This is called the pulsar’s magnetic inclination and it’s often quite far from 0, all the way to nearly orthogonal. Yes but this is a dynamic process that prod

This is called the pulsar’s magnetic inclination and it’s often quite far from 0, all the way to nearly orthogonal. Yes but this is a dynamic process that produces more correlated stars as the galaxy ages. Astronomers routinely measure such parameters using models to provide confidence bounds for their estimates. https://arxiv.org/pdf/2404.13857 https://arxiv.org/pdf/2404.13857