'Equilibrium temperature' diaporamas de présentation

Last rev. 022007a

Heat, Temperature And Phase Changes. Pisgah High School Chemistry. Mr. Jones. Last rev. 022007a. Part One Heat and Temperature. What temperature does the thermometer indicate?. What might be going on that would cause this temperature?.

1.98k views • 178 slides

Abundances in the solar system: what we achieved and how much was it dependent on space probes?

Abundances in the solar system: what we achieved and how much was it dependent on space probes?. Sandrine VINATIER LESIA, Observatoire de Paris- Meudon. Introduction: a typical planet radiation. 1. ? = 0. B ? d ? / ?. ?. Introduction: thermal IR emission .

768 views • 66 slides

Exploration of the Ultracold World

IAMS. Exploration of the Ultracold World. Ying-Cheng Chen( ??? ), Institute of Atomic & Molecular Sciences, Academia Sinica 12 October, 2009, NDHU. Outline. Overview of Ultracold Atoms Introduction to Ultracold Molecules Exploration I: Molecular cooling

945 views • 56 slides

Class 4 Inertia and Responding To Climate Change

Class 4 Inertia and Responding To Climate Change. Climate Change OLLI Summer 2013. Increase in Equilibrium Temperature Due to Increase in CO 2 Concentration from 280 ppm. ? T = ? T 2X * Ln(new CO 2 concentration/280 ppm concentration )/ Ln(2.0). Ln(2.0) = 0.69.

503 views • 50 slides

Class 3 Explaining the Present (Conclusion) And Projecting the Future

Class 3 Explaining the Present (Conclusion) And Projecting the Future. Climate Change OLLI Summer 2013. (Mostly) explaining the present. The Two Previous Coolings. Understanding the event Quantitative understanding comes after the event Qualitative understanding of second event by 1970s

508 views • 50 slides

Homeostasis

449 views • 29 slides

Light, Heat and Temperatures on Earth

Light, Heat and Temperatures on Earth. Temperatures on Earth or any planet are primarily determined by 1: The irradiance of sunlight (Presented in Previous Powerpoint). 2: The rate at which planets emit radiation back to space.

405 views • 28 slides

3.3 Theory of Climate Change

1.33k views • 19 slides

Lecture 7-8: Energy balance and temperature (Ch 3)

Lecture 7-8: Energy balance and temperature (Ch 3). the diurnal cycle in net radiation, temperature and stratification the friction layer local microclimates influences on regional temperature patterns. -L*. The diurnal (daily) cycle in net radiation at the base of the atmos.

332 views • 15 slides

Calorimetry

152 views • 11 slides

Earth as a blackbody

179 views • 8 slides

Heat Capacity

Heat Capacity. The work - energy principle applies to all objects. If an object speeds up it gains kinetic energy. If an object slows down it loses kinetic energy. Work In. Work done on a system. v 1. v 2. Temperature change is due to heat (Q).

141 views • 8 slides

Latent Heat

Latent Heat. Materials can also go through a change in state called a phase change. Changes between solid, liquid, gaseous and plasma states.

399 views • 6 slides

152 views • 5 slides

150 views • 2 slides