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Kravens T.E. — Physic of Solar System Plasmas
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Íàçâàíèå: Physic of Solar System PlasmasÀâòîð: Kravens T.E. Àííîòàöèÿ: Physics of Solar System Plasmas provides a comprehensive introduction to the plasma physics and magnetohydrodynamics that are needed to study the solar wind and magnetosphere. The text includes a broad introduction to plasma physics, including important discussions of kinetic theory, single particle motion, magnetohydrodynamics, geomagnetically trapped energetic particles and the physics of magnetic reconnection. This leads into a thorough description of the Sun and the solar wind, and, finally, the author addresses magnetospheric physics. Among the topics covered here are magnetospheric morphology, bow shocks, magnetospheric convection and electrical currents, substorms, ionospheric physics, magnetosphere-ionosphere coupling, auroral physics and the interaction of the solar wind with the planets. Problem sets at the end of each chapter make this a useful text for advanced undergraduate students in astrophysics, geophysics, or atmospheric sciences. Graduate students and researchers will also find it a valuable source of information.
ßçûê: Ðóáðèêà: Ôèçèêà /Ñòàòóñ ïðåäìåòíîãî óêàçàòåëÿ: Ãîòîâ óêàçàòåëü ñ íîìåðàìè ñòðàíèö ed2k: ed2k stats Ãîä èçäàíèÿ: 1997Êîëè÷åñòâî ñòðàíèö: 477Äîáàâëåíà â êàòàëîã: 17.03.2008Îïåðàöèè: Ïîëîæèòü íà ïîëêó |
Ñêîïèðîâàòü ññûëêó äëÿ ôîðóìà | Ñêîïèðîâàòü ID
Ïðåäìåòíûé óêàçàòåëü
MHD, stability 116—118 MHD, static balance 110—118 MHD, Waves 123—135 Momentum equation 22—36 40 91 110 320 Momentum equation, collision term for 26—29 40—41 Momentum equation, Jupiter, for 444 Momentum equation, mass-loading term, for 25 319—320 Momentum equation, MHD version of 121 370 375—378 Momentum equation, plasmasheet, for 408 Momentum equation, rotating reference frame, for 444 Momentum equation, single-fluid version of 102 Momentum equation, solar corona, for 211—212 Momentum equation, static equilibrium version 110 Momentum equation, two-fluid version of 91 Motional electric field 99 316 350 466 Neutral atmosphere see "Atmosphere" "Thermosphere" Neutral sheet 144 344 Optical depth 175 290 Parker, E. 5 225 Particle transport iheory 78—87 255—261 Pederson conductivity 307—309 372 417 446 Phase velocity/speed see "Velocity" Photoionization see "Ionization" Photosphere 3 173 Photosphere, granulation 181 Photosphere, sunspots 181—185 Pick-up ions 316—317 Pitch angle diffusion/scattering 69 80 82—85 255—258 318—319 Pitch angle, definition of 47 Planck's formula 176 Planets, characteristics of 270—272 plasma 1—2 7 9 90—104 Plasma beta 110 212 284 450 Plasma frequency 96—98 180 470 Plasma instabilities 81 Plasma oscillationsAvaves 91—98 Plasma parameter 38—39 Plasma, single-fluid 98—104 Plasma, two-fluid 90—98 Plasmapause 392—396 Plasmapause, outer planets, for 439—440 Plasmasheet 283—284 323 345 Plasmasheet, boundary of 345 Plasmasheet, comets, in 323 Plasmasheet, inner edge of 414—416 Plasmasheet, Jupiter, of 449—452 Plasmasheet, pressure in 408—416 Plasmasheet, properties of 401 Plasmasphere 68 390—396 Plasmasphere, refilling of 396 455 Poisson's equation 35—37 264 Polarization electric field 99—100 Potential, electrostatic 35 467—468 Potential, magnetic scalar 213—220 Potential, magnetic vector 467 Power spectral density 81 Power spectral density, solar wind, for 249 256 Poynting vector 123 382 471 Pressure gradient force 25—26 408 411 451 Pressure tensor 18 451 Pressure, thermal 18 31 73 271 450 Prominences, solar 183 187 Quasi-linear diffusion 78—82 255—258 318 Quasi-neutrality 37 98—100 Radiation bell see "Trapped particle radiation belts" Radiative transfer 174—177 290—291 