'Zeeman splitting' presentation slideshows

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??? ? ???????. Trions at low electron density limit 1 . Charged exciton-electron complexes ( trions ) 2 . Singlet and triplet trion states 3. Modulation doped QWs 4 . Trions in optical spectra 5. Action of magnetic fields on the trions

603 views • 51 slides

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??? ? ???????. Trions at low electron density limit 1 . Charged exciton-electron complexes ( trions ) 2 . Singlet and triplet trion states 3. Modulation doped QWs 4 . Trions in optical spectra 5. Action of magnetic fields on the trions

632 views • 51 slides

Talking About S pectrum

Talking About S pectrum. Hou Saiyu 04/01/2014 Note: Four digital numbers referring to wavelength in unit of angstrom here. outline. Introduction Properties Important spectrum in astronomy AGN spectrum. outline. Introduction Properties Important spectrum in astronomy

564 views • 42 slides

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Ultrahigh-resolution Laser Spectroscopy and The Zeeman Effect of Naphthalene S 1 ? S 0 Transition. c ( z ). Kazuto Yoshida , Shunji Kasahara Kobe University, Japan Masaaki Baba Kyoto University, Japan. b ( y ). a ( x ). Introduction. PAHs (Polycyclic Aromatic Hydrocarbons).

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ATOMIC SPECTROMETRY Flames Electrothermal Atomizers Plasmas

489 views • 28 slides

Observational Characterization of Magnetized Turbulence in Molecular Clouds

Observational Characterization of Magnetized Turbulence in Molecular Clouds. Martin Houde The University of Western Ontario. IAU, Beijing - 21 Aug. 2012. Outline. Main Observational Methods and Techniques Polarization Measurements Zeeman Dust mapping *

320 views • 22 slides

Quantum Dots and Spin Based Quantum Computing

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Zeeman effect of the hyperfine structure levels in H- and Li-like lead

Zeeman effect of the hyperfine structure levels in H- and Li-like lead. D. L. Moskovkin 1 , V. M. Shabaev 1 , and W. Quint 2 1 Department of Physics, St. Petersburg State University, Oulianovskaya 1, Petrodvorets, St. Petersburg 198504, Russia

374 views • 14 slides

Can masers trace the Galactic magnetic field?

Can masers trace the Galactic magnetic field?. The MAGMO Survey. CSIRO ASTRONOMY AND SPACE SCIENCE. Jimi Green | A Neapolitan of Maser Science 2013 | Sydney. 21 st May 2013. Overview Can hydroxyl (OH) masers map the Galactic magnetic field ?. Introduction

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The Incredible 6.7 GHz Methanol Masers: A key to understanding high-mass star formation.

Image credit: Robert Hurt (NASA/JPL, IPAC/SSC). MAGMO. The Incredible 6.7 GHz Methanol Masers: A key to understanding high-mass star formation. Jimi Green CSIRO Astronomy & Space Science, ATNF Great Barriers in Massive Star Formation 16 th September 2010, Townsville. THE MAGMO TEAM.

264 views • 14 slides

Methanol maser polarization in W3(OH)

Methanol maser polarization in W3(OH). Lisa Harvey-Smith Collaborators: Vlemmings, Cohen, Soria-Ruiz Joint Institute for VLBI in Europe. Overview. Formation of massive stars Support against cloud collapse -Turbulence -Magnetic support Maser polarization theory -Zeeman splitting

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Zeeman effect HFS and isotope shift

Zeeman effect HFS and isotope shift. Anomalous Zeeman Effect. More than three closely spaced optical lines were observed. The interaction that splits the energy levels in an external magnetic field is caused by interaction. The magnetic moment depends on

370 views • 12 slides