* Neutrinos: These are tiny, almost massless particles that interact very weakly with matter. They are produced in vast quantities in nuclear reactions within the Sun's core and stream out in all directions.
* Solar wind: This is a stream of charged particles, primarily protons and electrons, that constantly flows outward from the Sun's upper atmosphere (corona). It's responsible for phenomena like auroras and geomagnetic storms on Earth.
* Cosmic rays: These are high-energy particles that originate from various sources outside the solar system, including supernovae and active galactic nuclei. While not directly emitted by the Sun, they are influenced by the Sun's magnetic field and can sometimes interact with the solar wind.
While these particles are invisible to the naked eye, scientists use specialized detectors and telescopes to study them. This helps us understand the Sun's internal processes and their impact on the Earth.
