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040   $aDip.to Matematica$beng
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084   $aLC TA418.9.P6N54
084   $aAMS 76S05
100 1 $aNield, Donald A.$021339
245 10$aConvection in porous media /$cDonald A. Nield, Adrian Bejan
250   $a2nd ed.
260   $aNew York :$bSpringer,$cc1999
300   $axxi, 546 p. :$bill. ;$c25 cm
504   $aIncludes bibliographical references (p. [453]-537) and index
650  0$aPorous materials$xThermal properties
650  0$aPorous materials$xPermeability
650  0$aHeat$xConvection
650  0$aMass transfer
700 1 $aBejan, Adrian$eauthor$4http://id.loc.gov/vocabulary/relators/aut$09001
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996   $aConvection in porous media$9775783
997   $aUNISALENTO
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101 0 $aeng
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200 10$aMechanics of the solar system $ean introduction to mathematical astronomy /$fJ.A. Evans
210  1$aBath, England :$cBrown Dog Books,$d[2021]
210  4$dİ2021
215   $a1 online resource (270 pages)
330   $aThis book develops methods of computing astronomical phenomena from basic ideas. The position of a celestial body is defined by a vector, with components referred to a system of coordinate axes. The relations between various systems in regular use by astronomers are described. In cases where two systems differ in spatial orientation, they are related by a rotation matrix. These matrices are discussed in considerable detail in the mathematical notes. _x000D_ Other topics discussed include: Kepler's Laws and the dynamics of planetary motion, Precession and Nutation, transits of Venus and Mercury, Lagrange points._x000D_ While no previous knowledge of Astronomy is necessary, it is assumed that the reader is familiar with elementary algebra, trigonometry and calculus.
606   $aAstronomy$xMathematics
615  0$aAstronomy$xMathematics.
676   $a520.151
700   $aEvans$b Jocelyn A.$01524211
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996   $aMechanics of the solar system$93764836
997   $aUNINA