Mathis P. Hain, Ph.D.

Affiliations: 
2013 Geosciences Princeton University, Princeton, NJ 
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"Mathis Hain"

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Daniel M. Sigman grad student 2013 Princeton
 (Glacial/interglacial and deglacial changes in ocean circulation and their consequences for the global carbon cycle: A model study.)
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Publications

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Rafter PA, Gray WR, Hines SKV, et al. (2022) Global reorganization of deep-sea circulation and carbon storage after the last ice age. Science Advances. 8: eabq5434
Piccione G, Blackburn T, Tulaczyk S, et al. (2022) Subglacial precipitates record Antarctic ice sheet response to late Pleistocene millennial climate cycles. Nature Communications. 13: 5428
Paytan A, Griffith EM, Eisenhauer A, et al. (2021) A 35-million-year record of seawater stable Sr isotopes reveals a fluctuating global carbon cycle. Science (New York, N.Y.). 371: 1346-1350
Wu Y, Hain MP, Humphreys MP, et al. (2019) What drives the latitudinal gradient in open-ocean surface dissolved inorganic carbon concentration? Biogeosciences. 16: 2661-2681
Rafter PA, Carriquiry JD, Herguera J, et al. (2019) Anomalous > 2000‐Year‐Old Surface Ocean Radiocarbon Age as Evidence for Deglacial Geologic Carbon Release Geophysical Research Letters. 46: 13950-13960
Hawkings JR, Hatton JE, Hendry KR, et al. (2018) The silicon cycle impacted by past ice sheets. Nature Communications. 9: 3210
Kemeny PC, Kast ER, Hain MP, et al. (2018) A Seasonal Model of Nitrogen Isotopes in the Ice Age Antarctic Zone: Support for Weakening of the Southern Ocean Upper Overturning Cell Paleoceanography and Paleoclimatology. 33: 1453-1471
Hain MP, Foster GL, Chalk T. (2018) Robust Constraints on Past CO2 Climate Forcing From the Boron Isotope Proxy Paleoceanography and Paleoclimatology. 33: 1099-1115
Sosdian S, Greenop R, Hain M, et al. (2018) Constraining the evolution of Neogene ocean carbonate chemistry using the boron isotope pH proxy Earth and Planetary Science Letters. 498: 362-376
de Souza GF, Khatiwala SP, Hain MP, et al. (2018) On the origin of the marine zinc–silicon correlation Earth and Planetary Science Letters. 492: 22-34
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