Coronal line photometer

Physics

Scientific paper

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Astronomical Photometry, Emission Spectra, Line Spectra, Solar Corona, Solar Spectrometers, Spectral Line Width, Television Cameras, Temporal Resolution

Scientific paper

A photoelectric photometer to determine intensities of the spectral
lines of the solar corona is described. The measurements cover the range
400-900 nm with a time resolution up to 0.04 s. Starting from 1 January,
1991, the photometer is used for patrol observations of the green and
the red coronal lines at coronal station.

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