Presentation #431.01 in the session The Sun and Solar System III.
Galactic cosmic rays propagate in the heliosphere and interact with the solar surface and its surroundings. This generates quiet non-thermal emission from the Sun that extends up to hundreds of GeV. The study of this emission provides a huge potential for understanding cosmic rays, the Sun and its environment, the solar activity, and the solar magnetic field. We present theoretical advancements in the modeling of quiet solar emission.