Abstract
Ultraviolet astronomy is an important tool for the study of the interplanetary medium and diffuse, angularly extended emissions in planetary/comet atmospheres and their near space environments. We describe a new technique for high étendue observations of emission lines at R > 105 within all-reflective spatial heterodyne spectrometer and polarmetric sampling of these lines with an ultraviolet optimized waveplate-Brewster mirror combination. The resulting system is thermo-mechanically stable, has light collecting power substantially greater than HST for extended emissions, despite having a volume of several × 10-3 m3. This makes the SHS polarimeter ideal for spacecraft applications. We describe the SHS and polarmetric optical techniques and provide a discussion of its planned development for studies of interplanetary hydrogen.
Original language | English (US) |
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Pages (from-to) | 676-685 |
Number of pages | 10 |
Journal | Proceedings of SPIE - The International Society for Optical Engineering |
Volume | 4854 |
DOIs | |
State | Published - 2002 |
Event | Future EUV/UV and Visible Space Astrophysics Missions and Instrumentation - Waikoloa, HI, United States Duration: Aug 22 2002 → Aug 23 2002 |
Keywords
- Interferometry
- Polarimetry
- Spectroscopy
- Ultraviolet
ASJC Scopus subject areas
- Electronic, Optical and Magnetic Materials
- Condensed Matter Physics
- Computer Science Applications
- Applied Mathematics
- Electrical and Electronic Engineering