Объекты, где автором является "Kopnina T.F."

Kolomiets S.F., Gavrik A.L., Lukanina L.A., Kopnina T.F. AN EXPERIMENT AND DATA PROCESSING TECHNIQUE AIMED AT DETERMINING THE RADIAL SPEED OF SOLAR WIND INHOMOGENEITIES OF VARIOUS SPATIAL SCALES. In: THE TENTH MOSCOW SOLAR SYSTEM SYMPOSIUM 2019, 7-11 октября 2019 г., Москва, ИКИ РАН , IKI RAS (ИКИ РАН, Москва) , С. 469-470.

Gavrik A.L., Kolomiets S.F., Bondarenko M.I., Lukanina L.A., Kopnina T.F., Ilyushin Ya.A. Radio occultation on the VENERA-D mission: A concept of radio frequency subsystem and radio science technique. RADIOELECTRONICS. NANOSYSTEMS. INFORMATION TECHNOLOGIES. , 2019 , 11 (1). С. 5-12. ISSN 2218-3000

Gavrik A.L., Bondarenko M.I., Kolomiets S.F., Kopnina T.F., Lukanina L.A. Venera-D Mission: A Concept of Radio Frequency Subsystem and Radio Science Technique. In: 2019 Russian Open Conference on Radio Wave Propagation (RWP), 01-06 July 2019, Kazan, Russia , IEEE , С. 163-166.

Kolomiets S.F., Gavrik A.L., Gavrik Y.A., Kopnina T.F., Ilyushin Ya.A. A new criterion of the geometrical optics applicability as a foundation of a novel approach to radio occultation data interpretation. In: The Ninth Moscow Solar System Symposium (9M-S3), 8-12 October 2018, Moscow. Russia. Space Research Institute

Gavrik A.L., Kolomiets S.F., Bondarenko M.I., Ilyushin Ya.A., Kopnina T.F., Gavrik Yu.A. Radio-occultation measurements of plasma layers in Venusian ionosphere. In: Венера-Д. Конференция по моделированию атмосферы (GCM), внутреннего строения, поверхности, окружающей плазмы Венеры., 5-7 October 2017, Институт Космических Исследований, Москва , ИКИ РАН

Gavrik A.L., Kopnina T.F., Bondarenko M.I., Smislov A.A. Multi-frequency phase-coherent systems: new instrument for occultation in the project Venus-D. In: The Sixth Moscow Solar System Symposium (6MS3), October 5-9, 2015, Space Research Institute, Moscow, Russia , 243-ab.

Gavrik A.L., Kopnina T.F., Kuleshov E.A., Smislov A.A. Stratified multi-layer structures of the Venus ionosphere from Venera 15 and 16 radio occultation measurements. In: The Fourth Moscow Solar System Symposium, 14-18 October, IKI RAN, Moscow