Hagay Amit, Ph.D.
Affiliations: | 2006 | Johns Hopkins University, Baltimore, MD |
Area:
GeophysicsGoogle:
"Hagay Amit"Parents
Sign in to add mentor| Peter Olson | grad student | 2006 | Johns Hopkins | |
| (Imaging core flow from geomagnetic secular variation: Consequences for core-mantle interactions and geomagnetic dipole moment changes.) | ||||
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Publications
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| Amit H, Deguen R, Driscoll P, et al. (2019) Editorial: Stratification in the Cores of Earth and Other Planets Frontiers in Earth Science. 7 |
| Pinheiro K, Amit H, Terra-Nova F. (2019) Geomagnetic jerk features produced using synthetic core flow models Physics of the Earth and Planetary Interiors. 291: 35-53 |
| Huguet L, Amit H, Alboussière T. (2018) Geomagnetic Dipole Changes and Upwelling/Downwelling at the Top of the Earth's Core Frontiers in Earth Science. 6 |
| Peña D, Amit H, Pinheiro KJ. (2018) Deep magnetic field stretching in numerical dynamos Progress in Earth and Planetary Science. 5 |
| Thébault E, Langlais B, Oliveira J, et al. (2018) A time-averaged regional model of the Hermean magnetic field Physics of the Earth and Planetary Interiors. 276: 93-105 |
| Peña D, Amit H, Pinheiro KJ. (2016) Magnetic field stretching at the top of the shell of numerical dynamos 1. Geomagnetism Earth, Planets and Space. 68 |
| Choblet G, Amit H, Husson L. (2016) Constraining mantle convection models with palaeomagnetic reversals record and numerical dynamos Geophysical Journal International. 207: 1165-1184 |
| Huguet L, Amit H, Alboussière T. (2016) Magnetic to magnetic and kinetic to magnetic energy transfers at the top of the Earth's core Geophysical Journal International. 207: 934-948 |
| Terra-Nova F, Amit H, Hartmann GA, et al. (2016) Using archaeomagnetic field models to constrain the physics of the core: robustness and preferred locations of reversed flux patches Geophysical Journal International. 206: 1890-1913 |
| Sahoo S, Sreenivasan B, Amit H. (2016) Dynamos driven by weak thermal convection and heterogeneous outer boundary heat flux Physics of the Earth and Planetary Interiors. 250: 35-45 |