Turbulence properties along the Solar Probe trajectory

Details Turbulence properties along the Solar Probe trajectory Turbulence properties along the Solar Probe trajectory

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..385...67m&link_type=abstract

Scientific basis for robotic exploration close to the sun. AIP Conference Proceedings, Volume 385, pp. 67-76 (1997).

Computer Science

Solar Instruments

Scientific paper

Measurements of turbulence properties, including the degree of spectral anisotropy, are essential to the scientific objectives of the Solar Probe mission. Several types of measurements are discussed including component variances, reduced spectra, and helicities. The measurability of spectra with a single spacecraft depend upon some form of ``frozen-in'' approximation that allows conversion of frequency to wavenumber. Accuracy of several such approximations is examined along the proposed spacecraft trajectory.

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