Volcanic eruptions are one of the main natural causes of radiatively forced climatic changes over the Common Era, producing fluctuations on interannual to multi-year timescales. The analysis and interpretation of such changes has resulted in a wide body of research, especially following the influential work of H.H. Lamb (Lamb & Stanley, 1970), and expanding into many efforts to characterize and model the climate response to volcanism (e.g., Robock, 2000;Sigl et al., 2015;Zanchettin et al., 2016). It is now well understood that explosive volcanic eruptions can alter climate by injecting large amounts of sulfur-containing gases into the stratosphere, such as SO 2 and H 2 S, leading to the formation of liquid sulfate aerosols (Toohey & Sigl, 2017). These aerosols consequently scatter incoming solar radiation and absorb infrared radiation, which in turn leads to a net decrease in radiation reaching the Earth's surface and associated global cooling (Robock, 2000). The introduction of satellite observations led to rapid advancements in our understanding of how stratospheric aerosols affect global temperature, particularly since the El Chichon eruption in 1983 (e.g., Robock, 1983;Robock & Matson, 1983). This event served as a natural experiment to test and develop monitoring instruments and improved representations of atmospheric chemistry in climate models, which in turn improved simulations of the climate effects due to volcanic aerosols in the stratosphere (Rampino & Self, 1984). With the exception of the eruption of Mt. Pinatubo in 1991, however, the volcanic events monitored during the 20th century are of a much smaller magnitude than many of those that have occurred over the Common Era. Further improvement in our understanding of the impacts and dynamics of large volcanic eruptions is therefore dependent on high-resolution proxy reconstructions and model simulations of the larger volcanic events that occurred before the widespread availability of instrumental records. The