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 | |
| State | Published - Jun 2005 |
| Externally published | Yes |
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Keywords
- Interferometery
- Spectroscopy
ASJC Scopus subject areas
- Physical and Theoretical Chemistry
- Spectroscopy
- Atomic and Molecular Physics, and Optics
- Surfaces and Interfaces
Cite this
Applications of spatial heterodyne spectroscopy for remote sensing of diffuse UV-vis emission line sources in the solar system. / Harris, Walter M; 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
}
TY - JOUR
T1 - Applications of spatial heterodyne spectroscopy for remote sensing of diffuse UV-vis emission line sources in the solar system
AU - Harris, Walter M
AU - Roesler, Fred
AU - Ben-Jaffel, Lotfi
AU - Mierkiewicz, Edwin
AU - Corliss, Jason
AU - Oliversen, Ronald
AU - Neef, Tobias
PY - 2005/6
Y1 - 2005/6
N2 - 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.
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
UR - http://www.scopus.com/inward/record.url?scp=17444367724&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=17444367724&partnerID=8YFLogxK
U2 - 10.1016/j.elspec.2005.01.223
DO - 10.1016/j.elspec.2005.01.223
M3 - Article
AN - SCOPUS:17444367724
VL - 144-147
SP - 973
EP - 977
JO - Journal of Electron Spectroscopy and Related Phenomena
JF - Journal of Electron Spectroscopy and Related Phenomena
SN - 0368-2048
ER -