Chaotic transverse modes wave activity far upstream of the ion foreshock during intervals of an interplanetary magnetic field near parallel to the solar wind velocity.

Details Chaotic transverse modes wave activity far upstream of the ion foreshock during intervals of an interplanetary magnetic field near parallel to the solar wind velocity. Chaotic transverse modes wave activity far upstream of the ion foreshock during intervals of an interplanetary magnetic field near parallel to the solar wind velocity.

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agufmsh72a0547f&link_type=abstract

American Geophysical Union, Fall Meeting 2002, abstract #SH72A-0547

Physics

2114 Energetic Particles, Heliospheric (7514), 2149 Mhd Waves And Turbulence, 2784 Solar Wind/Magnetosphere Interactions, 2794 Instruments And Techniques

Scientific paper

Several events have been identified of an ion foreshock extending up to 250 RE upstream of the Earth. These events occur mostly during periods of slowly drifting radial interplanetary magnetic field (IMF) when the 1-min average values of the strengths of the IMF and the solar wind (SW) speeds are mostly steady (Berdichevsky et al., 1999T). Here we present an overview of our current investigation on the nature of the observed transverse modes of oscillation and a preliminary interpretation of their association to the observed diffuse ion population. These observations use high resolution Wind WAVES, MFI, 3DP, and SWE data. TBerdichevsky, D., G. Thejappa, R. Fitzenreiter, R. Lepping, T. Yamamoto, S. Kokubun, R. McEntire, D. Williams, and R.P. Lin, Widely spaced wave-particle observations during GEOTAIL and WIND magnetic conjunctions in the Earth's ion foreshock, J. Geophys. Res., 104, 463-482, 1999

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