def get_equations(m_val, g_val, l_val):
# This function body is copyied from:
# http://www.pydy.org/examples/double_pendulum.html
# Retrieved 2015-09-29
from sympy import symbols
from sympy.physics.mechanics import (dynamicsymbols, ReferenceFrame, Point,
Particle, KanesMethod)
q1, q2 = dynamicsymbols('q1 q2')
q1d, q2d = dynamicsymbols('q1 q2', 1)
u1, u2 = dynamicsymbols('u1 u2')
u1d, u2d = dynamicsymbols('u1 u2', 1)
l, m, g = symbols('l m g')
N = ReferenceFrame('N')
A = N.orientnew('A', 'Axis', [q1, N.z])
B = N.orientnew('B', 'Axis', [q2, N.z])
A.set_ang_vel(N, u1 * N.z)
B.set_ang_vel(N, u2 * N.z)
O = Point('O')
P = O.locatenew('P', l * A.x)
R = P.locatenew('R', l * B.x)
O.set_vel(N, 0)
P.v2pt_theory(O, N, A)
R.v2pt_theory(P, N, B)
ParP = Particle('ParP', P, m)
ParR = Particle('ParR', R, m)
kd = [q1d - u1, q2d - u2]
FL = [(P, m * g * N.x), (R, m * g * N.x)]
BL = [ParP, ParR]
KM = KanesMethod(N, q_ind=[q1, q2], u_ind=[u1, u2], kd_eqs=kd)
try:
(fr, frstar) = KM.kanes_equations(bodies=BL, loads=FL)
except TypeError:
(fr, frstar) = KM.kanes_equations(FL, BL)
kdd = KM.kindiffdict()
mm = KM.mass_matrix_full
fo = KM.forcing_full
qudots = mm.inv() * fo
qudots = qudots.subs(kdd)
qudots.simplify()
# Edit:
depv = [q1, q2, u1, u2]
subs = list(zip([m, g, l], [m_val, g_val, l_val]))
return zip(depv, [expr.subs(subs) for expr in qudots])
def get_equations(m_val, g_val, l_val):
# This function body is copyied from:
# http://www.pydy.org/examples/double_pendulum.html
# Retrieved 2015-09-29
from sympy import symbols
from sympy.physics.mechanics import (
dynamicsymbols, ReferenceFrame, Point, Particle, KanesMethod
)
q1, q2 = dynamicsymbols('q1 q2')
q1d, q2d = dynamicsymbols('q1 q2', 1)
u1, u2 = dynamicsymbols('u1 u2')
u1d, u2d = dynamicsymbols('u1 u2', 1)
l, m, g = symbols('l m g')
N = ReferenceFrame('N')
A = N.orientnew('A', 'Axis', [q1, N.z])
B = N.orientnew('B', 'Axis', [q2, N.z])
A.set_ang_vel(N, u1 * N.z)
B.set_ang_vel(N, u2 * N.z)
O = Point('O')
P = O.locatenew('P', l * A.x)
R = P.locatenew('R', l * B.x)
O.set_vel(N, 0)
P.v2pt_theory(O, N, A)
R.v2pt_theory(P, N, B)
ParP = Particle('ParP', P, m)
ParR = Particle('ParR', R, m)
kd = [q1d - u1, q2d - u2]
FL = [(P, m * g * N.x), (R, m * g * N.x)]
BL = [ParP, ParR]
KM = KanesMethod(N, q_ind=[q1, q2], u_ind=[u1, u2], kd_eqs=kd)
(fr, frstar) = KM.kanes_equations(FL, BL)
kdd = KM.kindiffdict()
mm = KM.mass_matrix_full
fo = KM.forcing_full
qudots = mm.inv() * fo
qudots = qudots.subs(kdd)
qudots.simplify()
# Edit:
depv = [q1, q2, u1, u2]
subs = list(zip([m, g, l], [m_val, g_val, l_val]))
return zip(depv, [expr.subs(subs) for expr in qudots])
def second_order_system():
# from sympy.printing.pycode import NumPyPrinter, pycode
coordinates = dynamicsymbols('q:1') # Generalized coordinates
speeds = dynamicsymbols('u:1') # Generalized speeds
# Force applied to the cart
cart_thrust = dynamicsymbols('thrust')
m = sp.symbols('m:1') # Mass of each bob
g, t = sp.symbols('g t')
# Gravity and time
ref_frame = ReferenceFrame('I') # Inertial reference frame
origin = Point('O') # Origin point
origin.set_vel(ref_frame, 0) # Origin's velocity is zero
P0 = Point('P0') # Hinge point of top link
# Set the position of P0
P0.set_pos(origin, coordinates[0] * ref_frame.x)
P0.set_vel(ref_frame, speeds[0] * ref_frame.x) # Set the velocity of P0
Pa0 = Particle('Pa0', P0, m[0]) # Define a particle at P0
# List to hold the n + 1 frames
frames = [ref_frame]
points = [P0] # List to hold the n + 1 points
# List to hold the n + 1 particles
particles = [Pa0]
# List to hold the n + 1 applied forces, including the input force, f
applied_forces = [(P0, cart_thrust * ref_frame.x - m[0] * g *
ref_frame.y)]
# List to hold kinematic ODE's
kindiffs = [coordinates[0].diff(t) - speeds[0]]
# Initialize the object
kane = KanesMethod(ref_frame, q_ind=coordinates,
u_ind=speeds, kd_eqs=kindiffs)
# Generate EoM's fr + frstar = 0
fr, frstar = kane.kanes_equations(particles, applied_forces)
state = coordinates + speeds
gain = [cart_thrust]
kindiff_dict = kane.kindiffdict()
M = kane.mass_matrix_full.subs(kindiff_dict)
F = kane.forcing_full.subs(kindiff_dict)
static_parameters = [g, m[0]]
transfer = M.inv() * F
return DynamicSystem(state, gain, static_parameters, transfer)
def test_rolling_disc():
