A Versatile Multi-Mode Fabry-Perot Instrument
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Published:1976-09
Issue:1
Volume:3
Page:35-38
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ISSN:1323-3580
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Container-title:Publications of the Astronomical Society of Australia
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language:en
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Short-container-title:Publ. Astron. Soc. Aust.
Author:
Dopita Michael A.,Hart John A.
Abstract
Fabry-Perot instruments have been extensively used for many years for the study of spatially extended emission nebulae because they offer a potential luminosity resolution product (L × Rpot) which exceeds by a high factor tha attainable by aerating spectrometer. Meaburn (1970) shows that this product is given by the relation
where P is the number of resolution elements each containing a maximum solid angle, Ω observed simultaneously, ti is the refractive index of the medium between the plates, A is the acceptance area of the device, εo is the transmission coefficient of the associated optics and εF the transmission coefficient of the Fabry-Perot (which if coated with dielectric multilayers can be very high).
Publisher
Cambridge University Press (CUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
1 articles.
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1. A CCD Hα Survey of Nearby Southern Spiral Galaxies;Publications of the Astronomical Society of Australia;1991