Compilations of U/Pb zircon geochronology from igneous rocks and arc-derived sediments show age peaks and troughs defining magmatic "flare-ups" and "lulls," respectively, on the timescales of tens of millions of years (e.g., Paterson & Ducea, 2015). Typically, these flare-ups or high magma flux events last ∼30 Myr and are separated by magmatic lulls spanning 20-50 Myr (e.g., Kirsch et al., 2016). Magma generation rates during the lulls in a continental arc are comparable to the rate of mantle-derived primitive magma generation in island arcs (DeCelles et al., 2009), representing a baseline for the magma contribution from the mantle wedge. The Armstrong unit (AU) is used to quantify the baseline magma generation rate, with 1 AU = 30 km 3 /Myr per kilometer length of arc (DeCelles et al., 2009; Reymer & Schubert, 1984). During a flare-up, the magma generation rate reaches 3-4 AU in the upper-middle crust (DeCelles et al., 2009). The AU can be converted to a volumetric flux (km 3 /km 2 /Myr or km/Myr) if the arc width is known. Given a characteristic arc width of 100 km, the baseline 1 AU is ∼0.3 km 3 /km 2 /Myr. For flare-ups in continental magmatic arcs, an estimated volumetric flux of ∼1 km 3 /km 2 /Myr (∼3-4 AU equivalent) is proposed for the main arc and > 0.6 km 3 /km 2 /Myr (>2 AU equivalent) for a broader region from the forearc to the retro-arc (Ratschbacher et al., 2019). This volumetric flux is also referred to as the magmatic thickening rate (km/Myr), representing