# Rolling Disc Example
# Here the rolling disc is formed from the contact point up, removing the
# need to introduce generalized speeds. Only 3 configuration and three
# speed variables are need to describe this system, along with the disc's
# mass and radius, and the local gravity (note that mass will drop out).
q1, q2, q3, u1, u2, u3 = dynamicsymbols('q1 q2 q3 u1 u2 u3')
q1d, q2d, q3d, u1d, u2d, u3d = dynamicsymbols('q1 q2 q3 u1 u2 u3', 1)
r, m, g = symbols('r m g')
# The kinematics are formed by a series of simple rotations. Each simple
# rotation creates a new frame, and the next rotation is defined by the new
# frame's basis vectors. This example uses a 3-1-2 series of rotations, or
# Z, X, Y series of rotations. Angular velocity for this is defined using
# the second frame's basis (the lean frame).
N = ReferenceFrame('N')
Y = N.orientnew('Y', 'Axis', [q1, N.z])
L = Y.orientnew('L', 'Axis', [q2, Y.x])
R = L.orientnew('R', 'Axis', [q3, L.y])
w_R_N_qd = R.ang_vel_in(N)
R.set_ang_vel(N, u1 * L.x + u2 * L.y + u3 * L.z)
# This is the translational kinematics. We create a point with no velocity
# in N; this is the contact point between the disc and ground. Next we form
# the position vector from the contact point to the disc's center of mass.
# Finally we form the velocity and acceleration of the disc.
C = Point('C')
C.set_vel(N, 0)
Dmc = C.locatenew('Dmc', r * L.z)
Dmc.v2pt_theory(C, N, R)
# This is a simple way to form the inertia dyadic.
I = inertia(L, m / 4 * r**2, m / 2 * r**2, m / 4 * r**2)
# Kinematic differential equations; how the generalized coordinate time
# derivatives relate to generalized speeds.
kd = [dot(R.ang_vel_in(N) - w_R_N_qd, uv) for uv in L]
# Creation of the force list; it is the gravitational force at the mass
# center of the disc. Then we create the disc by assigning a Point to the
# center of mass attribute, a ReferenceFrame to the frame attribute, and mass
# and inertia. Then we form the body list.
ForceList = [(Dmc, - m * g * Y.z)]
BodyD = RigidBody('BodyD', Dmc, R, m, (I, Dmc))
BodyList = [BodyD]
# Finally we form the equations of motion, using the same steps we did
# before. Specify inertial frame, supply generalized speeds, supply
# kinematic differential equation dictionary, compute Fr from the force
# list and Fr* from the body list, compute the mass matrix and forcing
# terms, then solve for the u dots (time derivatives of the generalized
# speeds).
KM = KanesMethod(N, q_ind=[q1, q2, q3], u_ind=[u1, u2, u3], kd_eqs=kd)
KM.kanes_equations(ForceList, BodyList)
MM = KM.mass_matrix
forcing = KM.forcing
rhs = MM.inv() * forcing
kdd = KM.kindiffdict()
rhs = rhs.subs(kdd)
rhs.simplify()
assert rhs.expand() == Matrix([(6*u2*u3*r - u3**2*r*tan(q2) +
4*g*sin(q2))/(5*r), -2*u1*u3/3, u1*(-2*u2 + u3*tan(q2))]).expand()
# This code tests our output vs. benchmark values. When r=g=m=1, the
# critical speed (where all eigenvalues of the linearized equations are 0)
# is 1 / sqrt(3) for the upright case.
A = KM.linearize(A_and_B=True, new_method=True)[0]
A_upright = A.subs({r: 1, g: 1, m: 1}).subs({q1: 0, q2: 0, q3: 0, u1: 0, u3: 0})
assert A_upright.subs(u2, 1 / sqrt(3)).eigenvals() == {S(0): 6}
def test_aux_dep():
# This test is about rolling disc dynamics, comparing the results found
# with KanesMethod to those found when deriving the equations "manually"
# with SymPy.
# The terms Fr, Fr*, and Fr*_steady are all compared between the two
# methods. Here, Fr*_steady refers to the generalized inertia forces for an
# equilibrium configuration.
# Note: comparing to the test of test_rolling_disc() in test_kane.py, this
# test also tests auxiliary speeds and configuration and motion constraints
#, seen in the generalized dependent coordinates q[3], and depend speeds
# u[3], u[4] and u[5].
# First, mannual derivation of Fr, Fr_star, Fr_star_steady.
# Symbols for time and constant parameters.
# Symbols for contact forces: Fx, Fy, Fz.
t, r, m, g, I, J = symbols('t r m g I J')
Fx, Fy, Fz = symbols('Fx Fy Fz')
# Configuration variables and their time derivatives:
# q[0] -- yaw
# q[1] -- lean
# q[2] -- spin
# q[3] -- dot(-r*B.z, A.z) -- distance from ground plane to disc center in
# A.z direction
# Generalized speeds and their time derivatives:
# u[0] -- disc angular velocity component, disc fixed x direction
# u[1] -- disc angular velocity component, disc fixed y direction
# u[2] -- disc angular velocity component, disc fixed z direction
# u[3] -- disc velocity component, A.x direction
# u[4] -- disc velocity component, A.y direction
# u[5] -- disc velocity component, A.z direction
# Auxiliary generalized speeds:
# ua[0] -- contact point auxiliary generalized speed, A.x direction
# ua[1] -- contact point auxiliary generalized speed, A.y direction
# ua[2] -- contact point auxiliary generalized speed, A.z direction
q = dynamicsymbols('q:4')
qd = [qi.diff(t) for qi in q]
u = dynamicsymbols('u:6')
ud = [ui.diff(t) for ui in u]
#ud_zero = {udi : 0 for udi in ud}
ud_zero = dict(zip(ud, [0.]*len(ud)))
ua = dynamicsymbols('ua:3')
#ua_zero = {uai : 0 for uai in ua}
ua_zero = dict(zip(ua, [0.]*len(ua)))
