Encyclopedia of Physical Science and Technology, Volume 2Robert Allen Meyers |
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Page 53
... region from 40 to 1000 μm . The wavelength range of 200 μm- 1000 μm is often called the submillimeter region . Interstellar dust : Solid grains that lie in the general galactic medium or within higher density clouds . Magnitude scale ...
... region from 40 to 1000 μm . The wavelength range of 200 μm- 1000 μm is often called the submillimeter region . Interstellar dust : Solid grains that lie in the general galactic medium or within higher density clouds . Magnitude scale ...
Page 291
... region low in the plasma , just above the inducted coil . This is a high - back- ground region , but the optimum sensitivity is achieved there because the signals are so large . In AFS the sensitivity of the measurements is very poor in ...
... region low in the plasma , just above the inducted coil . This is a high - back- ground region , but the optimum sensitivity is achieved there because the signals are so large . In AFS the sensitivity of the measurements is very poor in ...
Page 777
... REGION A voltage drop of the order of 2 to 12 V ( de- pending upon electrode material , the environ- ment , and current magnitude ) is typically ob- served in the anode fall region . In this region electrons bombard the anode surface ...
... REGION A voltage drop of the order of 2 to 12 V ( de- pending upon electrode material , the environ- ment , and current magnitude ) is typically ob- served in the anode fall region . In this region electrons bombard the anode surface ...
Contents
Executive Advisory Board ii BASIC Programming Language | 353 |
Editorial Advisory Board v Thomas E Kurtz | 373 |
Batteries | 387 |
Copyright | |
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absorption acid aldoses angular momentum applications asbestos atmosphere atoms auroral axis BASIC black hole Boolean algebra boundary layer carbon fibers catalyst cell charge chemical chrysotile clouds collision concentration cross section crystallites density developed disaccharide dust electric electron elements emission emitted energy engine equation example expert system field flux frequency function galaxies heat hemiacetal hydrogen hydroxyl groups infrared interaction interstellar interstellar medium ionization ions kinetic light magnetic mass material measurements mechanical ment metal method molecular molecules momentum monosaccharides motion nucleophile observed oligosaccharides operation optical orbit oxidation oxygen particles photons plane plume potential problem radiation reaction reactor region result saccharides sample satellite signal solar solution spectral spectroscopy spectrum speed stars stellar structure surface techniques temperature thermal tion transfer turbulence ture typical velocity vertical voltage wave wavelength wind