Efimov A.I., Lukanina L.A., Smirnov V.M., Chashei I.V., Bird M.K., Paetzold M. Detection of Strongly Turbulent Regions in the Supercorona with the Venus Express and Mars Express Satellites. Geomagnetism and Aeronomy , 2021 , 61 (3). С. 293-298. ISSN 0016-7932
Полный текст не доступен из этого репозитория.Аннотация
Experiments involving the radio sounding of solar plasma with signals from the Venus Express and Mars Express spacecraft, which were carried out from October 6 to December 6, 2006, provided data on frequency fluctuations of the radio signals for the western and eastern coronal limbs. The processing of this data provided information on the intensity of the frequency fluctuations, a parameter of plasma turbulence. High peaks of the intensity of frequency fluctuation were noted against the background of radial dependence; they can be explained by the passage of the compressed part of a corotating disturbance through a radio ray path. A delay in these events indicates a high-level connection of the fluctuations in the sounding radio-signal frequency within the same coronal region.
| Тип объекта: | Статья |
|---|---|
| Авторы на русском. ОБЯЗАТЕЛЬНО ДЛЯ АНГЛОЯЗЫЧНЫХ ПУБЛИКАЦИЙ!: | Ефимов А.И., Луканина Л.А. Смирнов В.М., Чашей И.В., Берд М.К., Петцольд М. |
| Подразделения (можно выбрать несколько, удерживая Ctrl): | 114 лаб. исследований космической плазмы радиофизическими методами 119 лаб. распространения радиоволн и дистанционного зондирования атмосферы |
| URI: | http://cplire.ru:8080/id/eprint/9608 |
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