Statistical investigation of the height of prominences observed at the Lomnicky Stit coronal station in the period 1967-1986

Astronomy and Astrophysics – Astronomy

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Solar Corona, Solar Prominences, Astronomical Catalogs, Czechoslovakia, Data Processing, Frequency Distribution, Solar Cycles, Time Dependence

Scientific paper

A statistical study of the heights of prominences in the catalogue of solar prominences of Rusin et al. (1988) is presented. The catalogue contains 16,620 prominences between 1967 and 1986. The analysis is conducted using the method proposed by Dermendjiev (1977). It is found that the height law distribution is dependent on the phase of the solar activity cycle. Also, it is shown that the height of polar prominences during a cycle changes more than the height of prominences in the main zone.

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