In the paper is described the construction of the radio telescope for the wavelengths of 56 and 130 cm which has been used on the observatory of the Astronomical Institute of the ČSAV at Ondřejov for radio observations of the sun. Prevailing part of the work is devoted to the receiving equipment for the wavelength of 56 crn, which whole was built in own laboratories and which has been for 3 years in everyday operation. The author explains the determination of the fundamental parameters of the equipment and describes the means necessary to reach them. The design proposal and the realization of the receiver for the wavelength of 56 cm together with a high-stability d. c. amplifier and the design and realization of the calibrating arrangements including diode noisegenerator are described. Further the author considers to the details the influence of different quantities on the measurement accuracy and on the estimation of the resulting power flux density in the antenna apertuře with this instrument. Finally, a servomechanism performing automatic transformation of equatorial to azimuthal coordinates is described. In the next part the 130 cm - equipment is briefly mentioned. This equipment was of substantial part built outside the Institute. The both receiving apparatus use a common mirror of 7‘5m diameter having in its focus two primary feeds with
polarizations perpendicular to each other.
This Paper is a continuation of four proceeding lists, which contained flares observed at Ondřejov since 1948 up to the end of June, 1957. This list presents data abour 727 flares, associated 536 Mc/s outburst, and atmospheries observed and recorded during the I. G. Y. Curves of the H2 line-width changes for all these flares are plotted in Fig. 1-15.
Spectral observations of solar radio bursts at 2.0 - 4.5 GHz taken at the Astronomical Observatory Ondřejov between January and December 1990 are presented. Also given are a tables and computer outputs in equidensities and in time intensity profiles of the bursts.
Spectral Observations of solar radio bursts at 2.0 - 4.5 GHz taken
at the Astronomical Observatory Ondřejov between January and August
1991 are presented. Also given are a tables and computer outputs in
equidensities and in time intensity profiles of the bursts. and - Abstract (s. 1) - zde před článkem
- Observed data (s. 9-139)