Climate Dynamics Starts with the Sun NASA Image From Wallace and Hobbs r = 6.96x10 8 m T=5780K Photosphere Sunspots Faculae Figure 1.1.

Slides:



Advertisements
Similar presentations
Volcanoes Large volcanic eruptions with high SO2 content can release SO2 into the stratosphere. This SO2 eventually combined with water vapor to make.
Advertisements

1 Climate Change some astrophysical perspectives.
M ODULE #2: C limate Change & Global Warming …Science & Sources of Greenhouse Gas (GHG) Emissions.
Tropospheric response to Solar and Volcanic forcing
Bare rock model Assumptions
SOLAR IRRADIANCE VARIABILITY OF RELEVANCE FOR CLIMATE STUDIES N.A. Krivova.
Radiative Properties of Clouds SOEE3410 Ken Carslaw Lecture 3 of a series of 5 on clouds and climate Properties and distribution of clouds Cloud microphysics.
Remarkable Low Temperature Emission of the 4 November 2003 Limb Flare J. Leibacher, J. Harvey, GONG Team (NSO), G. Kopp (CU/LASP), H. Hudson (UCB/SSL)
Radiative Properties of Clouds SOEE3410 Ken Carslaw Lecture 3 of a series of 5 on clouds and climate Properties and distribution of clouds Cloud microphysics.
Radiative Forcing of Ozone
Radiative Properties of Clouds ENVI3410 : Lecture 9 Ken Carslaw Lecture 3 of a series of 5 on clouds and climate Properties and distribution of clouds.
MONITORING EARTH’S CLIMATE SYSTEM & PLANETARY ENERGY BUDGET.
1 Pedagogical Review on Solar Cycles King-Fai Li Caltech GPS, YL Yung Group Jan 17, 2007.
1. How has the climate changed during the recent past? 2. What can we say about current climate change? 3. How do climate models work and what are their.
Solar Radiative Output and its Variability Preethi Ganapathy November 22, 2005 Claus Frölich and Judith Lean.
Why do climates change ? Climate changes over the last millennium.
Lecture 1: Introduction to the planetary energy balance Keith P Shine, Dept of Meteorology,The University of Reading
Conversations with the Earth Tom Burbine
Solar Irradiance Variability Rodney Viereck NOAA Space Environment Center Derived Total Solar Irradiance Hoyt and Schatten, 1993 (-5 W/m 2 ) Lean et al.,
The Deniers Cycles Within Cycles. Premise… Solar variability and long-term variation in solar luminosity are the key drivers of climate change.
Earth’s Energy Budget Earth has 2 heat engines: – Internal – External Internal Heat Engine – Energy that drives plate tectonics – Source = radioactive.
The Sun The center of our solar system A main sequence yellow star Is powered through Nuclear fusion. A reaction where 2 atoms of Hydrogen are forced together.
The Sun: Part 3 and Measuring the Stars: Part 1. Net result: 4 protons → 4 He + 2 neutrinos + energy Hydrostatic Equilibrium: pressure from fusion reactions.
Introduction to Climate Change and its Impact on Society Jagadish Shukla Center of Ocean-Land- Atmosphere studies Lecture2: Aug 28, 2008 CLIM 101: Weather,
CE 401 Climate Change Science and Engineering solar input, mean energy budget, orbital variations, radiative forcing January 2011.
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.
Sustainability and Globalization Global Warming. A global issue with regards to sustainability A world-wide warming of the Earth’s lower atmosphere.
Alan Robock Department of Environmental Sciences Rutgers University, New Brunswick, New Jersey USA
The thermodynamic equation for seawater where is the irreversible internal energy fluxes driven by temperature gradient, i.e., diffusion of heat. F S radiative.
CE 401 Climate Change Science and Engineering solar input, mean energy budget, orbital variations, radiative forcing January 2012.
Solar Irradiance Variability and Climate
CLIMATE CHANGE THE GREAT DEBATE Session 7. SOLAR POWER The Sun is the primary driving force of climate and sits in the centre of the solar system that.
THE SUN. The Photosphere The Photosphere - The “visible” surface of the sun.  Thin layer of gas (less than 500km deep) from which we receive the majority.
Physics of Planetary Climate Cors221: Physics in Everyday Life Fall 2010 Module 3 Lecture 8: Climate During This Interglacial.
V/1 Atmospheric transport and chemistry lecture I.Introduction II.Fundamental concepts in atmospheric dynamics: Brewer-Dobson circulation and waves III.Radiative.
TOPIC III THE GREENHOUSE EFFECT. SOLAR IRRADIANCE SPECTRA 1  m = 1000 nm = m Note: 1 W = 1 J s -1.
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.
SOLAR VARIABILITY AND CLIMATE. HAS THE EARTH WARMED? Climatic Research Unit, UK.
A Presentation by the _________ Crew _____, _______, _______, _________ ______________________________.
Modelling the climate system and climate change PRECIS Workshop Tanzania Meteorological Agency, 29 th June – 3 rd July 2015.
More Radiation EGR 4345 Heat Transfer.
VII. Climate Change Blackbody model Windows and saturation Feedbacks Aerosols.
SOLSTICE II -- Magnesium II M. Snow 1*, J. Machol 2,3, R. Viereck 4, M. Weber 5, E. Richard 1 1 Laboratory for Atmospheric and Space Physics, University.
PHY134 Introductory Astronomy Light and Matter 1.
The Sun: Part 2. Temperature at surface = 5800 K => yellow (Wien’s Law) Temperature at center = 15,000,000 K Average density = 1.4 g/cm 3 Density at center.
CE 401 Climate Change Science and Engineering solar input, mean energy budget, orbital variations, radiative forcing 20 January 2011.
Man Made Climate Change vs. Natural Variability Presented By: Mark Seaman Sam Atwood EESC W4400.
The Helioseismic and Magnetic Imager (HMI) on NASA’s Solar Dynamics Observatory (SDO) has continuously measured the vector magnetic field, intensity, and.
Global Change: Class Exercise Global Energy Balance & Planetary Temperature Mteor/Agron/Envsci/Envst 404/504.
1 Weather, Climate & Society ATMO 325 Global Energy Balance Greenhouse Effect.
The Solar System The Moon The Earth The Sun How do they move? Why doesn’t the Earth fly away? Photos by NASA.
© 2014 Pearson Education, Inc. The Oceans and Climate Change Chapter 1 Clickers Essentials of Oceanography Eleventh Edition Alan P. Trujillo Harold V.
Planck’s law  Very early in the twentieth century, Max Karl Ernest Ludwig Planck put forth the idea of the quantum theory of radiation.  It basically.
Solar Constant Emissivity Albedo
© 2014 Pearson Education, Inc. Chapter 16 The Oceans and Climate Change.
Solar variability and its impact on climate Laura Balmaceda 4 th El Leoncito Solar Physics School November, 2008.
To recap Give 2 examples of research methods that show long term historical climate change? How reliable are these? Give 2 ways of measuring medium term.
To what extent does solar variability contribute to climate change? Dr. David H. Hathaway NASA/Marshall Space Flight Center National Space Science and.
SOLAR CONSTANT Wm W m -2 is radiated on a plane tangent to the Earth at all times – the “Solar Constant.” This amounts to only.
Energy sources, fluxes, and sinks
Disconnects in Sun-Climate Studies: Removing Politics from Science
Developing Sunspot March 27
Surface Temperature and Blackbodies Surface temperature: the temperature of the visible disk of the Sun (photosphere) blackbody: a perfect radiator.
Climate: Earth’s Dynamic Equilibrium
Magnetic Field.
Climate Changes due to Natural Processes
The Sun: source of it all…
Orbital Changes Changes in how the Earth moves around the Sun are believed to cause ice ages. According to Milankovitch (a Serbian physicist), every 100,000.
TIMED SABER Data Enables Scientists to Derive a 70-year Time Series of the Thermosphere’s Infrared Energy Budget With its long, comprehensive dataset,
Natural climate change
Presentation transcript:

