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Anisotropy and Alfvenicity of hourly fluctuations in the fast polar solar wind

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dc.contributor.author Neugebauer, M. en_US
dc.date.accessioned 2004-09-16T23:50:12Z
dc.date.available 2004-09-16T23:50:12Z
dc.date.issued 2004-02 en_US
dc.identifier.citation Journal of geophysical research v.109, A02101, doi:10.1029/2003JA009947, 2004 en_US
dc.identifier.citation Tucson, AZ, USA en_US
dc.identifier.clearanceno 03-2003 en_US
dc.identifier.uri http://hdl.handle.net/2014/7803
dc.description.abstract Ulysses magnetic and plasma data obtained in the fast polar solar wind are used to study the nature of fluctuations in the frequency range between the turbulent inertial range and the lower-frequency range dominated by quasi-static structures originating at the Sun. For daily variations of hourly averages of the magnetic field components the anisotropy of the fluctuations is less than in the higher-frequency range, and the minimum varianced direction loses its alignment with the magnetic field in favor of a more radial direction as the solar distance increases. en_US
dc.format.extent 5239040 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Solar wind Alfvenicity waves anisotropy Ulysses en_US
dc.title Anisotropy and Alfvenicity of hourly fluctuations in the fast polar solar wind en_US


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