Rotating magnetospheres: a three dimensional approach

dc.contributor.advisorMichel, F. Curtisen_US
dc.creatorMorris, Clifford Deanen_US
dc.date.accessioned2018-12-18T21:17:23Zen_US
dc.date.available2018-12-18T21:17:23Zen_US
dc.date.issued1973en_US
dc.description.abstractSeveral authors have calculated the torque due to a stellar wind on a rotating body with an axisymmetric magnetic field. These discussions are restricted to the equatorial plane because the magnetic field structure is unknown elsewhere. Their treatment is here extended to the non-equatorial case. The axisymmetric magnetic field is described by a scalar function f. The various conservation equations allow the plasma flow to be described in terms of f. Although f has not been determined in the general case, it can be obtained in two special cases when the particle inertia is neglected. In the general case the Alfven critical points are obtained in terms of f, and with an assumption of a "minimum torque" solution, conditions on the angular momentum flow are found.en_US
dc.format.digitalOriginreformatted digitalen_US
dc.format.extent54 ppen_US
dc.identifier.callnoThesis Sp. Sci. 1973 Morrisen_US
dc.identifier.citationMorris, Clifford Dean. "Rotating magnetospheres: a three dimensional approach." (1973) Master’s Thesis, Rice University. <a href="https://hdl.handle.net/1911/104097">https://hdl.handle.net/1911/104097</a>.en_US
dc.identifier.digitalRICE1724en_US
dc.identifier.urihttps://hdl.handle.net/1911/104097en_US
dc.language.isoengen_US
dc.rightsCopyright is held by the author, unless otherwise indicated. Permission to reuse, publish, or reproduce the work beyond the bounds of fair use or other exemptions to copyright law must be obtained from the copyright holder.en_US
dc.titleRotating magnetospheres: a three dimensional approachen_US
dc.typeThesisen_US
dc.type.materialTexten_US
thesis.degree.departmentSpace Scienceen_US
thesis.degree.disciplineNatural Sciencesen_US
thesis.degree.grantorRice Universityen_US
thesis.degree.levelMastersen_US
thesis.degree.nameMaster of Scienceen_US
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