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MAIK Nauka/Interperiodica

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Possible role of electrostatic potential in formation of sharp boundaries of small-scale and middle-scale solar wind structures

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Large and sharp changes of solar wind dynamic pressure and disturbances of the magnetospheric magnetic field at geosynchronous orbit caused by these variations

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Density pulses in the solar wind

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Theory of type III radio bursts in the interplanetary space. II. Study of instability of the electron beam-solar wind plasma system in a linear approximation

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