Observations of Alfvénic turbulence evolution in the 3-D heliosphere

Details Observations of Alfvénic turbulence evolution in the 3-D heliosphere Observations of Alfvénic turbulence evolution in the 3-D heliosphere

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..377b&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 377-3

Physics

Plasma Physics

4

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

The heliospheric plasma is an excellent laboratory to study the behaviour of collisionless Alfvénic turbulence. This is a fundamental topic in both plasma physics and astrophysics. The impressive amount of observations at different solar distances and latitudes collected in last three decades allows to get a good view of the turbulence behaviour in the heliosphere inside 5 AU. In present review the focus will be on the evolution of the Alfvénic turbulence in both low- and high-latitude solar wind, as derived from old observations on the ecliptic and from recent observations by Ulysses at polar latitudes.

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