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      Mirror mode structures in the solar wind at 0.72 AU : BRIEF REPORT

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          Magnetic field investigation of the Venus plasma environment: Expected new results from Venus Express

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            Ulysses field and plasma observations of magnetic holes in the solar wind and their relation to mirror-mode structures

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              Characteristic size and shape of the mirror mode structures in the solar wind at 0.72 AU

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                Author and article information

                Journal
                Journal of Geophysical Research: Space Physics
                J. Geophys. Res.
                American Geophysical Union (AGU)
                01480227
                October 2009
                October 2009
                October 21 2009
                : 114
                : A10
                : n/a
                Affiliations
                [1 ]Space Research Institute; Austrian Academy of Sciences; Graz Austria
                [2 ]State Key Laboratory of Space Weather; Chinese Academy of Sciences; Beijing China
                [3 ]Institute of Geophysics and Planetary Physics; University of California; Los Angeles California USA
                [4 ]School of Astronautics; Beihang University; Beijing China
                [5 ]Department of Automatic Control and Systems Engineering; University of Sheffield; Sheffield UK
                [6 ]Institute of Geophysics; Universidad Nacional Autonoma de Mexico, Ciudad Universitaria; Mexico City Mexico
                Article
                10.1029/2009JA014103
                176c5c6e-e38a-491a-9156-26258bab5c88
                © 2009

                http://doi.wiley.com/10.1002/tdm_license_1.1

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