# Reference frames:
# Yaw intermediate frame: A.
# Lean intermediate frame: B.
# Disc fixed frame: C.
N = ReferenceFrame('N')
A = N.orientnew('A', 'Axis', [q[0], N.z])
B = A.orientnew('B', 'Axis', [q[1], A.x])
C = B.orientnew('C', 'Axis', [q[2], B.y])
# Angular velocity and angular acceleration of disc fixed frame
# u[0], u[1] and u[2] are generalized independent speeds.
C.set_ang_vel(N, u[0]*B.x + u[1]*B.y + u[2]*B.z)
C.set_ang_acc(N, C.ang_vel_in(N).diff(t, B)
+ cross(B.ang_vel_in(N), C.ang_vel_in(N)))
# Velocity and acceleration of points:
# Disc-ground contact point: P.
# Center of disc: O, defined from point P with depend coordinate: q[3]
# u[3], u[4] and u[5] are generalized dependent speeds.
P = Point('P')
P.set_vel(N, ua[0]*A.x + ua[1]*A.y + ua[2]*A.z)
O = P.locatenew('O', q[3]*A.z + r*sin(q[1])*A.y)
O.set_vel(N, u[3]*A.x + u[4]*A.y + u[5]*A.z)
O.set_acc(N, O.vel(N).diff(t, A) + cross(A.ang_vel_in(N), O.vel(N)))
# Kinematic differential equations:
# Two equalities: one is w_c_n_qd = C.ang_vel_in(N) in three coordinates
# directions of B, for qd0, qd1 and qd2.
# the other is v_o_n_qd = O.vel(N) in A.z direction for qd3.
# Then, solve for dq/dt's in terms of u's: qd_kd.
w_c_n_qd = qd[0]*A.z + qd[1]*B.x + qd[2]*B.y
v_o_n_qd = O.pos_from(P).diff(t, A) + cross(A.ang_vel_in(N), O.pos_from(P))
kindiffs = Matrix([dot(w_c_n_qd - C.ang_vel_in(N), uv) for uv in B] +
[dot(v_o_n_qd - O.vel(N), A.z)])
qd_kd = solve(kindiffs, qd)
# Values of generalized speeds during a steady turn for later substitution
# into the Fr_star_steady.
steady_conditions = solve(kindiffs.subs({qd[1] : 0, qd[3] : 0}), u)
steady_conditions.update({qd[1] : 0, qd[3] : 0})
# Partial angular velocities and velocities.
partial_w_C = [C.ang_vel_in(N).diff(ui, N) for ui in u + ua]
partial_v_O = [O.vel(N).diff(ui, N) for ui in u + ua]
partial_v_P = [P.vel(N).diff(ui, N) for ui in u + ua]
# Configuration constraint: f_c, the projection of radius r in A.z direction
# is q[3].
# Velocity constraints: f_v, for u3, u4 and u5.
# Acceleration constraints: f_a.
f_c = Matrix([dot(-r*B.z, A.z) - q[3]])
f_v = Matrix([dot(O.vel(N) - (P.vel(N) + cross(C.ang_vel_in(N),
O.pos_from(P))), ai).expand() for ai in A])
v_o_n = cross(C.ang_vel_in(N), O.pos_from(P))
a_o_n = v_o_n.diff(t, A) + cross(A.ang_vel_in(N), v_o_n)
f_a = Matrix([dot(O.acc(N) - a_o_n, ai) for ai in A])
# Solve for constraint equations in the form of
# u_dependent = A_rs * [u_i; u_aux].
# First, obtain constraint coefficient matrix: M_v * [u; ua] = 0;
# Second, taking u[0], u[1], u[2] as independent,
# taking u[3], u[4], u[5] as dependent,
# rearranging the matrix of M_v to be A_rs for u_dependent.
# Third, u_aux ==0 for u_dep, and resulting dictionary of u_dep_dict.
M_v = zeros(3, 9)
for i in range(3):
for j, ui in enumerate(u + ua):
M_v[i, j] = f_v[i].diff(ui)
M_v_i = M_v[:, :3]
M_v_d = M_v[:, 3:6]
M_v_aux = M_v[:, 6:]
M_v_i_aux = M_v_i.row_join(M_v_aux)
A_rs = - M_v_d.inv() * M_v_i_aux
u_dep = A_rs[:, :3] * Matrix(u[:3])
u_dep_dict = dict(zip(u[3:], u_dep))
#u_dep_dict = {udi : u_depi[0] for udi, u_depi in zip(u[3:], u_dep.tolist())}
# Active forces: F_O acting on point O; F_P acting on point P.
# Generalized active forces (unconstrained): Fr_u = F_point * pv_point.
F_O = m*g*A.z
F_P = Fx * A.x + Fy * A.y + Fz * A.z
Fr_u = Matrix([dot(F_O, pv_o) + dot(F_P, pv_p) for pv_o, pv_p in
zip(partial_v_O, partial_v_P)])
