NIRwave: A wave-turbulence-driven solar wind model constrained by PSP observations

We generate a model description of the solar wind based on an explicit wave-turbulence-driven heating mechanism, and constrain our with observational data. included coronal source term in general 3D magnetohydrodynamic code NIRVANA to simulate properties wind. The adapted mechanism is interaction subsequent dissipation counter-propagating Alfv\'en waves corona, accounting for turbulent rate Q_p. magnetic field assumed be axisymmetric dipole strength 1 G. Our results are validated against data taken by Parker Solar Probe (PSP). NIRwave reconstructs bimodal structure slow fast speeds 410 km/s 650 respectively. global mass-loss 2.6e-14 masses per year. Despite implementing simplified conditions represent field, parameters characterising steady-state solution reasonable agreement previously established empirical constraints. number density from good derived constraints, larger deviations radial velocity temperature. In comparison polytropic generated NIRVANA, we find that better constraints derive.