Vasily Oreshko

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Simultaneous multifrequency observations of the Crab pulsar giant pulses (GPs) were performed with the 64-m Kalyazin radio telescope at four frequencies 0.6, 1.4, 2.2 and 8.3 GHz using the K5 VLBI recording terminal. K5 terminal provided continuous recording in 16 4-MHz wide frequency channels distributed over 4 frequency bands. Several thousands of GPs(More)
We present a review of observed parameters of giant radio pulses, based on the observations conducted by our group during recent years. The observations cover a broad frequency range of about 3 octaves, concentrating between 600 and 4850 MHz. Giant pulses of both the Crab pulsar and the millisecond pulsar B1937+21 were studied with the 70-m Tidbinbilla, the(More)
В. А. Самодуров1,2, А.С. Позаненко3, А.Е. Родин1, Д.Д. Чураков4, Д.В. Думский1,2, Е.А. Исаев1,2, А.Н. Казанцев1, С.В. Логвиненко1, В.В. Орешко1, М.О. Торопов5, М.И. Волобуева6 1Пущинская Радиоастрономическая обсерватория АКЦ ФИАН, Пущино 2Национальный исследовательский университет «Высшая школа экономики», Москва 3Институт космических исследований РАН,(More)
Simultaneous multifrequency observations of the Crab pulsar giant pulses (GPs) were performed with the 64-m Kalyazin radio telescope at four frequencies ν = 0.6, 1.4, 2.2 and 8.3 GHz, using the K5 VLBI recording terminal. The K5 terminal provided continuous recording in 16 4-MHz wide frequency channels distributed over 4 frequency bands. Several thousand(More)
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