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Thermal Structure of Planetary Ionospheres
1973Electrons released in the photoionization process due to the absorption of solar XUV radiation in planetary atmospheres may have initially kinetic energies of one to 100 eV. The energy E of photoelectrons resulting from photons of energy h v interacting with an atmospheric constituent whose ionization potential is IP is given by $$E = hv - IP ...
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Atomic Data and the Density Structures of Planetary Nebulae
Monthly Notices of the Royal Astronomical Society, 2021Mónica Rodríguez
exaly
An Expression Method of Kinematic and Structure Diagrams for Planetary Gear Systems
Mechanisms and Machine Science, 2022Le Huy Vu
exaly
A Method for Detecting Degenerate Structures in Planetary Gear Trains
Mechanism and Machine Theory, 2005D R Salgado
exaly
Automatic Analysis of Kinematic Structure of Planetary Gear Trains
Journal of Mechanical Design, Transactions of the ASME, 1993Cheng-Ho Hsu
exaly
Automatic Detection of Embedded Structure in Planetary Gear Trains
Journal of Mechanical Design, Transactions of the ASME, 1997Yi-Chang Wu, Cheng-Ho Hsu
exaly