# Inertia force: R_star_O.
# Inertia of disc: I_C_O, where J is a inertia component about principal axis.
# Inertia torque: T_star_C.
# Generalized inertia forces (unconstrained): Fr_star_u.
R_star_O = -m*O.acc(N)
I_C_O = inertia(B, I, J, I)
T_star_C = -(dot(I_C_O, C.ang_acc_in(N)) \
+ cross(C.ang_vel_in(N), dot(I_C_O, C.ang_vel_in(N))))
Fr_star_u = Matrix([dot(R_star_O, pv) + dot(T_star_C, pav) for pv, pav in
zip(partial_v_O, partial_w_C)])
# Form nonholonomic Fr: Fr_c, and nonholonomic Fr_star: Fr_star_c.
# Also, nonholonomic Fr_star in steady turning condition: Fr_star_steady.
Fr_c = Fr_u[:3, :].col_join(Fr_u[6:, :]) + A_rs.T * Fr_u[3:6, :]
Fr_star_c = Fr_star_u[:3, :].col_join(Fr_star_u[6:, :])\
+ A_rs.T * Fr_star_u[3:6, :]
Fr_star_steady = Fr_star_c.subs(ud_zero).subs(u_dep_dict)\
.subs(steady_conditions).subs({q[3]: -r*cos(q[1])}).expand()
# Second, using KaneMethod in mechanics for fr, frstar and frstar_steady.
# Rigid Bodies: disc, with inertia I_C_O.
iner_tuple = (I_C_O, O)
disc = RigidBody('disc', O, C, m, iner_tuple)
bodyList = [disc]
# Generalized forces: Gravity: F_o; Auxiliary forces: F_p.
F_o = (O, F_O)
F_p = (P, F_P)
forceList = [F_o, F_p]
# KanesMethod.
kane = KanesMethod(
N, q_ind= q[:3], u_ind= u[:3], kd_eqs=kindiffs,
q_dependent=q[3:], configuration_constraints = f_c,
u_dependent=u[3:], velocity_constraints= f_v,
u_auxiliary=ua
)
# fr, frstar, frstar_steady and kdd(kinematic differential equations).
(fr, frstar)= kane.kanes_equations(forceList, bodyList)
frstar_steady = frstar.subs(ud_zero).subs(u_dep_dict).subs(steady_conditions)\
.subs({q[3]: -r*cos(q[1])}).expand()
kdd = kane.kindiffdict()
# Test
# First try Fr_c == fr;
# Second try Fr_star_c == frstar;
# Third try Fr_star_steady == frstar_steady.
# Both signs are checked in case the equations were found with an inverse
# sign.
assert ((Matrix(Fr_c).expand() == fr.expand()) or
(Matrix(Fr_c).expand() == (-fr).expand()))
assert ((Matrix(Fr_star_c).expand() == frstar.expand()) or
(Matrix(Fr_star_c).expand() == (-frstar).expand()))
assert ((Matrix(Fr_star_steady).expand() == frstar_steady.expand()) or
(Matrix(Fr_star_steady).expand() == (-frstar_steady).expand()))
def test_bicycle():
if ON_TRAVIS:
skip("Too slow for travis.")
# Code to get equations of motion for a bicycle modeled as in:
# J.P Meijaard, Jim M Papadopoulos, Andy Ruina and A.L Schwab. Linearized
# dynamics equations for the balance and steer of a bicycle: a benchmark
# and review. Proceedings of The Royal Society (2007) 463, 1955-1982
# doi: 10.1098/rspa.2007.1857
# Note that this code has been crudely ported from Autolev, which is the
# reason for some of the unusual naming conventions. It was purposefully as
# similar as possible in order to aide debugging.
# Declare Coordinates & Speeds
# Simple definitions for qdots - qd = u
# Speeds are: yaw frame ang. rate, roll frame ang. rate, rear wheel frame
# ang. rate (spinning motion), frame ang. rate (pitching motion), steering
# frame ang. rate, and front wheel ang. rate (spinning motion).
# Wheel positions are ignorable coordinates, so they are not introduced.
q1, q2, q4, q5 = dynamicsymbols('q1 q2 q4 q5')
q1d, q2d, q4d, q5d = dynamicsymbols('q1 q2 q4 q5', 1)
u1, u2, u3, u4, u5, u6 = dynamicsymbols('u1 u2 u3 u4 u5 u6')
u1d, u2d, u3d, u4d, u5d, u6d = dynamicsymbols('u1 u2 u3 u4 u5 u6', 1)
# Declare System's Parameters
WFrad, WRrad, htangle, forkoffset = symbols(
'WFrad WRrad htangle forkoffset')
forklength, framelength, forkcg1 = symbols(
'forklength framelength forkcg1')
forkcg3, framecg1, framecg3, Iwr11 = symbols(
'forkcg3 framecg1 framecg3 Iwr11')
Iwr22, Iwf11, Iwf22, Iframe11 = symbols('Iwr22 Iwf11 Iwf22 Iframe11')
Iframe22, Iframe33, Iframe31, Ifork11 = symbols(
'Iframe22 Iframe33 Iframe31 Ifork11')
Ifork22, Ifork33, Ifork31, g = symbols('Ifork22 Ifork33 Ifork31 g')
mframe, mfork, mwf, mwr = symbols('mframe mfork mwf mwr')
# Set up reference frames for the system
# N - inertial
# Y - yaw
# R - roll
# WR - rear wheel, rotation angle is ignorable coordinate so not oriented
# Frame - bicycle frame
# TempFrame - statically rotated frame for easier reference inertia definition
# Fork - bicycle fork
# TempFork - statically rotated frame for easier reference inertia definition
# WF - front wheel, again posses a ignorable coordinate
N = ReferenceFrame('N')
Y = N.orientnew('Y', 'Axis', [q1, N.z])
R = Y.orientnew('R', 'Axis', [q2, Y.x])
Frame = R.orientnew('Frame', 'Axis', [q4 + htangle, R.y])
WR = ReferenceFrame('WR')
TempFrame = Frame.orientnew('TempFrame', 'Axis', [-htangle, Frame.y])
Fork = Frame.orientnew('Fork', 'Axis', [q5, Frame.x])
TempFork = Fork.orientnew('TempFork', 'Axis', [-htangle, Fork.y])
WF = ReferenceFrame('WF')
# Kinematics of the Bicycle First block of code is forming the positions of
# the relevant points
# rear wheel contact -> rear wheel mass center -> frame mass center +
# frame/fork connection -> fork mass center + front wheel mass center ->
# front wheel contact point
WR_cont = Point('WR_cont')
WR_mc = WR_cont.locatenew('WR_mc', WRrad * R.z)
Steer = WR_mc.locatenew('Steer', framelength * Frame.z)
Frame_mc = WR_mc.locatenew('Frame_mc',
-framecg1 * Frame.x + framecg3 * Frame.z)
Fork_mc = Steer.locatenew('Fork_mc', -forkcg1 * Fork.x + forkcg3 * Fork.z)
WF_mc = Steer.locatenew('WF_mc', forklength * Fork.x + forkoffset * Fork.z)
WF_cont = WF_mc.locatenew(
'WF_cont',
WFrad * (dot(Fork.y, Y.z) * Fork.y - Y.z).normalize())
