Titlebook: MHD Structures, Waves and Turbulence in the Solar Wind; Observations and The C.-Y. Tu,E. Marsch Book 1995 Springer Science+Business Media D

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C.-Y. Tu,E. Marschziten reichen die Interventionsformen. Schlie?lich sucht die Person selbst ihre Entwicklung zu gestalten und zu optimieren, indem sie handelnd eingreift und so zum ?Produzenten“ ihrer eigenen Entwicklung wird (Featherman & Lerner, 1985; Lerner & Busch-Rossnagel, 1981). Zahlreiche informelle und inst

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Book 1995ly surveyed. Finally, open questions concerning theorigin, nature and evolution of the fluctuations are listed, andperspectives for future research are outlined. .The book is for graduate students and researchers in the field. Othertarget groups are scientists and professionals interested in spaceplasma physics and/or MHD turbulence. .

Synovial-Fluid

MHD Structures, Waves and Turbulence in the Solar WindObservations and The

輕快走過

transdermal

Intermittency of the Solar Wind Fluctuations,Aside of the usual spectral analysis discussed in Section 2, there is an equivalent or even further reaching method for studying fluctuations, which is to investigate directly the differences of any field variable in space and time. For the flow velocity the difference is defined as

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978-90-481-4520-1Springer Science+Business Media Dordrecht 1995