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In the following short review we will outline some of the possibleinteraction processes of lower solar atmospheric plasma with the embeddedsmall-scale solar magnetic fields. After introducing the topic, important typesof small-scale solar magnetic field elements are outlined to then focus ontheir creation and evolution, and finally end up describing foremost processesthese magnetic fields are involved in, such as the reconnection of magneticfield lines and the creation of magneto-hydrodynamic waves. The occurrence andglobal coverage in the solar atmosphere of such small-scale phenomena surpasson average those of the more explosive and intense events, mainly related tosolar active regions, and therefore their key role as building blocks of solaractivity even during the weaker phases of the 11-year solar cycle. Inparticular, understanding the finest ingredients of solar activity from thelower to the upper solar atmosphere could be determinant to fully understandthe heating of the solar corona, which stands out as one of the most intriguingproblems in astrophysics nowadays.

Interaction of convective plasma and small-scale magnetic fields in the lower solar atmosphere