'Displacement law' diaporamas de présentation

Climate, Climate Change Nuclear Power and the Alternatives

Climate, Climate Change Nuclear Power and the Alternatives. Climate, Climate Change Nuclear Power and the Alternatives. PHYC 40050 Peter Lynch Meteorology & Climate Centre School of Mathematical Sciences University College Dublin. The Energy Cycle of the Atmosphere. Lecture 2.

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Blackbody Radiation

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Radiation Laws Scattering Absorption Radiation Windows Reflectance Terrain-Energy Interactions For Monday: Read Chapter

Radiation Laws Scattering Absorption Radiation Windows Reflectance Terrain-Energy Interactions For Monday: Read Chapter 3. Electromagnetic Radiation II. http://www.crh.noaa.gov/news/display_cmsstory.php?wfo=mqt&storyid=99827&source=0. Stephan Boltzmann Law.

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Remote Sensing Thermal Remote Sensing

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Chapter 27

Chapter 27. Quantum Physics. Conceptual questions: 1,3,9,10 Quick Quizzes: 1,2,3 Problems: 13,42,43,51. Problems which classical physics could not solve. Blackbody Radiation E&M radiation emitted by a heated object Photoelectric Effect Emission of electrons by an illuminated metal

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Structure of Atmosphere

Structure of Atmosphere. From Cunningham & Cunningham, 2004, Fig. 9.1. Wavelength and energy. What are the 3 ways heat can be transferred?. Radiation : transfer by electromagnetic waves. Conduction : transfer by molecular collisions. Convection : transfer by circulation of a fluid.

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Blackbody radiation and solar radiation

Blackbody radiation and solar radiation. More on Blackbody Radiation; Black body radiation 2) Magnitude of Solar radiation. Summary. Radiation power mainly concentrated in an interval of

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Blackbody radiation and solar radiation

Blackbody radiation and solar radiation. More on Blackbody Radiation; Black body radiation 2) Magnitude of Solar radiation. Summary. Radiation power mainly concentrated in an interval of

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The Death Throes of a Star The future of the sun? Very likely!! A star just about identical

The Death Throes of a Star The future of the sun? Very likely!! A star just about identical to our sun is seen after it has thrown off a planetary nebula. It is in the process of collapsing to a white dwarf...all of its hydrogen

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Can the color of a glowing object tell us the temperature of the object?

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Can the color of a glowing object tell us the temperature of the object?

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Need to know and understand

Need to know and understand. Basic physical processes Attenuation of radiation by matter Optical depth Blackbody radiation Wien displacement law l max T = 2.9x10 6 nm.K Stefan-Boltzmann Law L = 4 p R 2 s T 4 Telescopes Basic design Diffraction-limited resolution Q = 1.22l / D

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