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From the Outer Heliosphere to the Local Bubble - Comparisons of New Observations with Theory (Paperback, 2009 ed.)
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From the Outer Heliosphere to the Local Bubble - Comparisons of New Observations with Theory (Paperback, 2009 ed.)
Series: Space Sciences Series of ISSI, 31
Expected to ship within 10 - 15 working days
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Knowledge about the outer heliosphere and the interstellar medium,
which were long treated as two separate fields, has improved
dramatically over the past 25 years as a consequence of recent
developments: The discovery of interstellar pickup ions and neutral
helium inside the heliosphere, the determination of the
interstellar hydrogen distribution in the heliosphere obtained
using backscattered solar Lyman-alpha radiation, the prediction and
subsequent detection of the hydrogen wall just outside of the
heliopause, the development of detailed global models for the
interaction of solar wind plasma with the interstellar medium, and
most recently, direct in-situ plasma and field measurements inside
of the heliosheath. At the same time, our understanding of the
nearby galactic environment, including the composition and dynamics
of the warm gas clouds and hot gas in the local bubble, has
benefited greatly from absorption-line spectroscopy using nearby
stars as background sources and dynamic modeling. The present
volume provides a synopsis of these developments organised into
seven sections: Dominant physical processes in the termination
shock and heliosheath, three-dimensional shape and structure of the
dynamic heliosphere, relation of the plasmas and dust inside and
outside of the heliosphere, origin and properties of the very local
interstellar medium, energy and pressure equilibria in the local
bubble, physical processes in the multiphase interstellar medium
inside of the local bubble, and the roles that magnetic fields play
in the outer heliosphere and the local bubble. The last theme is
probably the most basic of all as magnetic fields play important
roles in most of the phenomena discussed here. The volume concludes
with four papers providing the "big picture" by looking at the time
evolution of both the heliosphere and the local bubble, looking
beyond the local bubble, and finally addressing the challenges in
modeling the interface between the two media.
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