Rankine — Hugoniot relations 138—140 265 Recombination, electron-ion 178 296—297 300 303 Resistivity, electrical 103—104 see Resonance condition, for wave-particle interaction 81—82 256 317—318 Ring current 71—77 345 Saha equation 177—179 Scale height 111—113 Scale height, neutral 112 286—287 Scale height, plasma 112—113 163 294 337 Schwarzschild condition 167 Sector structure, solar wind 236—238 Shock jump relations see "Rankine — Hugoniot relations" Shock waves, collisionless 332—335 Shock waves, heliosphere termination 142 Shock waves, how shocks 142 329—332 Shock waves, interplanetary 142 Shock waves, jump conditions for 138—140 Shock waves, oblique 141 Shock waves, parallel and perpendicular 140 332—333 Shock waves, role of 141—143 Single charged particle motion 43—67 Single charged particle motion, dipole magnetic field, in 63—67 Single charged particle motion, electric and magnetic fields, in 48—50 Single charged particle motion, non-uniform magnetic field, in 50—57 Single charged particle motion, uniform magnetic field, in 44—47 Single particle distribution function see "Distribution function" Solar activity and cycle 183 185—188 Solar atmosphere 173—181 Solar atmosphere, corona 179—181 Solar atmosphere, ionization state of 177—179 Solar atmosphere, radiative transfer in 174—177 Solar atmosphere, regions of 173—176 Solar atmosphere, small-scale structure of 181—185 Solar corona see "Corona" Solar flares 186—188 Solar interior 159—173 Solar interior, convection in 166—167 Solar interior, energy transport in 162—165 Solar interior, temperature in 164—165 Solar interior, thermonuclear energy 161—162 Solar oscillations 167—171 Solar spectrum 177 Solar wind 3—5 Solar wind interaction 270—284 Solar wind interaction, comet-type 273 314—327 Solar wind interaction, Earth-type 272 273—290 Solar wind interaction, lunar-type 272 327—329 Solar wind interaction, Venus-type 114—115 272 309—314 Solar wind, composition 229—231 Solar wind, coronal mass ejections in 241 243—246 Solar wind, critical point of flow 205 Solar wind, density 231—234 Solar wind, dynamics of 195—209 Solar wind, electrons 249—252 Solar wind, magnetic field 209—228 Solar wind, shocks 243 Solar wind, speed 194 208 Solar wind, streams 242—243 Solar wind, structure 230—241 Solar wind, temperature 232—234 Solar wind, termination of 252—254 Solar wind, turbulence 246—249 Sound speed 125—128 197 208 Sound waves 124—128 170 Space weather 434—436 Spatial diffusion 69 Spatial diffusion, ambipolar 118—121 157 337 Spatial diffusion, ambipolar in ionospheres 293—294 Spatial diffusion, cross-L shell/radial 85—87 452—453 Spatial diffusion, parallel 257—258 262 Spatial diffusion, perpendicular 257—258 Spitzer conductivity 31 Substorms, magnetospheric, faraday loop model of 422—426 Substorms, magnetospheric, models of 420—422 Substorms, magnetospheric, morphology and phases 418—420 Sunspots 182—185 Tangential discontinuities 137 275 Thermal speed 16 97 Thermospheres 285—289 Thermospheres, diffusive separation in 286—287 Thermospheres, Earth, of 287 Thermospheres, hydrostatic balance in 286—287 Thermospheres, outer planets, of 289 Thermospheres, temperatures in 286—287 Thermospheres, Venus, of 288 Thomson scattering 180 Topside ionosphere 112—113 Transition layer of the Sun 173 Trapped particle radiation belts 7 65—71 345—346 Ultraviolet radiation 173—174 178—179 287 Van Allen belts see "Trapped particle radiation belts" Van allen, james 7 Vector potential, magnetic 467 Velocity/speed, bulk flow 17 101 Velocity/speed, group 93 98 470 Velocity/speed, moments 17—19 Velocity/speed, peculiar/random 23 Velocity/speed, phase 92 98 470 Vlasov equation 13 77—79 Wave equation 125 468 X-ray emission 4 180 185—187 190
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