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High Resolution Solar Spectra from 1780 to 1950 Å

Published online by Cambridge University Press:  12 April 2016

Howard C. McAllister  and
Richard J. Wolff
Howard C. McAllister
Affiliation:
Dept. of Physics and Astronomy and Institute for Astronomy, University of Hawaii, Hawaii, U.S.A.
Richard J. Wolff
Affiliation:
Dept. of Physics and Astronomy and Institute for Astronomy, University of Hawaii, Hawaii, U.S.A.

Extract

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Excellent spectrograms in the region from 1780 to 1950 ängströms were obtained from the flight of a high resolution spectrograph in an Aerobee 150 rocket at White Sands Missile Range on June 14, 1971. The instrument’s dispersing system, consisting of a 79 line mm-1 echelle crossed with a 1200 line mm-1 grating, was incorporated in a Czerny-Turner arrangement using spherical mirrors of one meter focal length. Spectral resolution was limited to 13 mÅ by a slit width of 25 μ. The plate factor was 0.5 Å mm-1. Spectra were recorded on Kodak type 101-01 film.

Type
Section III / Stellar and Solar UV Radiation
Information
International Astronomical Union Colloquium , Volume 14: Special Issue: Ultraviolet and X-Ray Spectroscopy of Astrophysical and Laboratory Plasmas , November 1972 , pp. 610 - 611
Copyright
Copyright © Reidel 1972