# Set the angular velocity of each frame.
# Angular accelerations end up being calculated automatically by
# differentiating the angular velocities when first needed.
# u1 is yaw rate
# u2 is roll rate
# u3 is rear wheel rate
# u4 is frame pitch rate
# u5 is fork steer rate
# u6 is front wheel rate
Y.set_ang_vel(N, u1 * Y.z)
R.set_ang_vel(Y, u2 * R.x)
WR.set_ang_vel(Frame, u3 * Frame.y)
Frame.set_ang_vel(R, u4 * Frame.y)
Fork.set_ang_vel(Frame, u5 * Fork.x)
WF.set_ang_vel(Fork, u6 * Fork.y)
# Form the velocities of the previously defined points, using the 2 - point
# theorem (written out by hand here). Accelerations again are calculated
# automatically when first needed.
WR_cont.set_vel(N, 0)
WR_mc.v2pt_theory(WR_cont, N, WR)
Steer.v2pt_theory(WR_mc, N, Frame)
Frame_mc.v2pt_theory(WR_mc, N, Frame)
Fork_mc.v2pt_theory(Steer, N, Fork)
WF_mc.v2pt_theory(Steer, N, Fork)
WF_cont.v2pt_theory(WF_mc, N, WF)
# Sets the inertias of each body. Uses the inertia frame to construct the
# inertia dyadics. Wheel inertias are only defined by principle moments of
# inertia, and are in fact constant in the frame and fork reference frames;
# it is for this reason that the orientations of the wheels does not need
# to be defined. The frame and fork inertias are defined in the 'Temp'
# frames which are fixed to the appropriate body frames; this is to allow
# easier input of the reference values of the benchmark paper. Note that
# due to slightly different orientations, the products of inertia need to
# have their signs flipped; this is done later when entering the numerical
# value.
Frame_I = (inertia(TempFrame, Iframe11, Iframe22, Iframe33, 0, 0,
Iframe31), Frame_mc)
Fork_I = (inertia(TempFork, Ifork11, Ifork22, Ifork33, 0, 0,
Ifork31), Fork_mc)
WR_I = (inertia(Frame, Iwr11, Iwr22, Iwr11), WR_mc)
WF_I = (inertia(Fork, Iwf11, Iwf22, Iwf11), WF_mc)
# Declaration of the RigidBody containers. ::
BodyFrame = RigidBody('BodyFrame', Frame_mc, Frame, mframe, Frame_I)
BodyFork = RigidBody('BodyFork', Fork_mc, Fork, mfork, Fork_I)
BodyWR = RigidBody('BodyWR', WR_mc, WR, mwr, WR_I)
BodyWF = RigidBody('BodyWF', WF_mc, WF, mwf, WF_I)
# The kinematic differential equations; they are defined quite simply. Each
# entry in this list is equal to zero.
kd = [q1d - u1, q2d - u2, q4d - u4, q5d - u5]
# The nonholonomic constraints are the velocity of the front wheel contact
# point dotted into the X, Y, and Z directions; the yaw frame is used as it
# is "closer" to the front wheel (1 less DCM connecting them). These
# constraints force the velocity of the front wheel contact point to be 0
# in the inertial frame; the X and Y direction constraints enforce a
# "no-slip" condition, and the Z direction constraint forces the front
# wheel contact point to not move away from the ground frame, essentially
# replicating the holonomic constraint which does not allow the frame pitch
# to change in an invalid fashion.
conlist_speed = [
WF_cont.vel(N) & Y.x,
WF_cont.vel(N) & Y.y,
WF_cont.vel(N) & Y.z
]
# The holonomic constraint is that the position from the rear wheel contact
# point to the front wheel contact point when dotted into the
# normal-to-ground plane direction must be zero; effectively that the front
# and rear wheel contact points are always touching the ground plane. This
# is actually not part of the dynamic equations, but instead is necessary
# for the lineraization process.
conlist_coord = [WF_cont.pos_from(WR_cont) & Y.z]
# The force list; each body has the appropriate gravitational force applied
# at its mass center.
FL = [(Frame_mc, -mframe * g * Y.z), (Fork_mc, -mfork * g * Y.z),
(WF_mc, -mwf * g * Y.z), (WR_mc, -mwr * g * Y.z)]
BL = [BodyFrame, BodyFork, BodyWR, BodyWF]
