3-D Heliosphere at Solar Maximum Proceedings of the 34th Eslab Symposium, 3-6 October 2000, Estec, Noordwijk, the Netherlands

The global structure of the heliosphere changes dramatically with the solar circle. Our knowledge of the heliosphere in three dimensions under solar-minimum conditions has advanced significantly in the last 10 years, largely as a result of the on-going ESA/NASA Ulysses mission. Similar advances in our understanding of the heliosphere at solar maximum are to be expected with the return of Ulysses to the Sun's polar regions in 2000/2001. The papers in this volume address a wide range of topics related to the solar-maximum heliosphere, and include many of the latest findings from Ulysses and other space-based missions. Ground-based studies and theoretical modeling are also well represented. Specific questions include: what are the dominant processes that determine the global structure of the inner heliosphere under conditions of high solar activity, and what are the key differences between the high-latitude heliosphere at solar maximum and solar minimum? The book is intended for those carrying out active research in the fields of solar and heliospheric physics.Marsden, R. G. is the author of '3-D Heliosphere at Solar Maximum Proceedings of the 34th Eslab Symposium, 3-6 October 2000, Estec, Noordwijk, the Netherlands' with ISBN 9780792370475 and ISBN 0792370473.