Astrophysical Fluid DynamicsCambridge University Press, 23 févr. 1996 - 242 pages This textbook is a general introduction to the dynamics of astrophysical fluids for students with a knowledge of basic physics at the undergraduate level. No previous knowledge of fluid dynamics or astrophysics is required because the author develops all new concepts in context. The first four chapters cover classical fluids, relativistic fluids, photon fluids and plasma fluids, with many cosmic examples being included. The remaining six chapters deal with astrophysical applications: stars, stellar systems, astrophysical plasmas, cosmological applications, and large scale structure of the universe. Astrophysical fluid dynamics is a promising branch of astronomy, with wide applicability. This textbook considers the role of plasma and magnetism in planets, stars, galaxies, the interplanetary, interstellar and intergalactic media, as well as the universe at large. |
Table des matières
III | 1 |
VI | 2 |
VII | 5 |
VIII | 7 |
IX | 8 |
XI | 10 |
XII | 12 |
XIII | 13 |
LXXVIII | 105 |
LXXIX | 107 |
LXXX | 108 |
LXXXI | 114 |
LXXXII | 116 |
LXXXIII | 119 |
LXXXV | 122 |
LXXXVI | 126 |
XV | 14 |
XVI | 15 |
XVII | 20 |
XIX | 23 |
XX | 24 |
XXI | 25 |
XXIII | 27 |
XXIV | 28 |
XXV | 29 |
XXVI | 33 |
XXVII | 35 |
XXIX | 36 |
XXX | 37 |
XXXI | 39 |
XXXII | 40 |
XXXIV | 42 |
XXXV | 44 |
XXXVI | 45 |
XXXVII | 46 |
XXXVIII | 47 |
XXXIX | 50 |
XLI | 51 |
XLII | 52 |
XLIII | 54 |
XLIV | 57 |
XLV | 60 |
XLVI | 61 |
XLVII | 62 |
XLIX | 63 |
L | 64 |
LI | 65 |
LII | 66 |
LIII | 67 |
LIV | 68 |
LV | 73 |
LVI | 74 |
LVII | 75 |
LVIII | 77 |
LXI | 78 |
LXII | 80 |
LXIII | 81 |
LXIV | 82 |
LXVI | 83 |
LXVII | 86 |
LXVIII | 87 |
LXIX | 88 |
LXX | 91 |
LXXI | 92 |
LXXII | 95 |
LXXIII | 97 |
LXXIV | 101 |
LXXVI | 102 |
LXXVII | 104 |
LXXXVII | 128 |
LXXXVIII | 130 |
LXXXIX | 133 |
XC | 134 |
XCI | 135 |
XCII | 136 |
XCIII | 138 |
XCIV | 140 |
XCV | 142 |
XCVI | 144 |
XCVII | 145 |
XCVIII | 146 |
XCIX | 147 |
CII | 149 |
CIII | 151 |
CIV | 155 |
CV | 158 |
CVI | 161 |
CVII | 164 |
CVIII | 170 |
CIX | 172 |
CX | 174 |
CXI | 175 |
CXII | 178 |
CXIII | 179 |
CXIV | 181 |
CXV | 184 |
CXVII | 185 |
CXVIII | 186 |
CXIX | 187 |
CXX | 188 |
CXXI | 189 |
CXXII | 190 |
CXXIII | 192 |
CXXIV | 194 |
CXXVII | 195 |
CXXVIII | 198 |
CXXIX | 200 |
CXXX | 201 |
CXXXI | 204 |
CXXXII | 205 |
CXXXIII | 206 |
CXXXIV | 207 |
CXXXVI | 208 |
CXXXVII | 210 |
CXXXIX | 213 |
CXL | 218 |
CXLI | 220 |
CXLII | 228 |
CXLIII | 229 |
236 | |
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Expressions et termes fréquents
adiabatic approximation assume astrophysical atmosphere B₁ baryonic becomes black body black hole Boltzmann's equation calculated Chapter chromosphere cloud coefficient collapse collision component considered constant continuity equation convective coordinates cosmic fluid cosmological dark matter defined diffusion direction disc distance distribution dr² electrons energy entropy epoch equation of motion field lines fluid dynamic flux force function galactic galaxies gravitational Hubble's law hydrostatic integral isotropic Jeans mass km s¹ luminosity macroscopic magnetic field mean momentum neutrinos Newtonian number density obtain order of magnitude particles peculiar velocity perfect fluid perturbation photons plasma pressure produce quantities radiation radiative radius recombination redshift relativistic rotation scale Schwarzschild sin² solar star stellar subindex surface temperature tensor term thermal thermodynamic equilibrium turbulence Universe V₁ vector Virial theorem viscosity volume element wet observer white dwarf zero др