Proceedings of the Fourteenth ISAS Lunar and Planetary Symposium: July 20-22, 1981Hiroichi Hasegawa, Mikio Shimizu |
Contents
Inference of Optical Parameters of AirWater System from | 1 |
Cloud Models of Venus from The Point of View | 11 |
Joule Heating of the Jovian Ionosphere by Corotation | 73 |
Copyright | |
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accretion Alfvén wave altitude amino acid anticodon asteroids atmosphere Ba/Ca basalt calculated chondrite parent body chondrules circular polarization coefficient collision collisional condensation cooling rate core craters crystals curve density diffusion dipole distribution dust storm earth effect electrons elements energy equation eucrite Figure flux Fujii Fujiwara function Geophys grains heating model Hill sphere Icarus interplanetary ionization ionosphere isotopic ratio Kyoto layer Lunar magnetic field magnetosphere mantle Mars mass materials Matsui measured melt Mercury meteorite Miyamoto moon north polar cap observed olivine Oort cloud optical orbit ordinary chondrite orthopyroxene parameters particles phase pigeonite Pioneer Venus planet planetary planetesimals plasma Proc projectile protoplanets pyroxene radiation radius reflectance region rotation sabot sabot stopper Saito sample scattering seismic shown shows silicate sintering solar nebula solar system solar wind Space Sr/Ca stress surface taenite temperature terrestrial thermal tidal Tokyo tRNA variation velocity wavelength