Contents

Cosmic Research

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Vol. 57, No. 6, 2019

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Physical Mechanism of a Solar Flare Based on the Accumulation of the Energy in the Magnetic Field of the Current Sheet in the Solar Corona

I. M. Podgorny and A. I. Podgorny p. 389  abstract

Solar Corona as Indicator of Differential Rotation of Subphotospheric Layers

V. N. Obridko and O. G. Badalyan p. 407  abstract

Comparing the Features of Generation of CMEs Moving with Different Speed in the Field of View of the LASCO Coronagraphs

Yu. S. Zagainova and V. G. Fainshtein p. 413  abstract

Disturbed Flows in the Inner Solar Wind and Near Earth’s Orbit

A. I. Efimov, L. A. Lukanina, V. M. Smirnov, I. V. Chashei, M. K. Bird and M. Pätzold p. 423  abstract

Small-Scale Plasma Fluctuations in Fast and Slow Solar Wind Streams

M. O. Riazantseva, L. S. Rakhmanova, G. N. Zastenker, Yu. I. Yermolaev, I. G. Lodkina and L. S. Chesalin p. 434  abstract

Turbulent Cascade in the Magnetosheath Affected by the Solar Wind’s Plasma Turbulence

L. S. Rakhmanova, M. O. Riazantseva, G. N. Zastenker, Yu. I. Yermolaev, I. G. Lodkina and L. S. Chesalin p. 443  abstract

Properties of the Ionosphere during an Extreme Storm

M. G. Deminov and G. F. Deminova p. 451  abstract

Periodic Orbits of N Bodies on a Sphere

J. J. Smulsky p. 459  abstract

Brief Communications

Estimation of the Size of an Electric Current with High Helium Abundance inside a Magnetic Cloud

Yu. I. Yermolaev p. 471  abstract

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