Abstract Details

Name: Soumitra Hazra
Affiliation: University of Massachusetts Lowell
Conference ID: ASI2021_372
Title : Modeling Solar Wind Variations over an 11-yr Cycle with Alfvén Wave Dissipation: a Parameter Study
Authors and Co-Authors : Soumitra Hazra (UMass Lowell; CEA Saclay), Victor Reville (IRAP, Toulose, France), Barbara Perri (CEA Saclay, France), Antoine Strugarek (CEA Saclay, France), Allan Sacha Brun (CEA Saclay, France), Eric Buchlin (IAS, Universite Paris Saclay)
Abstract Type :
Abstract Category : Sun and the Solar System
Abstract : We study the behaviour and properties of the solar wind using a 2.5D Alfvén wave driven wind model. We first systematically compare the results of an Alfvén wave (AW) driven wind model with a polytropic approach. Polytropic magnetohydrodynamic wind models are thermally driven, while Alfvén waves act as additional acceleration and heating mechanisms in the Alfvén wave driven model. We confirm that an AW-driven model is required to reproduce the observed bimodality of slow and fast solar winds. We are also able to reproduce the observed anti-correlation between the terminal wind velocity and the coronal source temperature with the AW-driven wind model. We also show that the wind properties along an eleven year cycle differ significantly from one model to the other. The AW-driven model again shows the best agreement with observational data. Indeed, solar surface magnetic field topology plays an important role in the Alfvén wave driven wind model, as it enters directly into the input energy sources via the Poynting flux. On the other hand, the polytropic wind model is driven by an assumed pressure gradient; thus it is relatively less sensitive to the surface magnetic field topology. Finally, we note that the net torque spinning down the Sun exhibits the same trends in the two models, showing that the polytropic approach still captures correctly the essence of stellar winds.