Results 291 to 300 of about 104,383 (339)

Plasmas in Planetary Interiors

2005
We give an overview of the properties of matter in planetary interiors. Of special interest are the equation of state and the conductivities. This field has gained much more interest because of the detection of Jupiter-like, extrasolar planets since 1995.
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Convection in planetary interiors

Icarus, 1968
Abstract The aim of the present paper is to formulate explicitly the linearized equations safe-guarding the conservation of mass, energy, and momentum of viscous flow inside a heterogeneous, compressible, rotating fluid configuration, in which the coefficient of viscosity is an arbitrary function of radial distance, and the rotation is about a fixed
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Magnetic probing of planetary interiors

Physics of the Earth and Planetary Interiors, 1979
Abstract The following general question is addressed: what can be learned about a planetary interior from measurements of the global planetary magnetic field at (or near) its surface? The discussion is placed in the context of Earth, for clarity, but the considerations apply to terrestrial planets in general (so long as the observed magnetism is ...
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Introduction to planetary interiors

Proceedings of the International School of Physics “Enrico Fermi”
1.
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Risk assessment of microplastic particles

Nature Reviews Materials, 2022
Albert A Koelmans, Paula Redondo Hasselerharm, Nur Hazimah Mohamed Nor   +2 more
exaly  

Electromicrobiology: the ecophysiology of phylogenetically diverse electroactive microorganisms

Nature Reviews Microbiology, 2021
Derek R Lovley
exaly  

Planetary Interiors

2020
Colette Salyk, Kevin Lewis
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Rheology, Planetary Interior

2011
Stamenkovi{c}} Vlada, Sohl Frank
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Liquid Crystals: Versatile Self-Organized Smart Soft Materials

Chemical Reviews, 2022
Hari Krishna Bisoyi, Quan Li
exaly  

Fluid Dynamics of Planetary Interiors

1990
Following Monin (1973) and Gavrilin and Monin (1974), let us consider a simplified model of the Earth in three layers: (1) an outer solid spherical layer (mantle and crust) with an outer radius r1 ≈ 6370 km (radius of Earth) and an inner radius r2 ≈ 3470 km; (2) a liquid outer layer of the core; and (3) a solid spherical core with a radius r3 ≈ 1470 km,
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