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Planetary

Isaac Newton modestly claimed to have stood on the shoulders of giants to explain how he was able to achieve his outstanding discoveries in the fields of gravitational attraction and planetary motion our Giants in the field of electromagnetic induction would probably have said the same. [Pg.272]

The miderstanding of the quantum mechanics of atoms was pioneered by Bohr, in his theory of the hydrogen atom. This combined the classical ideas on planetary motion—applicable to the atom because of the fomial similarity of tlie gravitational potential to tlie Coulomb potential between an electron and nucleus—with the quantum ideas that had recently been introduced by Planck and Einstein. This led eventually to the fomial theory of quaiitum mechanics, first discovered by Heisenberg, and most conveniently expressed by Schrodinger in the wave equation that bears his name. [Pg.54]

In fact, even in the solar system, despite the relative strengths of planetary attraction, there are constituents, the asteroids, with very irregular, chaotic behaviour. The issue of chaotic motion in molecules is an issue that will appear later with great salience.)... [Pg.55]

The astrochemistty of ions may be divided into topics of interstellar clouds, stellar atmospheres, planetary atmospheres and comets. There are many areas of astrophysics (stars, planetary nebulae, novae, supemovae) where highly ionized species are important, but beyond the scope of ion chemistry . (Still, molecules, including H2O, are observed in solar spectra [155] and a surprise in the study of Supernova 1987A was the identification of molecular species, CO, SiO and possibly ITf[156. 157]. ) In the early universe, after expansion had cooled matter to the point that molecules could fonn, the small fraction of positive and negative ions that remained was crucial to the fomiation of molecules, for example [156]... [Pg.819]

For remote sensing, spectroscopy at THz frequencies holds the key to our ability to remotely sense enviromnents as diverse as primaeval galaxies, star and planet-fonuing molecular cloud cores, comets and planetary atmospheres. [Pg.1233]

Nellis W J, Flamilton D C, Flolmes N C, Radousky FI B, Ree F FI, Mitohell A C and Niool M 1988 The nature of the interior of Uranus based on studies of planetary ioes at high dynamio pressure Science 240 779... [Pg.1964]

Anoilotto F, Chiarotti G L, Soandolo S and Tosatti E 1997 Dissooiation of methane into hydrooarbons at extreme (planetary) pressure and temperature Science 275 1288... [Pg.1964]

Hubbard WB 1984 Planetary Interiors (New York Van Nostrand-Reinhold)... [Pg.1965]

Bauer S J 1973 Physics of Planetary Ionospheres (Berlin Springer)... [Pg.2813]

S. R. Taylor, Planetary Science A. PunarPerspective, Lunar and Planetary Institute, Houston, Tex., 1982. [Pg.102]

Assemblies of small disks are rotated in a planetary movement around a central screw conveyor. The disks are mounted on six hoUow axles and the axles revolve on overhanging bearings from the gearbox at one end of the vessel where they are driven, via a drive shaft, by an electric motor. The filtrate is collected from the disks via the hoUow shafts and a filter valve into a large collecting pipe. The hoUow shafts also collect the water and air from the dewatering process, in another part of the rotational cycle. The number of disks mounted on the shafts can be adjusted for different materials, depending on the required capacity and the cake thickness to be used. [Pg.406]

As the vessel is only about half filled with slurry, the disks become coated with the cake when immersed, the cake is dewatered when the disks emerge from the slurry, and scraped or blown off, by reverse blow, into the central conveyor which takes the cake to one end of the vessel. The planetary action and the slow movement of the disks through the feed slurry ensure exceptionally good homogeneity of the cake which is critically important for good dewatering characteristics the typical speed of rotation of the planetary system of shafts is from 0.8 to 1 rpm. [Pg.406]

Fig. 3. Schematic of three commonly used types of MOCVD reactors where the arrows indicate gas flow (a) vertical rotating disk where (— represents an inlet to promote a laterally uniform gas flow, (b) planetary rotation, and (c) hori2ontal. Fig. 3. Schematic of three commonly used types of MOCVD reactors where the arrows indicate gas flow (a) vertical rotating disk where (— represents an inlet to promote a laterally uniform gas flow, (b) planetary rotation, and (c) hori2ontal.
Twin shell Vibratory pehhle mill tiirretf Vertical screw planetary types Cage mill Screw feeders... [Pg.1764]

Planetary Ball Milling This is a method of increasing the gravitational force acting on balls in a ball mill. For example, refractoiy metals and carbides can be ground to 1 to 2.6 [Lm in 5 to 20 min in an apparatus capable of applying a centrifugal force of 10 to 50 G. [Dobrovol sldi, Poroshk. MetalL, 7(6), 1-7 (1967)]. [Pg.1857]

Pulverit planetaiy mills are available from Geoscience Inc. Highspeed planetary-baU mills can be used to perform rapid tests to sinmlate ball milhng of materials [Vock, DECHEMA-Monogr, 69, HI-8 (1972)]. The size of high-speed mills will be much smaller than the size of same-capacity ball mills [Bradley, S. Afr Mech. Eng., 22, 129 (1972)]. [Pg.1857]

