Wavelet analysis of the structure of microstreams in the polar solar wind

Details Wavelet analysis of the structure of microstreams in the polar solar wind Wavelet analysis of the structure of microstreams in the polar solar wind

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..385...41n&link_type=abstract

Scientific basis for robotic exploration close to the sun. AIP Conference Proceedings, Volume 385, pp. 41-46 (1997).

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Solar Wind Plasma, Sources Of Solar Wind, Particle Emission, Solar Wind, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays, Mathematical Procedures And Computer Techniques

Scientific paper

The fluctuations in solar-wind velocity measured by the Ulysses spacecraft above the polar regions of the Sun are organized into structures called microstreams. The application of wavelet transformations to the Ulysses data reveals the scales and positions of the microstreams and their association with variations in the helium content of the solar wind. It is concluded that the microstreams must have their origin in solar structures associated with the acceleration of the solar wind with little modification resulting from interplanetary phenomena.

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