Intermittency in Solar Wind Turbulence From Fluid to Kinetic Scales
Solar wind is a highly turbulent medium exhibiting fluctuations ranging from the solar sidereal rotation period to proton and electron gyroperiods. Their amplitudes show remarkable scalings with frequency across more than seven decades, suggesting a self‐similar nature for these fluctuations. Howeve...
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| Format: | Article |
| Language: | English |
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American Geophysical Union (AGU)
2019-05-01
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| Series: | Earth and Space Science |
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| Online Access: | https://doi.org/10.1029/2018EA000535 |