Characteristics of the Taylor microscale in the solar wind/foreshock: magnetic field and electron velocity measurements
The Taylor microscale is one of the fundamental turbulence scales. Not easily estimated in the interplanetary medium employing single spacecraft data, it has generally been studied through two point correlations. In this paper we present an alternative, albeit mathematically equivalent, method f...
| Main Authors: | , , , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Copernicus Publications
2013-11-01
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| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/31/2063/2013/angeo-31-2063-2013.pdf |