Abstract
The results of a reduction of the dataset obtained with the RATAN-600 within the framework of the “Cosmological Gene” project are reported. The project was performed in order to estimate the contribution of atmospheric noise in observations of Galactic background radiation. Atmospheric noise prevails on time scales exceeded 10–100 seconds. The efficiency of preselecting the data with low atmospheric noise on the time scales of interest is demonstrated. The potential of the “Cosmological Gene” project for different accumulation times in the sky area studied are assessed with the effect of real atmospheric noise taken into account.
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Original Russian Text © T.A. Semenova, Yu.N. Pariiskij, P.G. Tsybulev, 2009, published in Astrofizicheskij Byulleten, 2009, Vol. 64, No. 2, pp. 196–203.
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Semenova, T.A., Parijskij, Y.N. & Tsybulev, P.G. The requirements toward the methods of “Clearing” the atmosphere in ground-based radio-astronomical observations of background emissions of the atmosphere. Astrophys. Bull. 64, 191–197 (2009). https://doi.org/10.1134/S1990341309020084
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DOI: https://doi.org/10.1134/S1990341309020084