# The N frame is the inertial frame, coordinates are supplied in the order
# of independent, dependent coordinates, as are the speeds. The kinematic
# differential equation are also entered here. Here the dependent speeds
# are specified, in the same order they were provided in earlier, along
# with the non-holonomic constraints. The dependent coordinate is also
# provided, with the holonomic constraint. Again, this is only provided
# for the linearization process.
KM = KanesMethod(N,
q_ind=[q1, q2, q5],
q_dependent=[q4],
configuration_constraints=conlist_coord,
u_ind=[u2, u3, u5],
u_dependent=[u1, u4, u6],
velocity_constraints=conlist_speed,
kd_eqs=kd)
(fr, frstar) = KM.kanes_equations(FL, BL)
# This is the start of entering in the numerical values from the benchmark
# paper to validate the eigen values of the linearized equations from this
# model to the reference eigen values. Look at the aforementioned paper for
# more information. Some of these are intermediate values, used to
# transform values from the paper into the coordinate systems used in this
# model.
PaperRadRear = 0.3
PaperRadFront = 0.35
HTA = evalf.N(pi / 2 - pi / 10)
TrailPaper = 0.08
rake = evalf.N(-(TrailPaper * sin(HTA) - (PaperRadFront * cos(HTA))))
PaperWb = 1.02
PaperFrameCgX = 0.3
PaperFrameCgZ = 0.9
PaperForkCgX = 0.9
PaperForkCgZ = 0.7
FrameLength = evalf.N(PaperWb * sin(HTA) -
(rake - (PaperRadFront - PaperRadRear) * cos(HTA)))
FrameCGNorm = evalf.N((PaperFrameCgZ - PaperRadRear -
(PaperFrameCgX / sin(HTA)) * cos(HTA)) * sin(HTA))
FrameCGPar = evalf.N(
(PaperFrameCgX / sin(HTA) +
(PaperFrameCgZ - PaperRadRear - PaperFrameCgX / sin(HTA) * cos(HTA)) *
cos(HTA)))
tempa = evalf.N((PaperForkCgZ - PaperRadFront))
tempb = evalf.N((PaperWb - PaperForkCgX))
tempc = evalf.N(sqrt(tempa**2 + tempb**2))
PaperForkL = evalf.N(
(PaperWb * cos(HTA) - (PaperRadFront - PaperRadRear) * sin(HTA)))
ForkCGNorm = evalf.N(rake +
(tempc * sin(pi / 2 - HTA - acos(tempa / tempc))))
ForkCGPar = evalf.N(tempc * cos((pi / 2 - HTA) - acos(tempa / tempc)) -
PaperForkL)
# Here is the final assembly of the numerical values. The symbol 'v' is the
# forward speed of the bicycle (a concept which only makes sense in the
# upright, static equilibrium case?). These are in a dictionary which will
# later be substituted in. Again the sign on the *product* of inertia
# values is flipped here, due to different orientations of coordinate
# systems.
v = symbols('v')
val_dict = {
WFrad: PaperRadFront,
WRrad: PaperRadRear,
htangle: HTA,
forkoffset: rake,
forklength: PaperForkL,
framelength: FrameLength,
forkcg1: ForkCGPar,
forkcg3: ForkCGNorm,
framecg1: FrameCGNorm,
framecg3: FrameCGPar,
Iwr11: 0.0603,
Iwr22: 0.12,
Iwf11: 0.1405,
Iwf22: 0.28,
Ifork11: 0.05892,
Ifork22: 0.06,
Ifork33: 0.00708,
Ifork31: 0.00756,
Iframe11: 9.2,
Iframe22: 11,
Iframe33: 2.8,
Iframe31: -2.4,
mfork: 4,
mframe: 85,
mwf: 3,
mwr: 2,
g: 9.81,
q1: 0,
q2: 0,
q4: 0,
q5: 0,
u1: 0,
u2: 0,
u3: v / PaperRadRear,
u4: 0,
u5: 0,
u6: v / PaperRadFront
}
# Linearizes the forcing vector; the equations are set up as MM udot =
# forcing, where MM is the mass matrix, udot is the vector representing the
# time derivatives of the generalized speeds, and forcing is a vector which
# contains both external forcing terms and internal forcing terms, such as
# centripital or coriolis forces. This actually returns a matrix with as
# many rows as *total* coordinates and speeds, but only as many columns as
# independent coordinates and speeds.
with warnings.catch_warnings():
warnings.filterwarnings("ignore", category=SymPyDeprecationWarning)
forcing_lin = KM.linearize()[0]
# As mentioned above, the size of the linearized forcing terms is expanded
# to include both q's and u's, so the mass matrix must have this done as
# well. This will likely be changed to be part of the linearized process,
# for future reference.
MM_full = KM.mass_matrix_full
MM_full_s = MM_full.subs(val_dict)
forcing_lin_s = forcing_lin.subs(KM.kindiffdict()).subs(val_dict)
MM_full_s = MM_full_s.evalf()
forcing_lin_s = forcing_lin_s.evalf()
