By analogy, a neutron star born rotating as fast as or faster than the convective period of 10 milliseconds could develop a widespread, ultrastrong magnetic field.
By analogy, a neutron star born rotating as fast as or faster than the convective period of 10 milliseconds could develop a widespread, ultrastrong magnetic field.
以此类推，在中子星诞生的时候，要是它的自转速率和10毫秒的对流周期一样快，甚至更快，就能发展出大区域的超强磁场。