Il Nuovo Cimento C
Year 2019 - Issue 1 - January-February
SoHe3 2018
The rotation angle distribution underlying magnetic field fluctuations in the 1/f range of solar wind turbulent spectra
Authors: L. Matteini, D. Stansby, T. S. Horbury, C. H. K. Chen
DOI: 10.1393/ncc/i2019-19016-y
Published online 31 May 2019
Article: 16
Open Access
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