SVzon

The study models the magnetic action of Jupiter's zonal winds and has been submitted to JGR planets (authors J.Wicht and U.R.C. Christensen, 2023). The field model JRM09 is used as a background field and my study the field changes and secular variation. Several different zonal winds models and two electrical conductivity models are used. The magnetic field changes induced by the winds are modelled by integrating in time with the Matlab package SVzon. The data provided here contain the Matlab package, a manual, and all required data and results for the JGR article.

本项研究模拟了木星带状风磁效应，并将其成果提交至《行星物理学杂志》（JGR planets），作者为J.Wicht和U.R.C. Christensen，发表于2023年。本研究以场模型JRM09作为背景场，探讨场的变化与长期变化。研究采用了多种带状风模型以及两种电导率模型。通过Matlab软件包SVzon对时间进行积分，对风诱导的磁场变化进行了建模。所提供的数据包括Matlab软件包、操作手册以及所有支持《行星物理学杂志》文章所需的数据和结果。