Paper
29 June 1992 The Coronal Ultraviolet Berkeley Spectrometer (CUBS)
Author Affiliations +
Abstract
We describe an instrument package to remotely measure thermospheric, exospheric, and plasmaspheric structure and composition. This instrument was flown aboard the second test flight of the Black Brant XII sounding rocket on December 5, 1989, which attained an apogee of 1460 km. The experiment package consisted of a spectrophotometer to measure He I 584 A, O II 834 A, O I 989 A, hydrogen Lyman beta (1025 A), hydrogen Lyman alpha (1216 A), and O I 1304 A transitions, and a photometer to measure the He II 304 A emission. The optical design of the spectrophotometer was identical to that of the Berkeley Extreme Ultraviolet (EUV) Airglow Rocket Spectrometer payload, flown on September 30, 1988 aboard the maiden flight of the Black Brant XII rocket. We present the initial data analysis and describe directions we will go toward the completion of our study.
© (1992) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Brett C. Bush, Daniel M. Cotton, and Supriya Chakrabarti "The Coronal Ultraviolet Berkeley Spectrometer (CUBS)", Proc. SPIE 1745, Instrumentation for Planetary and Terrestrial Atmospheric Remote Sensing, (29 June 1992); https://doi.org/10.1117/12.60619
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Sensors

Spectrophotometry

Hydrogen

Scattering

Rockets

Mirrors

Spectroscopy

RELATED CONTENT

The Photoelectric Spectroheliometer On ATM
Proceedings of SPIE (September 01 1974)
The Herschel-SPIRE instrument
Proceedings of SPIE (October 12 2004)
Radiometric calibration of PHEBUS: model and results
Proceedings of SPIE (September 17 2012)
Calibration Of The Berkeley EUV Airglow Rocket Spectrometer
Proceedings of SPIE (November 27 1989)

Back to Top