How to Define the Mean Square Amplitude of Solar Wind Fluctuations With Respect to the Local Mean Magnetic Field
نویسندگان
چکیده
منابع مشابه
Dependence of Solar Wind Power Spectra on the Direction of the Local Mean Magnetic Field
Wavelet analysis can be used to measure the power spectrum of solar wind fluctuations along a line in any direction (θ, φ) with respect to the local mean magnetic field B0. This technique is applied to study solar wind turbulence in high-speed streams in the ecliptic plane near solar minimum using magnetic field measurements with a cadence of eight vectors per second. The analysis of nine high-...
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ژورنال
عنوان ژورنال: Journal of Geophysical Research: Space Physics
سال: 2017
ISSN: 2169-9380
DOI: 10.1002/2017ja023864