Coverage for pySDC/implementations/problem_classes/FullSolarSystem.py: 100%

43 statements  

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1import numpy as np 

2 

3from pySDC.implementations.datatype_classes.particles import particles, acceleration 

4from pySDC.implementations.problem_classes.OuterSolarSystem import outer_solar_system 

5 

6 

7# noinspection PyUnusedLocal 

8class full_solar_system(outer_solar_system): 

9 r""" 

10 The :math:`N`-body problem describes the mutual influence of the motion of :math:`N` bodies. Formulation of the problem is 

11 based on Newton's second law. Therefore, the :math:`N`-body problem is formulated as 

12 

13 .. math:: 

14 m_i \frac{d^2 {\bf r}_i}{d t^2} = \sum_{j=1, i\neq j}^N G \frac{m_i m_j}{|{\bf r}_i - {\bf r}_j|^3}({\bf r}_i - {\bf r}_j), 

15 

16 where :math:`m_i` is the :math:`i`-th mass point with position described by the vector :math:`{\bf r}_i`, and :math:`G` 

17 is the gravitational constant. If only the sun influences the motion of the bodies gravitationally, the equations become 

18 

19 .. math:: 

20 m_i \frac{d^2 {\bf r}_i}{d t^2} = G \frac{m_1}{|{\bf r}_i - {\bf r}_1|^3}({\bf r}_i - {\bf r}_1). 

21 

22 This class implements the full solar system containing all planets including Earth's moon, i.e., :math:`N=10`. Initial conditions 

23 are taken from [1]_, and masses relative to the sun taken from [2]_. 

24 

25 Parameters 

26 ---------- 

27 sun_only : bool, optional 

28 If False, only the sun is taken into account for the influence of the motion. 

29 

30 Attributes 

31 ---------- 

32 G : float 

33 Gravitational constant. 

34 

35 References 

36 ---------- 

37 .. [1] https://www.aanda.org/articles/aa/full/2002/08/aa1405/aa1405.right.html 

38 .. [2] https://en.wikipedia.org/wiki/Planetary_mass#Values_from_the_DE405_ephemeris 

39 """ 

40 

41 dtype_u = particles 

42 dtype_f = acceleration 

43 

44 def __init__(self, sun_only=False): 

45 """Initialization routine""" 

46 

47 super().__init__(sun_only) 

48 self.init = ((3, 10), None, np.dtype('float64')) 

49 

50 def u_exact(self, t): 

51 r""" 

52 Routine to compute the exact/initial trajectory at time :math:`t`. Values here are taken from [1]_, [2]_. 

53 

54 Parameters 

55 ---------- 

56 t : float 

57 Time of the exact/initial trajectory. 

58 

59 Returns 

60 ------- 

61 me : dtype_u 

62 Exact/initial position and velocity. 

63 """ 

64 assert t == 0.0, 'error, u_exact only works for the initial time t0=0' 

65 me = self.dtype_u(self.init) 

66 

67 me.pos[:, 0] = [0.0, 0.0, 0.0] 

68 me.pos[:, 1] = [-2.503321047836e-01, +1.873217481656e-01, +1.260230112145e-01] 

69 me.pos[:, 2] = [+1.747780055994e-02, -6.624210296743e-01, -2.991203277122e-01] 

70 me.pos[:, 3] = [-9.091916173950e-01, +3.592925969244e-01, +1.557729610506e-01] 

71 me.pos[:, 4] = [+1.203018828754e00, +7.270712989688e-01, +3.009561427569e-01] 

72 me.pos[:, 5] = [+3.733076999471e00, +3.052424824299e00, +1.217426663570e00] 

73 me.pos[:, 6] = [+6.164433062913e00, +6.366775402981e00, +2.364531109847e00] 

74 me.pos[:, 7] = [+1.457964661868e01, -1.236891078519e01, -5.623617280033e00] 

75 me.pos[:, 8] = [+1.695491139909e01, -2.288713988623e01, -9.789921035251e00] 

76 me.pos[:, 9] = [-9.707098450131e00, -2.804098175319e01, -5.823808919246e00] 

77 

78 me.vel[:, 0] = [0.0, 0.0, 0.0] 

79 me.vel[:, 1] = [-2.438808424736e-02, -1.850224608274e-02, -7.353811537540e-03] 

80 me.vel[:, 2] = [+2.008547034175e-02, +8.365454832702e-04, -8.947888514893e-04] 

81 me.vel[:, 3] = [-7.085843239142e-03, -1.455634327653e-02, -6.310912842359e-03] 

82 me.vel[:, 4] = [-7.124453943885e-03, +1.166307407692e-02, +5.542098698449e-03] 

83 me.vel[:, 5] = [-5.086540617947e-03, +5.493643783389e-03, +2.478685100749e-03] 

84 me.vel[:, 6] = [-4.426823593779e-03, +3.394060157503e-03, +1.592261423092e-03] 

85 me.vel[:, 7] = [+2.647505630327e-03, +2.487457379099e-03, +1.052000252243e-03] 

86 me.vel[:, 8] = [+2.568651772461e-03, +1.681832388267e-03, +6.245613982833e-04] 

87 me.vel[:, 9] = [+3.034112963576e-03, -1.111317562971e-03, -1.261841468083e-03] 

88 

89 me.m[0] = 1.0 # Sun 

90 me.m[1] = 0.1660100 * 1e-06 # Mercury 

91 me.m[2] = 2.4478383 * 1e-06 # Venus 

92 me.m[3] = 3.0404326 * 1e-06 # Earth+Moon 

93 me.m[4] = 0.3227151 * 1e-06 # Mars 

94 me.m[5] = 954.79194 * 1e-06 # Jupiter 

95 me.m[6] = 285.88600 * 1e-06 # Saturn 

96 me.m[7] = 43.662440 * 1e-06 # Uranus 

97 me.m[8] = 51.513890 * 1e-06 # Neptune 

98 me.m[9] = 0.0073960 * 1e-06 # Pluto 

99 

100 return me