Paper
15 June 2015 Near ultraviolet spectrograph for balloon platform
A. G. Sreejith, Margarita Safonova, Jayant Murthy
Author Affiliations +
Proceedings Volume 9654, International Conference on Optics and Photonics 2015; 96540D (2015) https://doi.org/10.1117/12.2181749
Event: International Conference on Optics and Photonics 2015, 2015, Kolkata, India
Abstract
Small and compact scientific payloads may be easily designed constructed and own on high altitude balloons. Despite the fact that large orbital observatories provide accurate observations and statistical studies of remote and/or faint space sources, small telescopes on board balloons or rockets are still attractive because of their low cost and rapid response time. We describe here a near ultraviolet (NUV) spectrograph designed to be own on a high{altitude balloon platform. Our basic optical design is a modified Czerny-Turner system using off the shelf optics. We compare different methods of aberration corrections in such a system. We intend the system to be portable and scalable to different telescopes. The use of reflecting optics reduces the transmission loss in UV. We plan on using an image intensified CMOS sensor operating in photon counting mode as the detector of choice.
© (2015) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
A. G. Sreejith, Margarita Safonova, and Jayant Murthy "Near ultraviolet spectrograph for balloon platform", Proc. SPIE 9654, International Conference on Optics and Photonics 2015, 96540D (15 June 2015); https://doi.org/10.1117/12.2181749
Lens.org Logo
CITATIONS
Cited by 4 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Mirrors

Spectrographs

Monochromatic aberrations

Near ultraviolet

CMOS sensors

Spherical lenses

Aberration correction

Back to Top