# Finally, we construct an "A" matrix for the form xdot = A x (x being the
# state vector, although in this case, the sizes are a little off). The
# following line extracts only the minimum entries required for eigenvalue
# analysis, which correspond to rows and columns for lean, steer, lean
# rate, and steer rate.
Amat = MM_full_s.inv() * forcing_lin_s
A = Amat.extract([1, 2, 4, 6], [1, 2, 3, 5])
# Precomputed for comparison
Res = Matrix([[0, 0, 1.0, 0], [0, 0, 0, 1.0],
[
9.48977444677355,
-0.891197738059089 * v**2 - 0.571523173729245,
-0.105522449805691 * v, -0.330515398992311 * v
],
[
11.7194768719633,
-1.97171508499972 * v**2 + 30.9087533932407,
3.67680523332152 * v, -3.08486552743311 * v
]])
# Actual eigenvalue comparison
eps = 1.e-12
for i in xrange(6):
error = Res.subs(v, i) - A.subs(v, i)
assert all(abs(x) < eps for x in error)
def test_rolling_disc():
# Rolling Disc Example
# Here the rolling disc is formed from the contact point up, removing the
# need to introduce generalized speeds. Only 3 configuration and three
# speed variables are need to describe this system, along with the disc's
# mass and radius, and the local gravity (note that mass will drop out).
q1, q2, q3, u1, u2, u3 = dynamicsymbols('q1 q2 q3 u1 u2 u3')
q1d, q2d, q3d, u1d, u2d, u3d = dynamicsymbols('q1 q2 q3 u1 u2 u3', 1)
r, m, g = symbols('r m g')
# The kinematics are formed by a series of simple rotations. Each simple
# rotation creates a new frame, and the next rotation is defined by the new
# frame's basis vectors. This example uses a 3-1-2 series of rotations, or
# Z, X, Y series of rotations. Angular velocity for this is defined using
# the second frame's basis (the lean frame).
N = ReferenceFrame('N')
Y = N.orientnew('Y', 'Axis', [q1, N.z])
L = Y.orientnew('L', 'Axis', [q2, Y.x])
R = L.orientnew('R', 'Axis', [q3, L.y])
w_R_N_qd = R.ang_vel_in(N)
R.set_ang_vel(N, u1 * L.x + u2 * L.y + u3 * L.z)
# This is the translational kinematics. We create a point with no velocity
# in N; this is the contact point between the disc and ground. Next we form
# the position vector from the contact point to the disc's center of mass.
# Finally we form the velocity and acceleration of the disc.
C = Point('C')
C.set_vel(N, 0)
Dmc = C.locatenew('Dmc', r * L.z)
Dmc.v2pt_theory(C, N, R)
# This is a simple way to form the inertia dyadic.
I = inertia(L, m / 4 * r**2, m / 2 * r**2, m / 4 * r**2)
# Kinematic differential equations; how the generalized coordinate time
# derivatives relate to generalized speeds.
kd = [dot(R.ang_vel_in(N) - w_R_N_qd, uv) for uv in L]
# Creation of the force list; it is the gravitational force at the mass
# center of the disc. Then we create the disc by assigning a Point to the
# center of mass attribute, a ReferenceFrame to the frame attribute, and mass
# and inertia. Then we form the body list.
ForceList = [(Dmc, -m * g * Y.z)]
BodyD = RigidBody('BodyD', Dmc, R, m, (I, Dmc))
BodyList = [BodyD]
# Finally we form the equations of motion, using the same steps we did
# before. Specify inertial frame, supply generalized speeds, supply
# kinematic differential equation dictionary, compute Fr from the force
# list and Fr* from the body list, compute the mass matrix and forcing
# terms, then solve for the u dots (time derivatives of the generalized
# speeds).
KM = KanesMethod(N, q_ind=[q1, q2, q3], u_ind=[u1, u2, u3], kd_eqs=kd)
with warns_deprecated_sympy():
KM.kanes_equations(ForceList, BodyList)
MM = KM.mass_matrix
forcing = KM.forcing
rhs = MM.inv() * forcing
kdd = KM.kindiffdict()
rhs = rhs.subs(kdd)
rhs.simplify()
assert rhs.expand() == Matrix([
(6 * u2 * u3 * r - u3**2 * r * tan(q2) + 4 * g * sin(q2)) / (5 * r),
-2 * u1 * u3 / 3, u1 * (-2 * u2 + u3 * tan(q2))
]).expand()
assert simplify(KM.rhs() -
KM.mass_matrix_full.LUsolve(KM.forcing_full)) == zeros(
6, 1)
# This code tests our output vs. benchmark values. When r=g=m=1, the
# critical speed (where all eigenvalues of the linearized equations are 0)
# is 1 / sqrt(3) for the upright case.
A = KM.linearize(A_and_B=True)[0]
A_upright = A.subs({
r: 1,
g: 1,
m: 1
}).subs({
q1: 0,
q2: 0,
q3: 0,
u1: 0,
u3: 0
})
import sympy
assert sympy.sympify(A_upright.subs({u2: 1 / sqrt(3)})).eigenvals() == {
S.Zero: 6
}
def test_bicycle():
if ON_TRAVIS:
skip("Too slow for travis.")