Batch planetary mixers are used extensively in the pharmaceutical industiy for powder granulation. A typical batch size of 100 to 200 kg has a power input of 10 to 20 kW. Mixing times in these granulators are quite long (20 to 40 min). [Pg.1894]


See other pages where Planetary is mentioned: [Pg.284]    [Pg.316]    [Pg.337]    [Pg.4]    [Pg.1175]    [Pg.1233]    [Pg.1235]    [Pg.1235]    [Pg.1243]    [Pg.1960]    [Pg.230]    [Pg.1069]    [Pg.49]    [Pg.99]    [Pg.99]    [Pg.409]    [Pg.440]    [Pg.156]    [Pg.157]    [Pg.429]    [Pg.457]    [Pg.313]    [Pg.368]    [Pg.412]    [Pg.115]    [Pg.316]    [Pg.509]    [Pg.292]    [Pg.307]    [Pg.1732]    [Pg.1766]    [Pg.1820]    [Pg.445]    [Pg.76]   
See also in sourсe #XX -- [ Pg.22 ]

See also in sourсe #XX -- [ Pg.292 ]




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Abundances in planetary atmospheres

Abundances in planetary nebulae

Albedo mean planetary

Atmosphere planetary, composition

Atomic models planetary

Atoms planetary model

Ball mill planetary

Ball planetary

Ball-milling planetary

Bohr s planetary model

Clouds planetary systems

Component planetary

Compositional evolution planetary differentiation

Cosmochemistry, Planetary and Space Science

Detection of Planetary Atmospheres

Differentiation planetary

Earth, planetary features

Element fractionation resulting from planetary differentiation

Extra-Solar planetary system

Extrasolar planetary systems

Finding Other Planetary Ties

Fractionation planetary differentiation

From interstellar space to planetary atmospheres

Granulators batch planetary

Homogeneous systems from interstellar space to planetary atmospheres and primitive soup models

Influence planetary tables

Jupiter planetary tables

Lithophile elements planetary differentiation

Lunar and Planetary

Materials Properties for Modeling Planetary Formation

Measured radiation from planetary objects up to Neptune

Meteorites a record of nebular and planetary processes

Milling planetary mills

Mixer, planetary gear

Nebula planetary

Noble gases planetary atmospheres

Noble gases planetary components

Observational results on abundances in planetary nebulae

Oxygen planetary differentiation

PLANETARY EXTRUDER

PLANETARY ROLLER

PLANETARY ROLLER EXTRUDER

Planet formation planetary

Planetary Distribution of Apatite

Planetary Extruders

Planetary Fourier Spectrometer

Planetary Magnetic Fields as Tests for Dynamo Mechanisms

Planetary Noble Gases

Planetary Radar Astronomy

Planetary Ring Dynamics

Planetary accretion

Planetary albedo

Planetary atmospheres

Planetary atmospheres Earth

Planetary atmospheres Venus

Planetary atmospheres physical properties

Planetary atmospheres troposphere

Planetary atoms

Planetary blender

Planetary boundary layer

Planetary boundary layer defined

Planetary chemistry

Planetary coolers

Planetary destruction

Planetary differentiation abundances

Planetary differentiation basalts

Planetary differentiation composition

Planetary differentiation core formation

Planetary differentiation isotopic ratios

Planetary differentiation magma oceans

Planetary differentiation partitioning

Planetary differentiation primitive mantle composition

Planetary differentiation refractory elements

Planetary differentiation solar system composition

Planetary differentiation structure

Planetary differentiation volatile elements

Planetary distances

Planetary frontal zone

Planetary gear assembly

Planetary gear extruder

Planetary gear extruders

Planetary golden spiral

Planetary ices

Planetary magnetic field

Planetary mantles, core formation

Planetary mass spectrometer experiments

Planetary mass-dependent fractionations

Planetary mill

Planetary mixers

Planetary model

Planetary model of atom

Planetary motion

Planetary noble gas abundance patterns

Planetary orbital changes

Planetary orbits

Planetary physics

Planetary radiation

Planetary reactor

Planetary rulers

Planetary satellites

Planetary science

Planetary spiral

Planetary structure

Planetary surface

Planetary surface dynamics

Planetary system formation

Planetary systems

Planetary tables

Planetary tectonics

Planetary three-body problem

Planetary transits

Planetary warming

Planetary waves

Planetary-centrifugal milling

Planetary-paddle mixer

Planets/planetary compositions

Plate tectonics planetary

Pressure planetary atmospheres

Proto-planetary disks

Proto-planetary nebulae

Radiative Transfer in Planetary Atmospheres

Radiative Transfer in Planetary Subsurfaces

Radio Astronomy, Planetary

Radiogenic isotope fractionation and planetary differentiation

Rutherford, "planetary" model

Rutherford’s planetary model of the

Screw planetary

Siderophile elements planetary differentiation

Solar system planetary differentiation

Temperatures planetary atmospheres

Terrestrial planets planetary embryos

The Planetary Boundary Layer

The Planetary Model

Thermal processing of the pre-planetary material

Venus planetary tables

Viscous materials, mixing planetary

Wide-Field Planetary camera

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