The solar fine structure telescope.

Details The solar fine structure telescope. The solar fine structure telescope.

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990acasn..31..174s&link_type=abstract

Acta Astron. Sin., Vol. 31, No. 2, p. 174 - 180

Astronomy and Astrophysics

Astronomy

Solar Telescopes, Solar Chromosphere: Images, Solar Photosphere: Images

Scientific paper

The solar fine structure telescope is used to make simultaneous high spatial resolution observations in the same region of the solar chromosphere and photosphere. The clear aperture of the objectives is 260 mm. The central wavelength of the working wavelength range of the birefringent filter is 6562.8 Å and it is tuneable over the range 6562.8 ű1.5 Å. The diameters of the solar image used for the chromospheric photographic observations are 85 mm and 130 mm. The wavelength and the solar image diameter of photospheric photographic observations are 5500 Å and 300 mm respectively.

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