Climate Dynamics Starts with the Sun NASA Image From Wallace and Hobbs r = 6.96x10 8 m T=5780K Photosphere Sunspots Faculae Figure 1.1

Integration of Intensity over a Hemisphere to Get Net Downward Energy Flux Density in W/m 2. 1 m 2 area We want Watts per m 2. Figure 1.2

Sun and Earth Blackbody Spectra, Trace Gas Absorption Lines From Wallace and Hobbs Figure 1.3

Climate Dynamics Starts with the Sun NASA Image From Wallace and Hobbs r = 6.96x10 8 m T=5780K Photosphere Sunspots Faculae Figure 1.4

The Earth’s Orbit is Elliptical Figure 1.5

Measurement of the Solar Constant from Satellite is Difficult Figure 1.6 Improved Instrument More Scattering, Higher Irradiance Measured Kopp and Lean (2010)

Recent Solar Constant Measurements from the SORCE Experiment Figure 1.7 Courtesy of Greg Kopp (LASP)

Climate Dynamics Starts with the Sun NASA Image From Wallace and Hobbs r = 6.96x10 8 m T=5780K Photosphere Sunspots Faculae Figure 1.8

11-Year Sunspot Cycle Indicates Variations in Solar Luminosity Percent Area of Photosphere Covered by Sunspots Fraction Area of Entire Photosphere Covered by Sunspots Yellow >1% Figure 1.9

Direct Measurements of Solar “Constant” IPCC 2013 Satellite Retrievals Figure 1.10

Solar “Constant” Reconstructions Suggest Stronger Longer-Term Variations IPCC 2007 Figure 1.11

IPCC 2013 Figure 1.12 Solar Forcing Since 1750 is Relatively Small Compared to Other External Perturbations to the Climate System. *Volcanic Ignored.