Laboratoire de Physique Statistique, Ecole Normale Supérieure, CNRS, Université Pierre et Marie Curie, Université Paris Diderot, Paris, France.
Phys Rev Lett. 2012 Apr 6;108(14):144501. doi: 10.1103/PhysRevLett.108.144501. Epub 2012 Apr 2.
We report the first experimental observation of a spatially localized dynamo magnetic field, a common feature of astrophysical dynamos and convective dynamo simulations. When the two propellers of the von Kármán sodium experiment are driven at frequencies that differ by 15%, the mean magnetic field's energy measured close to the slower disk is nearly 10 times larger than the one close to the faster one. This strong localization of the magnetic field when a symmetry of the forcing is broken is in good agreement with a prediction based on the interaction between a dipolar and a quadrupolar magnetic mode.
我们报告了空间局域化的星风发电机磁场的首次实验观测结果,这是天体物理星风发电机和对流星风发电机模拟的常见特征。当范卡门钠实验的两个螺旋桨以相差 15%的频率驱动时,靠近较慢的磁盘测量到的平均磁场能量几乎是靠近较快的磁盘的 10 倍。当强迫的对称性被打破时,磁场的这种强烈局域化与基于偶极子和四极子磁场模式之间相互作用的预测非常吻合。