%0 Generic %1 citeulike:14090495 %A Shivamoggi, B. K. %D 2016 %K imported %T Parker's Model for Stellar Wind and Magnetohydrodynamic Extensions %U http://arxiv.org/abs/1607.01380 %X In this paper, we first revisit Parker's hydrodynamic model for a stellar wind and make further analytic considerations. We show that the visualization of an effective de Laval type nozzle associated with Parker's model is valid only in a superficial sense and not on the dynamical level. We then make an analytic considerations on the Weber-Davis magnetohydrodynamic (MHD) extension of Parker's model with a view to provide a qualitative understanding of the coupling between the magnetic field and the plasma motion in the stellar wind. We find that, *the MHD azimuthal velocity profile actually resembles that for hydrodynamic Lamb-Oseen vortex; *Keplerian-orbit conditions prevail near a strong rotator even in a magnetized situation; *Parker's hydrodynamic scenario Par seems to reappear in the strong magnetization regime.itemize

@misc{citeulike:14090495, abstract = {In this paper, we first revisit Parker's hydrodynamic model for a stellar wind and make further analytic considerations. We show that the visualization of an effective de Laval type nozzle associated with Parker's model is valid only in a superficial sense and not on the dynamical level. We then make an analytic considerations on the Weber-Davis magnetohydrodynamic (MHD) extension of Parker's model with a view to provide a qualitative understanding of the coupling between the magnetic field and the plasma motion in the stellar wind. We find that, *the MHD azimuthal velocity profile actually resembles that for hydrodynamic Lamb-Oseen vortex; *Keplerian-orbit conditions prevail near a strong rotator even in a magnetized situation; *Parker's hydrodynamic scenario \cite{Par} seems to reappear in the strong magnetization regime.\end{itemize}}, added-at = {2019-03-25T08:20:55.000+0100}, archiveprefix = {arXiv}, author = {Shivamoggi, B. K.}, biburl = {https://www.bibsonomy.org/bibtex/29f3f3e18cf9789b07f35c82ad3d80134/ericblackman}, citeulike-article-id = {14090495}, citeulike-linkout-0 = {http://arxiv.org/abs/1607.01380}, citeulike-linkout-1 = {http://arxiv.org/pdf/1607.01380}, day = 5, eprint = {1607.01380}, interhash = {5fc32446c4d79fb742ac8ff696bb3a12}, intrahash = {9f3f3e18cf9789b07f35c82ad3d80134}, keywords = {imported}, month = jul, posted-at = {2016-07-06 20:59:16}, priority = {2}, timestamp = {2019-03-25T08:20:55.000+0100}, title = {{Parker's Model for Stellar Wind and Magnetohydrodynamic Extensions}}, url = {http://arxiv.org/abs/1607.01380}, year = 2016 }