Non-Gaussian probability distributions of solar wind fluctuations
The probability distributions of field differences ∆<i>x</i>(τ)=<i>x</i>(<i>t</i>+τ)-<i>x</i>(<i>t</i>), where the variable <i>x</i>(<i>t</i>) may denote any solar wind scalar field or vector field component at time <i>t</i&