Encyclopedia of Physical Science and Technology, Volume 2Academic Press, 1992 - Physical sciences |
From inside the book
Results 1-3 of 83
Page 172
... relative to hydrogen , than expected on the basis of relative elemental abundances in the sun and stars . It was conjectured that this " depletion " was the result of dust grain formation . Regions of the interstellar medium containing ...
... relative to hydrogen , than expected on the basis of relative elemental abundances in the sun and stars . It was conjectured that this " depletion " was the result of dust grain formation . Regions of the interstellar medium containing ...
Page 371
... relative widths of the atomic absorption profile ( half - width typically 0.005 nm ) and the HCL emission profile ( typically 0.002 nm ) . ( b ) x , the normal calibration curve obtained for AAS ; y , a change in slope and linear ...
... relative widths of the atomic absorption profile ( half - width typically 0.005 nm ) and the HCL emission profile ( typically 0.002 nm ) . ( b ) x , the normal calibration curve obtained for AAS ; y , a change in slope and linear ...
Page 760
... relative to a standard material . Asym- metry in the electric field surrounding the nu- cleus produces splitting of the energy levels . Ad- ditional splitting results from a permanent magnetic field surrounding the nucleus . The ...
... relative to a standard material . Asym- metry in the electric field surrounding the nu- cleus produces splitting of the energy levels . Ad- ditional splitting results from a permanent magnetic field surrounding the nucleus . The ...
Contents
Guide to Using the Encyclopedia ix Atomic Physics | 339 |
Approximations and Expansions 1 Atomic Spectrometry | 357 |
Archaeological Geology 31 Atomic Spectroscopy | 381 |
Copyright | |
17 other sections not shown
Other editions - View all
Common terms and phrases
absorption acid aldoses angular momentum approximation asbestos atmosphere atoms auroral BASIC battery black hole Boolean algebra carbon fibers catalyst cell chemical chrysotile clouds collision complex components concentration convection cross section curve density developed disaccharide disk distribution dust electron elements emission emitted energy engine equations example expert system flux function galaxies heat hydrogen hydroxyl groups infrared input interaction interstellar interstellar medium ionization ions mass material measurements mechanism ment metal molecular molecules monosaccharides neutron stars nucleophile observed oligosaccharides operator orbital oxidation oxygen parameter particles photons plume problem radiation reaction reactor region result saccharide solar solution space spectral spectroscopy spectrum speed spline stable stars stellar structure surface techniques telescope temperature Theorem thermal tion tive turbulence ture typical variable velocity vertical wave wavelength weight white dwarf wind