Applications of spatial heterodyne spectroscopy for remote sensing of diffuse UV-vis emission line sources in the solar system

Walter Harris; Fred Roesler; Lotfi Ben-Jaffel; Edwin Mierkiewicz; Jason Corliss; Ronald Oliversen; Tobias Neef

doi:10.1016/j.elspec.2005.01.223

Applications of spatial heterodyne spectroscopy for remote sensing of diffuse UV-vis emission line sources in the solar system

Walter Harris, Fred Roesler, Lotfi Ben-Jaffel, Edwin Mierkiewicz, Jason Corliss, Ronald Oliversen, Tobias Neef

Research output: Contribution to journal › Article › peer-review

22 Scopus citations

Abstract

Spatial heterodyne spectrographs combine high spectral resolution with large étendue in a compact instrument. This combination makes them useful for studies of extended diffuse sources requiring velocity resolution or the separation of closely packed emission lines, while their small size makes them suitable for platforms ranging from ground-based observatories to satellites. Improvements in optical element and detector capabilities have expanded opportunities for SHS in the VUV, where its combination of size, resolution, and étendue have not been available. Here we discuss the basics of the SHS technique and how an instrument may be designed to study various emission line sources in the solar system.

Original language	English (US)
Pages (from-to)	973-977
Number of pages	5
Journal	Journal of Electron Spectroscopy and Related Phenomena
Volume	144-147
DOIs	https://doi.org/10.1016/j.elspec.2005.01.223
State	Published - Jun 2005
Externally published	Yes

Keywords

Interferometery
Spectroscopy

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Radiation
Atomic and Molecular Physics, and Optics
Condensed Matter Physics
Spectroscopy
Physical and Theoretical Chemistry

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10.1016/j.elspec.2005.01.223

Cite this

Applications of spatial heterodyne spectroscopy for remote sensing of diffuse UV-vis emission line sources in the solar system. / Harris, Walter; Roesler, Fred; Ben-Jaffel, Lotfi; Mierkiewicz, Edwin; Corliss, Jason; Oliversen, Ronald; Neef, Tobias.

In: Journal of Electron Spectroscopy and Related Phenomena, Vol. 144-147, 06.2005, p. 973-977.

Research output: Contribution to journal › Article › peer-review

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abstract = "Spatial heterodyne spectrographs combine high spectral resolution with large {\'e}tendue in a compact instrument. This combination makes them useful for studies of extended diffuse sources requiring velocity resolution or the separation of closely packed emission lines, while their small size makes them suitable for platforms ranging from ground-based observatories to satellites. Improvements in optical element and detector capabilities have expanded opportunities for SHS in the VUV, where its combination of size, resolution, and {\'e}tendue have not been available. Here we discuss the basics of the SHS technique and how an instrument may be designed to study various emission line sources in the solar system.",

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AU - Harris, Walter

AU - Roesler, Fred

AU - Ben-Jaffel, Lotfi

AU - Mierkiewicz, Edwin

AU - Corliss, Jason

AU - Oliversen, Ronald

AU - Neef, Tobias

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AB - Spatial heterodyne spectrographs combine high spectral resolution with large étendue in a compact instrument. This combination makes them useful for studies of extended diffuse sources requiring velocity resolution or the separation of closely packed emission lines, while their small size makes them suitable for platforms ranging from ground-based observatories to satellites. Improvements in optical element and detector capabilities have expanded opportunities for SHS in the VUV, where its combination of size, resolution, and étendue have not been available. Here we discuss the basics of the SHS technique and how an instrument may be designed to study various emission line sources in the solar system.

KW - Interferometery

KW - Spectroscopy

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Applications of spatial heterodyne spectroscopy for remote sensing of diffuse UV-vis emission line sources in the solar system

Abstract

Keywords

ASJC Scopus subject areas

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