With the solar activity expected to decline during the coming decades, the assessment of solar influences on temperature and composition of the middle atmosphere is crucial for identifying the natural forcing contribution to long-term climate variability. One aspect of solar activity is Energetic Particle Precipitation (EPP), either directly by coronal mass ejections producing sporadically large fluxes of solar energetic particles or indirectly by the quasi-continuous, but highly variable, impact of the solar wind on the Earth’s magnetosphere. EPP causes enhanced ionisation in the polar upper mesosphere and lower thermosphere leading to the formation of nitrogen oxides. These can be transported down, affecting the stratospheric ozone layer, and potentially interfering with polar ozone recovery. This, in turn, can affect the regional weather systems in mid-to high latitudes. EPP is therefore recognized as an integral part of the solar climate forcing.