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By Richard Marsden

Our wisdom of the heliosphere in 3 dimensions close to sunlight minimal has complex considerably within the final 10 years, principally as a result on-going ESAINASA Ulysses challenge. related advances in our realizing of the worldwide heliosphere close to sun greatest are to be anticipated with the go back of Ulysses to excessive sun latitudes in 2000/200 I. With this in brain, the thirty fourth ESLAB Symposium, held at ESTEC in Noordwijk, The Netherlands, on 3-6 October, 2000, was once dedicated to 'The 3-D Heliosphere at sunlight Maximum'. This used to be the 3rd ESLAB Sympo­ sium concentrating on the third-dimensional heliosphere (previous symposia being in 1985 and 1994), and the timing was once fairly applicable, marking because it did the tenth anniversary of the release of the Ulysses spacecraft. moreover, Ulysses had simply begun its 3rd high-latitude go, the second one over the Sun's south polar areas. The symposium addressed a variety of themes with regards to the solar-maximum heliosphere, with displays on a number of the most modern findings from Ulysses and different space-based missions. Ground-based stories and theoretical modeling have been additionally good represented. particular inquiries to which solutions have been sought incorporated the following.

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The 3-D Heliosphere at Solar Maximum - Proceedings of the 34th ESLAB Symposium by Richard Marsden

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