A high resolution ultraviolet solar telescope-spectrograph mounted on an equatorial balloon platform

Details A high resolution ultraviolet solar telescope-spectrograph mounted on an equatorial balloon platform A high resolution ultraviolet solar telescope-spectrograph mounted on an equatorial balloon platform

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983esasp.183..401s&link_type=abstract

In ESA Sixth ESA Symp. on European Rocket and Balloon Programs and Related Res. p 401-407 (SEE N83-33397 21-46)

Physics

Balloon-Borne Instruments, Fine Structure, Solar Atmosphere, Solar Spectrometers, Spectrographs, Ultraviolet Telescopes, Angular Resolution, High Altitude Balloons, Near Ultraviolet Radiation, Pointing Control Systems, Solar Spectra, Spectral Resolution

Scientific paper

A balloon-borne 30 cm telescope-spectrograph combination was built to
observe fine structures of the solar atmosphere with very high spectral
and angular resolution in two atmospheric windows: 2700 to 2950 A and
1900 to 2300 A. Solar spectra with spectral resolution of 15 mA and
angular resolution of 4 arcsec were recorded.

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