Neutron stars, pulsars, and magnetars do not experience solar weather phenomena like the Sun, such as solar flares or sunspots. While they do have unique events, such as starquakes and pulsar winds, these are fundamentally different from solar weather. Starquakes can significantly impact a magnetar's magnetic field and occur due to the crust's compression. The magnetic fields of neutron stars are vastly stronger than those of main sequence stars, leading to different types of magnetospheric events. Overall, while there are analogous phenomena, they do not equate to traditional solar weather.