Simulations tie the deep-mantle primordial neon reservoir to an initial embryo mass of ~0.3 Earth masses assembled during solar-nebula dispersal.
Nonlinear Processes in Geophysics 22(4):371--376
2 Pith papers cite this work. Polarity classification is still indexing.
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Fills the 1858.9-1860.9 gap in IERS C01 Y_p using parametric astronomical and SSA models, preferring SSA for its more complete representation.
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Constructing Earth Formation History Using Deep Mantle Noble Gas Reservoirs
Simulations tie the deep-mantle primordial neon reservoir to an initial embryo mass of ~0.3 Earth masses assembled during solar-nebula dispersal.
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Filling the gap in the IERS C01 polar motion series in 1858.9-1860.9
Fills the 1858.9-1860.9 gap in IERS C01 Y_p using parametric astronomical and SSA models, preferring SSA for its more complete representation.