Solar System DynamicsCambridge University Press, 13/02/2000 The Solar System is a complex and fascinating dynamical system. This is the first textbook to describe comprehensively the dynamical features of the Solar System and to provide students with all the mathematical tools and physical models they need to understand how it works. It is a benchmark publication in the field of planetary dynamics and destined to become a classic. Clearly written and well illustrated, Solar System Dynamics shows how a basic knowledge of the two- and three-body problems and perturbation theory can be combined to understand features as diverse as the tidal heating of Jupiter's moon Io, the origin of the Kirkwood gaps in the asteroid belt, and the radial structure of Saturn's rings. Problems at the end of each chapter and a free Internet Mathematica® software package are provided. Solar System Dynamics provides an authoritative textbook for courses on planetary dynamics and celestial mechanics. It also equips students with the mathematical tools to tackle broader courses on dynamics, dynamical systems, applications of chaos theory and non-linear dynamics. |
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النتائج 1-5 من 14
الصفحة viii
... ring R D(R) set of divisors of the ring R the degree of the polynomial f determinant of the matrix A dimension of the D-vector space V E(R) set of all idempotents in the ring R endomorphism ring of the R-module A (f,g) the ideal ...
... ring R D(R) set of divisors of the ring R the degree of the polynomial f determinant of the matrix A dimension of the D-vector space V E(R) set of all idempotents in the ring R endomorphism ring of the R-module A (f,g) the ideal ...
الصفحة 6
... ring T(R) is Boolean, and in this case, T(R) = R. It is well known that Boolean rings are commutative and reduced with characteristic 2. For a commutative ring R, the set of idempotents of R forms a Boolean algebra, denoted by B(R) ...
... ring T(R) is Boolean, and in this case, T(R) = R. It is well known that Boolean rings are commutative and reduced with characteristic 2. For a commutative ring R, the set of idempotents of R forms a Boolean algebra, denoted by B(R) ...
الصفحة 11
... ring enjoys the structure of a finite field. A two-sided ideal I of a ring is a subset that is closed under addition and by multiplication by any element of the ring. This means that I is also a subring of R. (Closed under ...
... ring enjoys the structure of a finite field. A two-sided ideal I of a ring is a subset that is closed under addition and by multiplication by any element of the ring. This means that I is also a subring of R. (Closed under ...
الصفحة 20
... ring under the laws of composition thus inherited from R. To show that S is a subring it suffices to prove that x , yЄS⇒x - yES and xy ES . If F is a field then a subfield of F is a subring of the ring F which is also a field . Note ...
... ring under the laws of composition thus inherited from R. To show that S is a subring it suffices to prove that x , yЄS⇒x - yES and xy ES . If F is a field then a subfield of F is a subring of the ring F which is also a field . Note ...
الصفحة 49
... ring center figure , made with shuttle thread , and two threads are used for the outside part . For the center make a ring of 4 d.s. , p . , repeat 5 times , close . Make the other 3 rings close to this one , joining by 1st picot , as ...
... ring center figure , made with shuttle thread , and two threads are used for the outside part . For the center make a ring of 4 d.s. , p . , repeat 5 times , close . Make the other 3 rings close to this one , joining by 1st picot , as ...
المحتوى
LXVIII | 261 |
LXIX | 264 |
LXX | 270 |
LXXI | 274 |
LXXII | 279 |
LXXIII | 283 |
LXXIV | 289 |
LXXV | 293 |
19 | |
22 | |
23 | |
25 | |
32 | |
37 | |
42 | |
45 | |
48 | |
XIX | 54 |
XX | 57 |
XXI | 60 |
XXII | 63 |
XXIII | 64 |
XXIV | 68 |
XXV | 71 |
XXVI | 74 |
XXVII | 77 |
XXVIII | 83 |
XXIX | 95 |
XXX | 97 |
XXXI | 102 |
XXXII | 107 |
XXXIII | 110 |
XXXIV | 115 |
XXXV | 121 |
XXXVI | 128 |
XXXVII | 130 |
XXXVIII | 131 |
XXXIX | 136 |
XL | 140 |
XLI | 149 |
XLII | 153 |
XLIII | 155 |
XLIV | 158 |
XLV | 160 |
XLVI | 166 |
XLVII | 174 |
XLVIII | 175 |
XLIX | 178 |
L | 183 |
LI | 186 |
LII | 189 |
LIII | 194 |
LIV | 200 |
LV | 210 |
LVI | 215 |
LVII | 217 |
LVIII | 222 |
LIX | 225 |
LX | 226 |
LXI | 228 |
LXII | 233 |
LXIII | 238 |
LXIV | 246 |
LXV | 248 |
LXVI | 251 |
LXVII | 253 |
LXXVI | 299 |
LXXVII | 302 |
LXXVIII | 307 |
LXXIX | 309 |
LXXX | 314 |
LXXXI | 317 |
LXXXII | 318 |
LXXXIII | 321 |
LXXXIV | 326 |
LXXXV | 328 |
LXXXVI | 332 |
LXXXVII | 334 |
LXXXVIII | 337 |
LXXXIX | 341 |
XC | 364 |
XCI | 371 |
XCII | 373 |
XCIII | 375 |
XCIV | 385 |
XCV | 387 |
XCVI | 390 |
XCVII | 394 |
XCVIII | 396 |
XCIX | 399 |
C | 402 |
CI | 405 |
CII | 406 |
CIII | 409 |
CIV | 410 |
CV | 413 |
CVI | 421 |
CVII | 428 |
CVIII | 448 |
CIX | 452 |
CX | 456 |
CXI | 466 |
CXII | 469 |
CXIII | 471 |
CXIV | 474 |
CXVII | 475 |
CXVIII | 481 |
CXIX | 492 |
CXX | 495 |
CXXI | 512 |
CXXII | 515 |
CXXIII | 518 |
CXXIV | 520 |
CXXV | 522 |
CXXVI | 524 |
CXXVII | 526 |
CXXVIII | 527 |
CXXIX | 529 |
CXXX | 530 |
CXXXI | 535 |
CXXXII | 539 |
CXXXIII | 557 |
CXXXIV | 577 |
طبعات أخرى - عرض جميع المقتطفات
عبارات ومصطلحات مألوفة
amplitude angle angular approach approximate argument associated assume asteroid body calculate centre chaotic circle circular close consider constant corresponding curves defined denote derived determined direction distance disturbing function dynamics Earth eccentricity effect encounter energy equal equations equilibrium points evolution example expansion expression follows force frame function given gives gravitational Hamiltonian Hence inclination increase initial inner integration Jupiter libration longitude mass mean motion moving Note numerical objects observed obtain occur orbit origin outer particle path pericentre period perturbations planet planetary plot position possible potential problem quantities radial radius reference relation resonance respectively ring rotating satellite Saturn Sect secular semi-major axis shown in Fig solar system solution stable surface Table theory tidal tide trajectory values variation vector write