The emission of greenhouse gases (GHGs) has increased rapidly since the pre-industrial era (1750 C.E.). The concentration of GHGs in the atmosphere has reached a historic level, inducing various unwanted phenomena, such as global warming, glacier melting, and extreme weather events (IPCC, 2014). Among the primary GHGs [water vapor, carbon dioxide (CO 2 ), methane, nitrous oxide, and ozone], CO 2 is the most important as it has strong infrared absorption and contributes ∼66% of the radiative forcing by long-lived GHGs (Stuiver & Quay, 1981). Currently, sources/sinks and biogeochemical cycling of CO 2 play an important role in global climate change, and their abundance is considered to further continue being a dominant factor for future climate change (Albritton et al., 2001;Li et al., 2014). According to the IPCC AR5 Synthesis Report, the global mean surface temperature in the late twenty-first century would be largely determined by the cumulative emission of CO 2 (IPCC, 2014). Ice core studies reveal that the atmospheric CO 2 mole fraction was only approximately 278 ppm around 1750 C.E.