High Resolution Telescope and Spectrograph (HRTS)

Details High Resolution Telescope and Spectrograph (HRTS) High Resolution Telescope and Spectrograph (HRTS)

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986stos.work....6m&link_type=abstract

In its Solar Terrestrial Observatory Space Station Workshop Report p 6 (SEE N86-19349 10-19)

Physics

Solar Flares, Solar Observatories, Space Stations, Spectroheliographs, Sun, Sunspots, Telescopes, Ultraviolet Spectrometers, Display Devices, Energy Distribution, Mass Distribution, Pointing Control Systems, Spacelab Payloads

Scientific paper

The major objectives of the high resolution telescope and spectrograph (HRTS) are: (1) the investigation of the energy balance and mass balance of the temperature minimum, chromosphere, transition zone, and corona in quiet regions on the Sun as well as in plages, flares, and sunspots; (2) the investigation of the velocity field of the lower corona to study the origin of the solar wind; and (3) the investigation of preflare and flare phenomena. The HRTS instruments consists of a telescope, an ultraviolet spectrograph, an ultraviolet spectroheliograph, and an H alpha slit display system, all housed in a thermal control cannister mounted on an instrument pointing system.

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