Study of Space Plasma with Multifractality and Intermittency Scaling during Solar Cycle 23

This study deals with the multifractality and intermittency scaling of plasma parameters (Proton Density and Proton Temperature) for January 1996 to December 2006 which is nearly the time span of Solar Cycle 23. The datasets of these parameters have been taken from OMNI Web server and the level of multifractality and intermittency is analyzed for solar wind plasma parameters. Our results show the inconsistent rate of the transfer of the energy flux which are clear indications of multifractal and intermittence behavior of solar wind plasma parameter turbulence in the inner heliosphere and describes the energy transfer is responsible for turbulence in various environments and their features having similar behavior like nonlinear multifractal systems. This result also shows that the degree of asymmetry for these scaled parameters have much better agreement with the real data for solar cycle 23 and data sampling shows weakly correlation with the phase of the solar activity.