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2023 |
NIRwave: A wave-turbulence-driven solar wind model constrained by PSP observations \ Aims: We generate a model description of the solar wind based on an explicit wave-turbulence-driven heating mechanism, and constrain our model with observational data. \ Methods: We included an explicit coronal heating source term in the general 3D magnetohydrodynamic code NIRVANA to simulate the properties of the solar wind. The adapted heating mechanism is based on the interaction and subsequent dissipation of counter- propagating Alfv\ en waves in the solar corona, accounting for a turbulent heating rate Q$_p$. The sola ... Schleich, S.; Saikia, Boro; Ziegler, U.; Güdel, M.; Bartel, M.; Published by: \aap Published on: apr YEAR: 2023   DOI: 10.1051/0004-6361/202245009 Parker Data Used; magnetohydrodynamics (MHD); Solar wind; Sun: activity; turbulence; waves; Astrophysics - Solar and Stellar Astrophysics; Physics - Space Physics |
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