Physics
Scientific paper
Jul 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..140....1m&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 140, no. 1, July 1992, p. 1-6.
Physics
6
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.
Minarovjech Milan
Rybansky Milan
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