PPT-Energy Dispersive spectroscopy

EDS analysis High Resolution Microscopy and Advanced Imaging Center FLORIDA TECH Tatiana Karpova MD PhD What is energy dispersive spectroscopy Energy Dispersive Spectroscopy EDS also known as energy dispersive Xray spectroscopy EDX and sometimes called Xray energy dispersive spectroscopy XEDS is a qualitative and quantitative Xray . Seda Yerli 20824388. Serap . Sunatepe. 20824245. Gonca Çalışkan 20823894 . Beytepe. ,Ankara. 12.04.2012. OUTLINE. History. of IR . Radiation. . and. FTIR. General . Information. . about. IR . 1.2-m UK Schmidt Telescope. Author: . Primož Cigler. Mentor: . prof. dr. Tomaž Zwitter. Seminar Leader: . prof. dr. Peter Križan. What I will be talking today about?. Basics about spectroscopy and some theoretical background. Professor. Dr. HANS SCHUESSLER . By. . Ansam Jameel Talib. Molecular Physics Course. . . . History of Raman Scattering. 1923. . – Inelastic light . scattering . predicted by A. . meeting #8. Filter systems. Johnson system . SDSS system (Gunn filters). IR filters. Narrow-band filters. More…. >215 systems …. Spectrographs. Dispersive elements: prism. High throughput; low resolution; wavelength-dependant . Frequency combs – evolutionary tree. Overview. Basic Features: Frequency . C. ombs. Applications:. Frequency Metrology. Measuring Frequency Gaps. Frequency Combs as Optical Synthesizers. Time Domain Applicatons . 12. th. International User Meeting on Cavity Enhanced Spectroscopy, 13 June, 2017. 1A12. Charles R. Markus. , Jefferson E. McCollum, Thomas S. Dieter, Philip A. . Kocheril. , and Benjamin J. McCall. 2. UV Spectroscopy. Introduction. UV radiation and Electronic Excitations. The difference in energy between molecular bonding, non-bonding and anti-bonding orbitals ranges from 125-650 kJ/mole. This energy corresponds to EM radiation in the ultraviolet (UV) region, 100-350 nm, and visible (VIS) regions 350-700 nm of the spectrum. Alex Flanagan (University of Wisconsin). J. F. Drake (UMD), M. Swisdak (UMD). Magnetic Reconnection?. Magnetic energy converted to kinetic . and thermal energy. Occurs in solar corona, magnetosphere, laboratory plasma experiments, and even at edge of solar system. 1 IR-Spectroscopy IR region The part of electromagnetic radiation between the visible and microwave regions 0.8  m to 50  m ( 12,500 cm -1 - 200 cm -1 ) is called IR region Most interested region in Infrared Spectroscopy is between 2.5 Chapter 5. Sub Topics. Introduction to Atomic Spectroscopy. Atomic . Absorption Spectroscopy AAS. Atomic . Emission . Spectroscopy. AES. Interferences and Comparisons. Atomic Absorption and Emission Spectroscopy. 2. Nuclear Magnetic Resonance Spectroscopy. After hydrogen, the most useful atom providing information is carbon-13.. The . overall intensity of a . 13. C signal is about 6400 . times . less than the intensity of an . MSSL, March 17-18, 2009. Frits Paerels. Columbia Astrophysics Laboratory. Columbia University, New York. cgs. units throughout!. Hα. Hβ. Hγ. Hδ. Wavelength (Å). NB: 1 Å = 10. -8. cm. E = . hc/λ. Transmissions Electron Microscopy (TEM). Part I:. The microscope. Sample preparation. Imaging. Part II:. Diffraction. Defects. Part III. Spectroscopy. . Repetision. :. Electron . Diffraction. :. Powder. Marie-Laure Mauborgne. SLB. CSG17 – July 17. th. 2023. 1. Founded by a physicist and an engineer in 1926 to conduct the first geophysical measurements of rock formations . What is SLB?. (former Schlumberger).