Spectral polarization analysis of the interplanetary magnetic field fluctuations

Details Spectral polarization analysis of the interplanetary magnetic field fluctuations Spectral polarization analysis of the interplanetary magnetic field fluctuations

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..149..381p&link_type=abstract

Solar Physics, vol. 149, no. 2, p. 381-389

Physics

4

Circular Polarization, Fourier Analysis, Interplanetary Magnetic Fields, Magnetohydrodynamic Waves, Power Spectra, Solar Wind, Spectral Energy Distribution, Spectrum Analysis, Fast Fourier Transformations, Giacobini-Zinner Comet, Heos B Satellite, Lebesgue Theorem, Nyquist Frequencies, Pioneer 10 Space Probe, Pioneer 11 Space Probe, Plasma Turbulence

Scientific paper

A new computational method and algorithm, based on complex Fourier analysis, is used to derive the spectral density of plane and circularly polarized fluctuation components of the interplanetary magnetic field. Applications of the method have been made using HEOS 2 (1 AU), Pioneer 10 (5 AU), Pioneer 11 (20 AU), and International Cometary Explorer (ICE) (Giocabini-Zinner's comet) data sets. The results show the existence of circularly polarized magnetohydrodynamic (MHD) waves in all cases.

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