Description: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.We have made it easy for you to find a PDF Ebooks without any digging. And by having access to our ebooks online or by storing it on your computer, you have convenient answers with The 3-D Heliosphere at Solar Maximum: Proceedings of the 34th ESLAB Symposium, 3–6 October 2000, ESTEC, Noordwijk, The Netherlands. To get started finding The 3-D Heliosphere at Solar Maximum: Proceedings of the 34th ESLAB Symposium, 3–6 October 2000, ESTEC, Noordwijk, The Netherlands, you are right to find our website which has a comprehensive collection of manuals listed. Our library is the biggest of these that have literally hundreds of thousands of different products represented.
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The 3-D Heliosphere at Solar Maximum: Proceedings of the 34th ESLAB Symposium, 3–6 October 2000, ESTEC, Noordwijk, The Netherlands
Description: 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.We have made it easy for you to find a PDF Ebooks without any digging. And by having access to our ebooks online or by storing it on your computer, you have convenient answers with The 3-D Heliosphere at Solar Maximum: Proceedings of the 34th ESLAB Symposium, 3–6 October 2000, ESTEC, Noordwijk, The Netherlands. To get started finding The 3-D Heliosphere at Solar Maximum: Proceedings of the 34th ESLAB Symposium, 3–6 October 2000, ESTEC, Noordwijk, The Netherlands, you are right to find our website which has a comprehensive collection of manuals listed. Our library is the biggest of these that have literally hundreds of thousands of different products represented.