PPT-Blackbody radiation and Light: a wave or a particle

Visit httpscheckinicsuciedu Log in and select Chem 1A When prompted type the word of the day is will be given in class Ensure when asked if you will share your location you select allow . Aim. Calculate local natural convection heat-transfer coefficients for a sphere. Calculate the local boundary layer . Calculate experimental mean Nusselt number. Compare experimental and theoretical Nusselt numbers. Wave-particle duality. (c) So Hirata, Department of Chemistry, University of Illinois at Urbana-Champaign. . This material has . been developed and made available online by work supported jointly by University of Illinois, the National Science Foundation under Grant CHE-1118616 (CAREER), and the Camille & Henry Dreyfus Foundation, Inc. through the Camille Dreyfus Teacher-Scholar program. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the sponsoring agencies. May . 21, . 11.30am -1.30pm, here, cumulative. Chs. : 2, 3, 4, 5, 6, 7, 8, 9, 11, 13, 14, 15, 19, 20, 22, 23, 24, 25, 26, 27, 31. . Review Session . Tue May . 14. Today. :. . “Intro . to Quantum . )=I0e-tn+Bn(1-e-tn)EscapingradiationBn(Tin)Bn(Tout)Valid provided that all the gas is in therm n)=Bn(Tin)1-tn[]+Bn(Tout) Almost all of our information on the heavens is derived from the light we see. We have returned samples from the Moon and a comet . Also obtained meteor samples. We have landed (with unmanned probes) on only a handful of planets and moons. Astronomical magnitude system dates back ~2100 y ago to Hipparchus. Defined their . flux. in . terms of . apparent magnitudes . (m), where the brightest stars were first magnitude (m=1) and the faintest stars visible to the naked eye were sixth magnitude (m=6. Professor M. Sajborg Alam. University at Albany. Sep 28 2010. Adapted from the Internet. Vocabulary terms. polarization . polarizer rest . energy destructive . interference. ultraviolet . time dilation . Neal Boseman, Vessen Hopkins, and Sarah Moorman. Topics of Discussion:. What is Blackbody Radiation?. History of Blackbody Radiation. How has this discovery impacted Modern Physics?. Applications of Blackbody Radiation. Contact information: pemigh@uw.edu. Student Understanding of Blackbody Radiation and Its Application to Everyday Objects. Paul J. . Emigh. Gina . Passante. Peter S. . Shaffer. Previous Research. The . Basics. The . global hydrological cycle. Precipitation. Soil water (lab work). Surface energy . fluxes. Evaporation . and transpiration. Snowpack. Groundwater. Streamflow. Floods . & . Droughts. Water management. M. ulticam. .. Ettienne Cox (. ecox@csir.co.za. ). Ettienne. . Cox. CSIR . - . Where do we fit in. Multicam. background. Multicam. Commercialization. C. urrent . status. Future prospects. . Content. Chapter 9: Electrons in Atoms and the Periodic Table. Learning Goals. Compare the wave and particle natures of light.. Define a quantum of energy, and explain how it is related to an energy change of matter.. To Review. Particle in a Box: A Model. A)Particle in a box according to Newtonian physics. B-D) Quantum mechanical interpretation B) Particle in a box n=1 C) Particle in a box n=2 D) Particle in a box n=3. . Lecture:. . Hans-Jürgen . Wollersheim. e-mail: h.j.wollersheim@gsi.de. Particle Interaction with Matter. Aurora Borealis. Ionization. Particle Interaction with Matter. Cherenkov Light. Characteristic glow from a reactor.