Development of a high resolution ultraviolet solar spectrograph to be launched on a balloon equatorial platform

Details Development of a high resolution ultraviolet solar spectrograph to be launched on a balloon equatorial platform Development of a high resolution ultraviolet solar spectrograph to be launched on a balloon equatorial platform

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978esasp.135..283l&link_type=abstract

In ESA European Sounding Rocket, Balloon and Related Res., with Emphasis on Expt. at High Latitudes p 283-286 (SEE N79-31637 2

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Balloon-Borne Instruments, Solar Spectrometers, Sun, Ultraviolet Astronomy, High Resolution, Solar Physics, Solar Spectra, Spectrographs, Telescopes

Scientific paper

A telescope-spectrometer instrumentation to study the sun in the spectral ranges 1950-2200 A and 2650-2900 A is being developed to obtain spatial, spectral, and time information on quiet and active fine structures of the solar photosphere-chromosphere zone. To achieve these objectives, an instrumentation able to give 0.5 arcsec angular resolution on the solar surface and 0.01 A spectral resolution was studied.

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