Methylmercury (CH3Hg+, MMHg) in the phytoplankton
and zooplankton, which form the bottom of marine food webs, is a good
predictor of MMHg in top predators, including humans. Therefore, evaluating
the potential exposure of MMHg to higher trophic levels (TLs) requires
a better understanding of relationships between MMHg biomagnification
and plankton dynamics. In this study, a coupled ecological/physical
model with 366 plankton types of different sizes, biogeochemical functions,
and temperature tolerance is used to simulate the relationships between
MMHg biomagnification and the ecosystem structure. The study shows
that the MMHg biomagnification becomes more significant with increasing
TLs. Trophic magnification factors (TMFs) in the lowest two TLs show
the opposite spatial pattern to TMFs in higher TLs. The low TMFs are
usually associated with a short food-chain length. The less bottom-heavy
trophic pyramids in the oligotrophic oceans enhance the MMHg trophic
transfer. The global average TMF is increased from 2.3 to 2.8 in the
warmer future with a medium climate sensitivity of 2.5 °C. Our
study suggests that if there are no mitigation measures for Hg emission,
MMHg in the high-trophic-level plankton is increased more dramatically
in the warming future, indicating greater MMHg exposure for top predators
such as humans.