Solar physics assessment of future high-resolution observations in the grazing-incidence domain

Details Solar physics assessment of future high-resolution observations in the grazing-incidence domain Solar physics assessment of future high-resolution observations in the grazing-incidence domain

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ssrv...29..301m&link_type=abstract

(Schweizerische Naturforschende Gesellschaft and Eidgenosische Technische Hochschule Zurich, Conference on Solar Physics from Sp

Astronomy and Astrophysics

Astronomy

3

Grazing Incidence, Grist (Telescope), High Resolution, Solar Instruments, Ultraviolet Astronomy, Atmospheric Heating, Electron Density (Concentration), Extreme Ultraviolet Radiation, Metals, Plasma Diagnostics, Solar Corona

Scientific paper

The project for a Grazing Incidence Solar Telescope (GRIST) offers, for the first time, the combinations of high spatial (1-arcmin) and spectral resolution in the extreme-ultraviolet wavelength range. The three-dimensional electron density and temperature structure of the transition region and corona will be determined. The dynamics of the structures which make up the corona will be studied. GRIST can be expected to provide definitive improvement in the understanding of the coronal heating problem.

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