Solar Wind Nine: Proceedings of the Ninth International Solar Wind Conference: Nantucket, Massachusetts, 5-9 October 1998
Shadia Rifai Habbal, Ruth Esser, Joseph V. Hollweg, Philip A. Isenberg
American Inst. of Physics, Jun 24, 1999 - Science - 895 pages
The Solar Wind Nine Conference was the ninth in the series of solar wind conferences established in 1964 by Dr. Marcia Neugebauer to provide a forum for the interaction between solar physicists and space physicists interested in the origin and evolution of the solar wind. One of the scientific goals of the conference was to reflect the importance of the synergistic interaction between theory, numerical modeling and simulations, in situ measurements and remote sensing observations, in the exploration of the solar wind. Indeed, the opportunity provided by the many concurrent missions Ulysses, Yohkoh, SOHO, TRACE, SPARTAN, WIND, and ACE, which probe the Sun and interplanetary space from different vantage points, provided very rich material for the contributions. The presentations included invited reviews and contributed talks as well as poster presentations. This conference took place almost 40 years after Parkers prediction of the existence of the solar wind.
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Coronal Plasma Characteristics and Solar Wind Theory
The Dynamic Solar Chromosphere and the Ionization of Hydrogen
Solar Wind Measured by Interplanetary Scintillation Method
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1999 The American acceleration Alfven waves American Institute amplitude anisotropy associated Astrophys average boundary chromosphere component coronagraph coronal hole coronal mass ejections correlation cosmic ray current sheet distance distribution dynamic edited by S. R. emission energy equation Esser fast solar wind field lines Figure flare flow fluctuations flux rope flux tubes frequency Geophys heliocentric heliosphere heliospheric current sheet Institute of Physics interaction interplanetary J. V. Hollweg km/s lar wind LASCO latitude Lett magnetic clouds magnetic field measurements netic observed P. A. Isenberg panel parameters particle photospheric plasma polar coronal hole profiles propagation proton quiet Sun radial ratio region rotation S. R. Habbal scale shock shown shows simulations slow solar wind solar corona solar minimum Solar Wind Nine solar wind speed Space spacecraft spectra spectrum stream streamer belt structure temperature termination shock thermal tion turbulence Ulysses values variations velocity wavenumber