CHM260 - Spectroscopy Method
The Maier-Leibnitz-Laboratory for Nuclear and Particle Physics of LMU Munich and TU Munich Nuclear Structure Studies at the MLL Tandem accelerator Prof.
D O N OW (3/7/14): 1. What is a photon? 2. What are some characteristics of photons? 3. Does light interact with matter as a particle or a wave? Justify.
Photosynthesis
Photosynthesis Pres
De Broglie wavelengths Contents: de Broglie wavelengths Example 1 Whiteboards Transmission electron microscopes Scanning electron microscopes Scanning.
Niels Bohr and the quantum atom Contents: Problems in nucleus land Spectral lines and Rydberg’s formula Photon wavelengths from transition energies Electron.
Stellar Temperatures Wien’s law works perfectly for objects with Planck spectra. Stars don’t quite have Planck-like spectra. UV Blue Green Red Infrared.
Astro 201: Sept. 14, 2010 Read: Hester, Chapter 4 Chaos and Fractal information on class web page On-Line quiz #3: available after class, due next Tuesday.
Lecture 16: Electromanetic Radiation Reading: Zumdahl 12.1, 12.2 Outline –The nature of electromagnetic radiation. –Light as energy. –The workfunction.
Schottky Enabled Photoemission & Dark Current Measurements John Power, Eric Wisniewski, Wei Gai Argonne Wakefield Accelerator Group Argonne National Laboratory.
Indian Astronomy Satellite Mission (ASTROSAT) National Institutions 1.ISRO, Bangalore 2.TIFR, Mumbai 3.IIA, Bangalore 4.RRI, Bangalore 5.PRL, Ahmedabad.
