Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-25T19:23:59.523Z Has data issue: false hasContentIssue false

A microcomputer controlled CCD H-alpha spectrometer

Published online by Cambridge University Press:  04 August 2017

David A. McDavid*
Affiliation:
Division of Earth and Physical Sciences, University of Texas at San Antonio San Antonio, Texas 78285

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A miniaturized spectrometer designed for mounting at the Cassegrain focus of a 40 cm telescope has been built and laboratory tested with promising results. The optical system consists of a slit, spherical mirror, and reflection grating in a Littrow configuration. The detector is a 128 element linear CCD cooled by an evacuated microminiature nitrogen refrigerator and interfaced to a microcomputer using direct memory access. Laboratory spectra of a mercury vapor discharge tube have been obtained and demonstrate 1 Angstrom resolution with low noise. The spectral coverage of about 100 Angstroms is suitable for measurement of stellar H-alpha line profiles, and it is anticipated that the instrument can be used to monitor bright Be stars.

Type
III. Spectroscopic Research Programmes
Copyright
Copyright © Reidel 1986