Basic properties of solar wind MHD turbulence near 0.3 AU analyzed by means of Elsaesser variables

Details Basic properties of solar wind MHD turbulence near 0.3 AU analyzed by means of Elsaesser variables Basic properties of solar wind MHD turbulence near 0.3 AU analyzed by means of Elsaesser variables

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jgr....9411739t&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 94, Sept. 1, 1989, p. 11739-11759.

Physics

94

Interplanetary Magnetic Fields, Magnetohydrodynamic Turbulence, Magnetohydrodynamic Waves, Solar Wind, Cross Correlation, Helios Satellites, Magnetic Field Configurations, Power Spectra, Wave Propagation

Scientific paper

Magnetic field and plasma data from Helios 1 and 2 are used to study the
solar wind MHD turbulence near 0.3 AU. The power spectra corresponding
to Elsaesser variables are calculated to identify the wave modes that
elucidate the physical picture of the turbulence. The possible
mechanisms responsible for the observed spectra are discussed.

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