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Titlebook: Magnetospheric Physics; Achievements and Pro Bengt Hultqvist,C.-G. Fälthammar Book 1990 Springer Science+Business Media New York 1990 earth

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Active Experiments in Magnetospheric Physics,ing given to active experiments for the purpose of clarifying specific phenomena in the magnetospheric plasma. The earliest global scale experiments were the production of artificial radiation belts by high altitude nuclear bomb bursts in 1958–62 and the observation of their geophysical effects. Oth
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,The Encounter of Voyager 2 with Neptune’s Magnetosphere, the Neptune system on August 24 through 28, 1989. These included measurements of the magnetic field, plasma (10 ev ≤ E ≤ 6 keV), energetic and high energy particles (22 keV ≤ E ≤ 5 MeV), plasma waves (10 Hz to 50 kHz) and radio emissions (~ 20 to ~1300 kHz); additional information relating to UV em
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The Need for High Time Resolution Measurements in the Magnetosphere,aries and energy conversion processes are controlled by non-linear micro-physic s that occur on time scales as fast as 1 to 100 microseconds. The understanding of these phenomena requires measurements of plasma distributions and time domain electric fields with appropriately high time resolutions. S
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Why do We Need Ground Based, Balloon and Sounding Rocket Measurements in the Future?,o longer a use for data obtained through traditional remote sensing techniques from the ground or from balloon borne probes. In this paper it will be shown that data from arrays of ground based remote sensors play an instrumental role in defining the global characteristics of magnetospheric and iono
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Large-Scale Organization of Solar System Plasmas,o­sphere. The latter is itself likely to be a large plasma cell embedded within the local interstellar medium. The heliosphere and magnetosphere plasma cells delineate spatial regions where matter is organized by electromagnetic forces, as opposed to gravitational forces. The recognition of the univ
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