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<p><strong>Abstract.</strong> In this review we collate recent results for the statistical scaling properties of fluctuations in the solar wind with a view to synthesizing two descriptions: that of evolving MHD turbulence and that of a scaling signature of coronal origin that passively propagates with the solar wind. The scenario that emerges is that of coexistent signatures which map onto the well known "two component" picture of solar wind magnetic fluctuations. This highlights the need todoi:10.5194/npg-15-445-2008 fatcat:yo3w2qx7yrfutpzocrb5g7mfiq