Päikesekaitseteguri
Päikesekaitseteguri, also known as the solar wind interaction region, refers to the dynamic interaction between the solar wind—a stream of charged particles emanating from the Sun—and the magnetic fields and atmospheres of celestial bodies, particularly planets and moons. This phenomenon is crucial in understanding the space weather of a planetary system, including the formation of phenomena such as auroras, planetary magnetospheres, and radiation belts.
The solar wind, composed primarily of electrons and protons, travels outward from the Sun at speeds ranging
Without a strong magnetic field, such as on Mars or Venus, the solar wind can directly interact
Research in this field combines observations from space missions, such as NASA’s Parker Solar Probe or ESA’s