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Satellite Beacons Observations from 1964 to 1970, G. K. Hartmann; K. Oberl?nder; G. Schmidt; J. P. S


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Автор: G. K. Hartmann; K. Oberl?nder; G. Schmidt; J. P. S
Название:  Satellite Beacons Observations from 1964 to 1970
ISBN: 9783540058939
Издательство: Springer
Классификация:



ISBN-10: 3540058931
Обложка/Формат: Paperback
Страницы: 98
Вес: 0.25 кг.
Дата издания: 03.07.1972
Серия: Mitteilungen aus dem Max-Planck-Institut f?r Aeronomie
Язык: English
Размер: 279 x 210 x 6
Основная тема: Physics
Ссылка на Издательство: Link
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Поставляется из: Германии
Описание: From October 1964 to May 1969 the 40 MHz, 41 MHz, and 360 MHz signals of the satellite Explo- 0 0 rer 22, were recorded at Lindau (51,650 N; The Faraday effect recordings at 40 MHz and 41 MHz and Dispersive-Doppler-effect recordings at 40 MHz and 360 MHz were used to calculate the ionospheric electron content up to 1000 km.


Trajectories of Artificial Celestial Bodies as Determined from Observations / Trajectoires des Corps Celestes Artificiels D?termin?es D`apr?s les Observations

Автор: J. Kovalevsky
Название: Trajectories of Artificial Celestial Bodies as Determined from Observations / Trajectoires des Corps Celestes Artificiels D?termin?es D`apr?s les Observations
ISBN: 3642493289 ISBN-13(EAN): 9783642493287
Издательство: Springer
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Описание: In May 1962 the International Union of Theoretical and Applied Mechanics (IUTAM) organized a symposium in Paris on the theory of the movement of the Earth's artificial satellites designated to confront the results of the first spatial experiences with the mechanical point of view. The papers submitted during this meeting have been published in 1963 in a collection entitled "Dynamics of Satellites" by Springer- Verlag. During the last three years the importance of studies pertaining to the dynamics of artificial satellites has continued to increase, and many results due to observations have led to a deeper knowledge of the field of forces in which these objects move, particularly the field of gravitation of the Earth, the forces due to pressure of radiation, friction of the atmosphere, etc . . . A new symposium seemed therefore suitable to determine these recent advances. However, this time it appeared appropriate to consider it more from the point of view of the interpretation obtained from the results of observations (determination of orbits and forces existing) than from the point of view of the theory of motion. For this reason the complete title of the second symposium is as follows: "Trajectories of Artificial Celestial Bodies, as Determined from Observations."


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