Titlebook: Advances in Magnetospheric Physics with GEOS-1 and ISEE; K. Knott,A. Durney,K. Ogilvie Book 1979 D. Reidel Publishing Company, Dordrecht,

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Gon?alo Avelar,José Sim?o,Luís Veiga per charge range from thermal to 16 keV/.. From measurements made in the keV range during eleven magnetic storms we find that the percentage of heavy (. > 1) ions present in the outer magnetosphere increases by a factor of 3 to 10 during disturbances. We conclude that two independent sources (solar

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Maximize

Fumin Liu,Yuezhong Wu,Falong Xiao,Qiang Liu T., are derived from the plasma frequency and Debye length, the values of which determine the shape of the frequency dependent mutual impedance curves. The existing limits of the method are pointed out. They may be instrumental or arise from a lack of theoretical development, for instance when the

Recess

Hao Ge,Qianmu Li,Shunmei Meng,Jun Houticular, the plasma frequency, which gives the electron density..We have now measurements over the whole dayside of the magnetosphere, from the evening to the night sectors..The behaviour of the plasma resonance depends on local time, the nightime echoes being generally weaker..Density measurements

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Guilherme Galante,Rodrigo da Rosa Righibe the motion of energetic particles and the evolution of fluxes along a given orbit. In the second one, the exact internal and external fields are used for field line tracing and the determination of conjugate points. Applications to the calculation of synchronous fluxes and the Geos conjugate points are given.