THE RT-32 RADIO TELESCOPE CONSTRUCTION BASED ON THE MARK-4B ANTENNA SYSTEM. 3. LOCAL OSCILLATORS AND SELF-NOISE OF THE RECEIVING SYSTEM

Purpose: High resolution investigation of spectral lines of space sources requires low intrinsic noise of the radio telescope receiving system. It is provided with both input cryogenic amplifiers and low phase noise of local oscillators. To make spectral studies, it is neces ary to be able to tune t...

Full description

Bibliographic Details
Main Authors: O. M. Ulyanov, V. V. Zakharenko, E. A. Alekseev, O. M. Reznichenko, I. O. Kulahin, V. V. Budnikov, V. I. Prisiazhnii, A. V. Poikhalo, V. V. Voytyuk, V. N. Mamarev, V. V. Ozhinskyi, V. P. Vlasenko, V. M. Chmil, I. K. Sunduchkov, M. M. Berdar, V. I. Lebed, M. I. Palamar, A. V. Chaikovskii, Yu. V. Pasternak, M. A. Strembitskii, M. P. Natarov, S. O. Steshenko, V. V. Glamazdin, O. I. Shubnyi, A. O. Kyrylenko, D. Yu. Kulyk
Format: Article
Language:English
Published: National Academy of Sciences of Ukraine, Institute of Radio Astronomy 2020-09-01
Series:Radio Physics and Radio Astronomy
Subjects:
Online Access:http://rpra-journal.org.ua/index.php/ra/article/view/1335/pdf#