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Titlebook: Maligne gastrointestinale Tumoren; Peter M. Schlag (Direktor),Christian Dittrich (Vor Conference proceedings 1995 Springer-Verlag/Wien 199

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P. Ferenciects possess magnetic fields, which may differ significantly in magnitude and other characteristics. Measurements of the strengths, directions, distributions and variations of so many magnetic fields have become one of the main tasks of contemporary astrophysical observations. After several decades
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ects possess magnetic fields, which may differ significantly in magnitude and other characteristics. Measurements of the strengths, directions, distributions and variations of so many magnetic fields have become one of the main tasks of contemporary astrophysical observations. After several decades
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G. H. Mostbeckzes the nature of magnets such as the Earth and the Sun is entirely different from the nature of a horseshoe magnet. The source of cosmic magnetism is associated with the hydrodynamic motions of a highly conductive medium. In this aspect, cosmic magnets resemble a dynamo. However, currents in the dy
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M. Kontrus,M. Wiesmayr,Ch. Heroldzes the nature of magnets such as the Earth and the Sun is entirely different from the nature of a horseshoe magnet. The source of cosmic magnetism is associated with the hydrodynamic motions of a highly conductive medium. In this aspect, cosmic magnets resemble a dynamo. However, currents in the dy
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Th. Rand the author at Argonne National Laboratory (ANL) in September of 1973. Large parts of the book evolved from lectures given to graduate students at the University of TUbingen during the past three years. It is the purpose of this book to provide an introduction to the many features of magnetic flux s
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G. Heinz-Peerssical or low-temperature superconductors. It went out of print not long after the discovery of high-temperature superconductors in 1986 by J.G. Bednorz and K.A. Miiller, a discovery which resulted worldwide in an explosive growth of research and development in the field of superconductivity. Becaus
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f the angular momentum operator. The energylevels for a variety of spins are generated, and the modeling of the magnetization, the magneticsusceptibility, and the heat capacity is done. Theoretical formulae necessary for performing theenergy level calculations for a multiterm system are prepared wit
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