Compressibility change in iron-rich melt and implications for core formation models

Chrystèle Sanloup; W. van Westrenen; R. Dasgupta; H. Maynard-Casely; J.-P. Perrillat

doi:10.1016/j.epsl.2011.03.039

Journal Articles Earth and Planetary Science Letters Year : 2011

Compressibility change in iron-rich melt and implications for core formation models

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Chrystèle Sanloup

Function : Author
PersonId : 11862
IdHAL : chrystele-sanloup
ORCID : 0000-0003-2412-6073
IdRef : 091939402

Institut des Sciences de la Terre de Paris

W. van Westrenen

Function : Author

Faculty of Earth and Life Sciences

R. Dasgupta

Function : Author

Department of Earth Sciences [Houston]

H. Maynard-Casely

Function : Author

Centre for Study at Extreme Conditions and School of Physics

J.-P. Perrillat

Function : Author

European Synchrotron Radiation Facility

Domains

Sciences of the Universe [physics] Earth Sciences

Marie José Queyroy : Connect in order to contact the contributor

https://hal.science/hal-00591407

Submitted on : Monday, May 9, 2011-10:59:59 AM

Last modification on : Thursday, June 9, 2022-8:20:06 AM

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hal-00591407 , version 1 (09-05-2011)

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HAL Id : hal-00591407 , version 1
DOI : 10.1016/j.epsl.2011.03.039

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Chrystèle Sanloup, W. van Westrenen, R. Dasgupta, H. Maynard-Casely, J.-P. Perrillat. Compressibility change in iron-rich melt and implications for core formation models. Earth and Planetary Science Letters, 2011, 306, pp.118-122. ⟨10.1016/j.epsl.2011.03.039⟩. ⟨hal-00591407⟩

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Compressibility change in iron-rich melt and implications for core formation models

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