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APPLICATION OF AN HYBRID MHD WIND MODEL WITH LATITUDINAL DEPENDENCES TO THE ULYSSES SOLAR WIND DATA AT MINIMUM

机译:混合MHD风模型在延迟依赖于妇女依赖于尤利索太阳风数据的应用

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From two different models of exact axisymmetric analytical solutions of the MHD equations that govern a magnetized and rotating object, a new hybrid model is presented. The hybrid model input parameters are set from ULYSSES data of the solar wind for solar minimum. Using spacecraft data, the latitudinal dependences of density, velocity and magnetic field are constrained. This hybrid model is built having in mind the high flexibility of the parent models when applied in their proper domains. For the dead-zone, a three component solution for velocity and magnetic field is used, providing a wind geometry with non-radial streamlines and enabling the description of usual flaring of the field lines ob served in coronal holes, specially during the solar minimum (Tsinganos Sauty 1992, Sauty Tsinganos 1994). From the Alfven radius to one a.u. and further, the hybrid model keeps the latitudinal dependence as flexible as possible, this means to give up the latitudinal component of velocity and magnetic field and work with the remainders, turning the stream-lines into radial ones (Lima, Priest Tsinganos, 2001). This two component model provides the latitudinal versatility needed to deal with sharp variations of certain quantities near the equator, which are ob- served in ULYSSES data. The hybrid model allows describing the behaviour of all physical quantities with some agreement with the observational data.
机译:从管理一个磁化和旋转物体的MHD方程精确对称解析解两种不同型号,一种新的混合模型。混合模型输入参数是从太阳风太阳能最小的ULYSSES数据集。使用宇宙飞船数据,密度,速度和磁场的纬度依赖性被约束。这种混合模式的一点,当在其适当的领域应用内置有父模型的高度灵活性。为死区,对速度和磁场的三成组分溶液时,提供具有非径向流线的风力几何形状和使在冕洞OB所服务的场线通常燃烧的描述中,特别在太阳能最小值( Tsinganos Sauty 1992年,Sauty Tsinganos 1994年)。从阿尔芬半径一个A.U.并且进一步地,混合模型保持纬向依赖性尽可能地灵活,这装置放弃速度和磁场和工作与余数的纬度分量,转动流线成径向酮(利马,牧师Tsinganos,2001) 。此双组分模型提供了处理在赤道附近一定量的急剧变化,这是在转播数据ULYSSES服务所需的纬向通用性。混合模式可以描述与观测数据的一些协议的所有物理量的行为。

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