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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

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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

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Full field measurements of hidden objects around corners or through scatterers reaching sub-mm resolution will be presented. The single-shot 3D movie camera is a highly precise 3D sensor for the measurement of fast macroscopic live scenes.


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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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KEYWORDS: Near infrared, Telescopes, Stars, Imaging systems, Cameras, Sensors, Adaptive optics, Coronagraphy, Optical benches, Planets Read Abstract + Exo-Planets search and characterization has been the science case driving the SHARK-NIR design, which is one of the two coronagraphic instruments proposed for the Large Binocular Telescope.

Various fundamental-physics experiments such as measurement of the magnetic birefringence of the vacuum, searches for ultralight dark-matter particles (e.g., axions), and precision spectroscopy of complex systems (including exotic atoms containing antimatter constituents) are enabled by Cited by: 4.

S.K. Solanki et al.: The Polarimetric and Helioseismic Imager on Solar Orbiter To gain a better knowledge and understanding of magneto-convection, it is important to know the full velocity and magnetic field vector with as few assumptions as possible.

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