Encyclopedia of Physical Science and Technology, Volume 2Academic Press, 1992 - Physical sciences |
From inside the book
Results 1-3 of 77
Page 46
... method is more natural and transparent to the user . It has become one of the most popular methods in use today . Other methods for knowl- edge representation include ways to describe " objects " and their attributes and relationships ...
... method is more natural and transparent to the user . It has become one of the most popular methods in use today . Other methods for knowl- edge representation include ways to describe " objects " and their attributes and relationships ...
Page 581
... methods are developed by integrating the governing differential equations of the problem with an arbitrary solution ... methods become the only feasible means of ob- taining results . The numerical methods most widely used at present ...
... methods are developed by integrating the governing differential equations of the problem with an arbitrary solution ... methods become the only feasible means of ob- taining results . The numerical methods most widely used at present ...
Page 587
... methods are developed by integrating the governing differential equations of the problem with an arbitrary solution ... methods become the only feasible means of ob- taining results . The numerical methods most widely used at present ...
... methods are developed by integrating the governing differential equations of the problem with an arbitrary solution ... methods become the only feasible means of ob- taining results . The numerical methods most widely used at present ...
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