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The internal structure of planetary bodies
Contemporary Physics, 1972Abstract Each planet in the Solar System is represented as a mechanically spherical cold body, possibly in rotation. It is seen that, on this basis, the properties of the planets can be understood within the already established principles of the physics of matter under high pressures.
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Temperature structure of nongray planetary atmospheres
Icarus, 1969Abstract To reduce by several orders of magnitude the number of frequency points needed in calculating net fluxes for molecular atmospheres, transmission average opacities are introduced. A power-law representation of these broad-band opacities is suggested for paths at constant pressure and temperature and generalized to nonhomogeneous paths.
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Fresnel zone structure in planetary occultations
Radio Science, 1981In many planetary and satellite occultations, both at light and at radio wavelengths, there may exist two propagation paths around an occulting body. The shorter of these two paths traverses the nearest portion of the limb, supports a stronger signal, and accounts for all radio occultation measurements to date.
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Structural design options for planetary entry
9th Structural Dynamics and Materials Conference, 1968Structural design options for decelerative aeroshell configurations for atmospheric entry on unmanned planetary ...
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Empirical constraints on turbulence in proto-planetary discs
New Astronomy Reviews, 2023Giovanni P Rosotti
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Triboelectric sensor for planetary gear fault diagnosis using data enhancement and CNN
Nano Energy, 2022Mingyu Yu, Di Yu
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Life-cycle assessment to guide solutions for the triple planetary crisis
Nature Reviews Earth & Environment, 2023Stefanie Hellweg +2 more
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