Abstract
A description of the SOlar Radio Spectrometer (SORS) experiment as part of the KORONAS-I project is given. The goal of this experiment is to study the solar radio emission and plasma wave phenomena in the Earth ionosphere in a wide frequency range of from 100 kHz to 300 MHz. The results of the SORS observations for a three-month working period are discussed, and the proposals for improvement of the SORS equipment for future KORONAS missions are presented.
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