget for 2000–2005 (W/m2). (Trenberth & Fasullo, 2011) https://climatedataguide.ucar.edu/climate-data/budgets-mass-moisture-energy

Total = 341 W m‑2 – (239 + 102) W m‑2 = 0 W m‑2 Outer Space: Total = 341 W m‑2 – (239 + 102) W m‑2 = 0 W m‑2 Climatological annual mean energy budget for 2000–2005 (W/m2). (Trenberth & Fasullo, 2011) https://climatedataguide.ucar.edu/climate-data/budgets-mass-moisture-energy

Total = 341.3 W m‑2 – (238.5 + 101.9) W m‑2 = -0.9 W m‑2 Outer Space: Total = 341.3 W m‑2 – (238.5 + 101.9) W m‑2 = -0.9 W m‑2 Climatological annual mean energy budget for 2000–2005 (W/m2). (Trenberth & Fasullo, 2011) https://climatedataguide.ucar.edu/climate-data/budgets-mass-moisture-energy

Total = (78 + 17 + 80 + 374) W m‑2 - (187 + 30 + 333) W m‑2 = -1 W m‑2 Atmosphere: Total = (78 + 17 + 80 + 374) W m‑2 - (187 + 30 + 333) W m‑2 = -1 W m‑2 Climatological annual mean energy budget for 2000–2005 (W/m2). (Trenberth & Fasullo, 2011) https://climatedataguide.ucar.edu/climate-data/budgets-mass-moisture-energy

Total = (161 + 333) W m‑2 - (17 + 80 + 396) W m‑2 = 1 W m‑2 Surface: Total = (161 + 333) W m‑2 - (17 + 80 + 396) W m‑2 = 1 W m‑2 T = 255 K T = 288 K Greenhouse effect Climatological annual mean energy budget for 2000–2005 (W/m2). (Trenberth & Fasullo, 2011) https://climatedataguide.ucar.edu/climate-data/budgets-mass-moisture-energy

Annual average incident solar radiation (W/m2) Annual average absorbed solar radiation at top of atmosphere (W/m2) Fig. 5.5

Planetary albedo (%) Fig. 5.6

Dependence of water albedo on solar zenith angle, θZ Fig. 5.7

Annual mean outgoing longwave radiation (W/m2) Fig. 5.8

Net radiation at top of atmosphere (W/m2) Fig. 5.9

Net radiation at top of atmosphere (W/m2) Fig. 5.9

Solar radiation absorbed at surface, SABS (W/m2) Fig. 5.10

Outgoing longwave radiation at surface, esT4 (W/m2) Fig. 5.11a

Downward back radiation at surface, FBACK (W/m2) Fig. 5.11b

Sensible heat flux at surface, HS (W/m2) Fig. 5.12a

Latent heat flux at surface, HL (W/m2) Fig. 5.12b

Horizontal and vertical heat fluxes at surface, FH + FV (W/m2) Fig. 5.13

A thermally direct circulation Fig. 7.1

Annual mean, zonal mean meridional (m/s) and vertical velocities (interval 5 x 10-3 Pa/s) Fig. 7.2

Zonal mean stream function (x 1010 kg/s), positive is clockwise. Fig. 7.3

http://www.physicalgeography.net/fundamentals/7p.html

http://www.physicalgeography.net/fundamentals/7p.html

http://www.geogonline.org.uk/g3a_ki2.1.htm

http://www. personal. psu http://www.personal.psu.edu/czn115/blogs/meteo241/2010/10/e-portfolio-2.html