Titlebook: Interball in the ISTP Program; Studies of the Solar D. G. Sibeck,K. Kudela Book 1999 Springer Science+Business Media Dordrecht 1999 Solar w

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J. Šafránková,Z. Němeček,M. Borák, along with other agents and interventions. There are several effective psychotherapeutic treatments, which lead to observable changes in the brain. Antidepressants and psychotherapy may have distinct neural effects. Their combination seems to have some advantages..Apathy partially overlaps with de

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Closely-Spaced Multi-Satellite Project Roy to Study Small-Scale Structures during Magnetic Field Ane strong plasma turbulence, and magnetic “reconnection” occur in the critical magnetospheric domains. At the dayside these are mainly outer cusps and subsolar magnetopause, but recent findings from the INTERBALL Project show that flanks of the magnetosphere can also be sites of these active plasma p

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Heliospheric Energetic Particle Flux Variations,e, and in galactic sources. Suprathermal and energetic particles usually play a minor role in the mass, momentum and energy density carried by the solar wind at 1 AU, although they are likely to have more important dynamical effects at very small and very large heliospheric radii. The intensity dist

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,On the Earth’s Bow Shock Near Solar Minimum,interplanetary medium streaming from the Sun. This boundary is important because it is here that the streaming solar wind is slowed, heated, and partially deflected around the Earth’s magnetosphere. The bow shock has been extensively mapped and modeled ever since it was first discovered a number of

Commodious

Interball and Geotail Observations of Flux Transfer Events,he dayside and flank magnetopause. At 1530 universal time (UT) on January 29, 1996, Geotail was located just inside the prenoon magnetopause, where it observed a series of transient events marked by bipolar flow signatures normal to the nominal magnetopause. There were no significant magnetic field

Pelvic-Floor

Relative Timing on Magnetospheric Substorm Onset Signatures, and the relative timing of onset between different substorm signatures at various locations in space is essential to the understanding of the physical mechanisms of substorm onset. In this paper we will emphasize the importance of this issue by demonstrating inconsistency among several widely used