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Titel Variable low-frequency radio emission of the solar system and galactic objects
VerfasserIn Alexander Konovalenko, Vladimir Kolyadin, Helmut Rucker, Vyacheslav Zakharenko, Philippe Zarka, Jean-M. Griessmeier, Loran Denis, Valentin Melnik, Galina Litvinenko, Valerij Zaitsev, Igor Falkovich, Oleg Ulyanov, Mikhail Sidorchuk, Sergej Stepkin, Alexander Stanislavskij, Nikolaj Kalinichenko, Nastja Boiko, Iaroslavna Vasiljiva, Dmytro Mukha, Artem Koval
Konferenz EGU General Assembly 2013
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 15 (2013)
Datensatznummer 250076886
 
Zusammenfassung
There are many physical processes and propagation effects for the producing the time variable radio emission just at the low frequencies (at the decameter wavelength). The study of this radio emission is the important part of the modern radio astronomy. Strong progress in the development of the radio telescopes, methods and instrumentation allowed to start the corresponding investigations at new quality and quantity levels. It related to the implementation of the world largest UTR-2 radio telescope (effective area is more than 100 000 sq.m) more high sensitive at frequencies less than 30 MHz. During last years many new observations were carried out with this radio telescope and many new effects have been detected for the Sun, planets, interplanetary medium, exoplanets as well as various kinds of the stars.