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2 edition of High-precision velocity and magnetic measurements of bright stars with a magneto-optical filter found in the catalog.

High-precision velocity and magnetic measurements of bright stars with a magneto-optical filter

William James Chaplin

High-precision velocity and magnetic measurements of bright stars with a magneto-optical filter

by William James Chaplin

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  • 15 Currently reading

Published by University of Birmingham in Birmingham .
Written in English


Edition Notes

Thesis (Ph.D) - University of Birmingham, School of Physics and Space Research, 1994.

Statementby William James Chaplin.
ID Numbers
Open LibraryOL21124036M

DATE: Octo TIME: PM in PSE SPEAKER: Prof. Cody Storry, Department of Physics and Astronomy, York University. ABSTRACT: The goal of our ATRAP collaboration is to make, trap and laser cool antihydrogen atoms for a precise comparison between the atomic spectra of antimatter and matter and a sensitive test of CPT invariance.I will discuss results from our first . “Ultra-High-Precision Velocity Measurements of Oscillations in α Centauri A”, Astrophysical Journal, , L75 – L78 Google Scholar Buzasi D. ().

The dashed lines are defined by equations E=~v(kx ± lB −2 ro), where v is the velocity of electrons at the charge neutrality point of 2D graphene, lB is the magnetic length and kx is the. Methods: Analysis of laser-induced fluorescence (LIF): spectral measurements, relative intensity distributions in the spectra, measurements of LIF kinetic after pulsed excitation, polarisation studies, changes of LIF polarisation and circularity in external magnetic field (Hanle effect), and electric field (Stark-Hanle effect), 1(state mixing.

The simulation illustrates how model parameters affect the galactic rotation (or circular velocity) curve, and also how the rotation curve affects directly observable quantities such as the radial velocities of stars. This connection to observable quantities allows the user to determine the set of parameter values that best fits the data. g-2 of the Muon and Electron: anomalous anomalies: Prof Thomas Teubner: University of Liverpool: , Friday 10 January Physics Seminar Room (Building 46/) The anomalous magnetic moment of the muon, g-2, has been measured and calculated with very high is one of few observables which persistently show a deviation between experiment and Standard Model prediction.


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High-precision velocity and magnetic measurements of bright stars with a magneto-optical filter by William James Chaplin Download PDF EPUB FB2

This work is comprised of the study of two magneto-optical phenomena: the Kerr effect and the Faraday effect. Neutron physics experiments often utilize polarized neutrons, and one method to generate or guide polarized neutrons involves the use of a system of magnetic super-mirrors.

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et al.ApJS,L; arXivv1. HMI velocity, intensity, and magnetic-field measurements are used in numerous investigations, so understanding the quality of the data is important. This article describes the calibration measurements used to track the performance of the HMI instrument, and it details trends in important instrument parameters during the prime mission.

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