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Published in

Cambridge University Press, Proceedings of the International Astronomical Union, T28A(7), p. 95-124, 2011

DOI: 10.1017/s1743921312002694

Cambridge University Press, Proceedings of the International Astronomical Union, T27A(4), p. 124-144, 2008

DOI: 10.1017/s1743921308025374

Cambridge University Press, Proceedings of the International Astronomical Union, T26A(1), p. 103-120, 2005

DOI: 10.1017/s1743921306004406

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Commission 49: Interplanetary Plasma and Heliosphere

This paper is available in a repository.
This paper is available in a repository.

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Data provided by SHERPA/RoMEO

Abstract

AbstractCommission 49 covers research on the solar wind, shocks and particle acceleration, both transient and steady-state, e.g., corotating, structures within the heliosphere, and the termination shock and boundary of the heliosphere. During the last three years there was considerable progress made in studies of solar energetic particles, compositional and other signatures in the heliosphere, solar wind pickup ions, the termination shock, which was finally crossed by a spacecraft, and the boundary between the heliosphere and interstellar medium, and in solar wind modeling and space weather. These topics have been summarized here in five articles, each with extensive references that will guide the reader who wants further details. Observations from the following spacecraft have extensively used during this period: Ulysses, Cassini, Voyager 1 and 2, MESSENGER, ACE, Genesis, SOHO, Wind, and RHESSI.