Encyclopedia of Physical Science and Technology, Volume 2Academic Press, 1992 - Physical sciences |
From inside the book
Results 1-3 of 80
Page 518
... effect . It is most noticeable in eclipsing sys- tems because these present the largest path length through material in the orbital plane . In some cases , atmospheric eclipses can also dis- tort the lines because of stellar winds and ...
... effect . It is most noticeable in eclipsing sys- tems because these present the largest path length through material in the orbital plane . In some cases , atmospheric eclipses can also dis- tort the lines because of stellar winds and ...
Page 561
... effect , called light bending , was one of the first predictions of general rela- tivity to be confirmed by solar system measure- ments . Near a black hole the gravitational field is so strong that photons can be put into circular ...
... effect , called light bending , was one of the first predictions of general rela- tivity to be confirmed by solar system measure- ments . Near a black hole the gravitational field is so strong that photons can be put into circular ...
Page 760
... effect of the chemisorption of NH3 on the 57Fe resonance of a highly dispersed Fe / SiO2 catalyst . The iron is in the ferrous state following the hydrogen reduc- tion of microcrystalline ferric oxide deposits . The addition of NH3 to ...
... effect of the chemisorption of NH3 on the 57Fe resonance of a highly dispersed Fe / SiO2 catalyst . The iron is in the ferrous state following the hydrogen reduc- tion of microcrystalline ferric oxide deposits . The addition of NH3 to ...
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