Slide 1 Slide 2 Tony Hey Director of UK e-Science Core Program [email protected] The UK e-Science Program and the Grid Slide 3 e-Science and the Grid e-Science is about…

Slide 1THE SUN AND ITS RELATION TO OTHER STARS 1 Slide 2 Stellar astronomy Well discuss properties of solar-type and other stars – lets first review some preliminaries:…

Slide 11 ColourColour David Molyneaux Slide 2 2 Light is electromagnetic energy Light is a wave Colour is the way the eye perceives light at different wavelengths inside…

Slide 1Magnetic Fields in T Tauri Disks A. Meredith Hughes Wesleyan University What Millimeter Polarimetry Can Tell Us Chat Hull, David Wilner, Sean Andrews, Jungyeon Cho,…

Slide 1Fluorescence – a key to unravel (atomic) structure and dynamics Slide 2 What is a fluorescence? Wiki: emission of light by a substance that has absorbed light or…

Slide 1 Slide 2 UV Detectors Fixed Wavelength Variable Wavelength Diode array Slide 3 High Pressure Mercury Lamp Fixed Wavelength Mercury vapor lamps are probably the most…

Slide 1Norton group meeting 11/2010, David Neff Comparison of excitation output Hg vs HgXe vs Xe lamp at objective of TE200 with Optisplit: justification for 2 optics necessary…

Slide 1Chapter 3 Photophysics Slide 2 Emission and loss processes: Several of pathways for loss of electronic excitation shown in Fig. as a emission of light as luminescence…

Slide 1Spectral Lines Celestial Fingerprinting Visit www.worldofteaching.comwww.worldofteaching.com For 100’s of free powerpoints Slide 2 Goals From light we learn about…

Slide 1Noadswood Science, 2011 Slide 2 EM & Communications  To understand how EM waves are used in communications Monday, August 25, 2014 Slide 3 Anagrams Solve the…