Drawdown of Atmospheric pCO2 via Variable Particle Flux Stoichiometry in
the Ocean Twilight Zone
Abstract
The strength of the biological soft tissue pump in the ocean critically
depends on how much organic carbon is produced via photosynthesis and
how efficiently the carbon is transferred to the ocean interior. For a
given amount of limiting nutrient, phosphate, soft tissue pump would be
strengthened if the carbon (C) to phosphorus (P) ratio of sinking
organic matter increases as the remineralization length scale of C
increases. Here, we present a new data compilation of particle flux
stoichiometry and show that C:P of sinking particulate organic matter
(POM) in the ocean twilight zone on average is likely to be higher than
the C:P ratio of surface suspended POM. We further demonstrate using a
physics-biology coupled global ocean model combined with a theory from
first principles that an increase in C:P export flux ratio in the
ocean’s twilight zone can lead to a considerable drawdown of atmospheric
pCO2.