Abstract

We describe one of the possible designs for the UV–visible spectrograph optics to be employed in the ODIN project. The spectrograph will be used in a future satellite mission for aeronomy observations and will image a column of atmosphere just above the Earth’s surface onto a two-dimensional CCD array with the spatial and spectral content aligned orthogonal to one another.

© 1995 Optical Society of America

GEMINI spectrograph optics

Ian Powell
Appl. Opt. 32(16) 2949-2956 (1993)

Far-ultraviolet spectrographs: the impact of holographic grating design

Webster Cash
Appl. Opt. 34(13) 2241-2246 (1995)

Ultraviolet and visible imaging and spectrographic imaging instrument

J. F. Carbary, E. H. Darlington, T. J. Harris, P. J. McEvaddy, M. J. Mayr, K. Peacock, and C. I. Meng
Appl. Opt. 33(19) 4201-4213 (1994)

Tomographic extreme-ultraviolet spectrographs: TESS

Daniel M. Cotton, Andrew Stephan, Timothy Cook, James Vickers, Valerie Taylor, and Supriya Chakrabarti
Appl. Opt. 39(22) 3991-3999 (2000)

The Diffuse Interstellar Cloud Experiment: a high-resolution far-ultraviolet spectrograph

Eric Schindhelm, Matthew Beasley, Eric B. Burgh, and James C. Green
Appl. Opt. 51(7) 812-822 (2012)