# Code to get equations of motion for a bicycle modeled as in:
# J.P Meijaard, Jim M Papadopoulos, Andy Ruina and A.L Schwab. Linearized
# dynamics equations for the balance and steer of a bicycle: a benchmark
# and review. Proceedings of The Royal Society (2007) 463, 1955-1982
# doi: 10.1098/rspa.2007.1857
# Note that this code has been crudely ported from Autolev, which is the
# reason for some of the unusual naming conventions. It was purposefully as
# similar as possible in order to aide debugging.
# Declare Coordinates & Speeds
# Simple definitions for qdots - qd = u
# Speeds are: yaw frame ang. rate, roll frame ang. rate, rear wheel frame
# ang. rate (spinning motion), frame ang. rate (pitching motion), steering
# frame ang. rate, and front wheel ang. rate (spinning motion).
# Wheel positions are ignorable coordinates, so they are not introduced.
q1, q2, q4, q5 = dynamicsymbols('q1 q2 q4 q5')
q1d, q2d, q4d, q5d = dynamicsymbols('q1 q2 q4 q5', 1)
u1, u2, u3, u4, u5, u6 = dynamicsymbols('u1 u2 u3 u4 u5 u6')
u1d, u2d, u3d, u4d, u5d, u6d = dynamicsymbols('u1 u2 u3 u4 u5 u6', 1)
# Declare System's Parameters
WFrad, WRrad, htangle, forkoffset = symbols('WFrad WRrad htangle forkoffset')
forklength, framelength, forkcg1 = symbols('forklength framelength forkcg1')
forkcg3, framecg1, framecg3, Iwr11 = symbols('forkcg3 framecg1 framecg3 Iwr11')
Iwr22, Iwf11, Iwf22, Iframe11 = symbols('Iwr22 Iwf11 Iwf22 Iframe11')
Iframe22, Iframe33, Iframe31, Ifork11 = symbols('Iframe22 Iframe33 Iframe31 Ifork11')
Ifork22, Ifork33, Ifork31, g = symbols('Ifork22 Ifork33 Ifork31 g')
mframe, mfork, mwf, mwr = symbols('mframe mfork mwf mwr')
# Set up reference frames for the system
# N - inertial
# Y - yaw
# R - roll
# WR - rear wheel, rotation angle is ignorable coordinate so not oriented
# Frame - bicycle frame
# TempFrame - statically rotated frame for easier reference inertia definition
# Fork - bicycle fork
# TempFork - statically rotated frame for easier reference inertia definition
# WF - front wheel, again posses a ignorable coordinate
N = ReferenceFrame('N')
Y = N.orientnew('Y', 'Axis', [q1, N.z])
R = Y.orientnew('R', 'Axis', [q2, Y.x])
Frame = R.orientnew('Frame', 'Axis', [q4 + htangle, R.y])
WR = ReferenceFrame('WR')
TempFrame = Frame.orientnew('TempFrame', 'Axis', [-htangle, Frame.y])
Fork = Frame.orientnew('Fork', 'Axis', [q5, Frame.x])
TempFork = Fork.orientnew('TempFork', 'Axis', [-htangle, Fork.y])
WF = ReferenceFrame('WF')
# Kinematics of the Bicycle First block of code is forming the positions of
# the relevant points
# rear wheel contact -> rear wheel mass center -> frame mass center +
# frame/fork connection -> fork mass center + front wheel mass center ->
# front wheel contact point
WR_cont = Point('WR_cont')
WR_mc = WR_cont.locatenew('WR_mc', WRrad * R.z)
Steer = WR_mc.locatenew('Steer', framelength * Frame.z)
Frame_mc = WR_mc.locatenew('Frame_mc', - framecg1 * Frame.x
+ framecg3 * Frame.z)
Fork_mc = Steer.locatenew('Fork_mc', - forkcg1 * Fork.x
+ forkcg3 * Fork.z)
WF_mc = Steer.locatenew('WF_mc', forklength * Fork.x + forkoffset * Fork.z)
WF_cont = WF_mc.locatenew('WF_cont', WFrad * (dot(Fork.y, Y.z) * Fork.y -
Y.z).normalize())
# Set the angular velocity of each frame.
# Angular accelerations end up being calculated automatically by
# differentiating the angular velocities when first needed.
# u1 is yaw rate
# u2 is roll rate
# u3 is rear wheel rate
# u4 is frame pitch rate
# u5 is fork steer rate
# u6 is front wheel rate
Y.set_ang_vel(N, u1 * Y.z)
R.set_ang_vel(Y, u2 * R.x)
WR.set_ang_vel(Frame, u3 * Frame.y)
Frame.set_ang_vel(R, u4 * Frame.y)
Fork.set_ang_vel(Frame, u5 * Fork.x)
WF.set_ang_vel(Fork, u6 * Fork.y)
# Form the velocities of the previously defined points, using the 2 - point
# theorem (written out by hand here). Accelerations again are calculated
# automatically when first needed.
WR_cont.set_vel(N, 0)
WR_mc.v2pt_theory(WR_cont, N, WR)
Steer.v2pt_theory(WR_mc, N, Frame)
Frame_mc.v2pt_theory(WR_mc, N, Frame)
Fork_mc.v2pt_theory(Steer, N, Fork)
WF_mc.v2pt_theory(Steer, N, Fork)
WF_cont.v2pt_theory(WF_mc, N, WF)
# Sets the inertias of each body. Uses the inertia frame to construct the
# inertia dyadics. Wheel inertias are only defined by principle moments of
# inertia, and are in fact constant in the frame and fork reference frames;
# it is for this reason that the orientations of the wheels does not need
# to be defined. The frame and fork inertias are defined in the 'Temp'
# frames which are fixed to the appropriate body frames; this is to allow
# easier input of the reference values of the benchmark paper. Note that
# due to slightly different orientations, the products of inertia need to
# have their signs flipped; this is done later when entering the numerical
# value.
Frame_I = (inertia(TempFrame, Iframe11, Iframe22, Iframe33, 0, 0, Iframe31), Frame_mc)
Fork_I = (inertia(TempFork, Ifork11, Ifork22, Ifork33, 0, 0, Ifork31), Fork_mc)
WR_I = (inertia(Frame, Iwr11, Iwr22, Iwr11), WR_mc)
WF_I = (inertia(Fork, Iwf11, Iwf22, Iwf11), WF_mc)
# Declaration of the RigidBody containers. ::
BodyFrame = RigidBody('BodyFrame', Frame_mc, Frame, mframe, Frame_I)
BodyFork = RigidBody('BodyFork', Fork_mc, Fork, mfork, Fork_I)
BodyWR = RigidBody('BodyWR', WR_mc, WR, mwr, WR_I)
BodyWF = RigidBody('BodyWF', WF_mc, WF, mwf, WF_I)
# The kinematic differential equations; they are defined quite simply. Each
# entry in this list is equal to zero.
kd = [q1d - u1, q2d - u2, q4d - u4, q5d - u5]
# The nonholonomic constraints are the velocity of the front wheel contact
# point dotted into the X, Y, and Z directions; the yaw frame is used as it
# is "closer" to the front wheel (1 less DCM connecting them). These
# constraints force the velocity of the front wheel contact point to be 0
# in the inertial frame; the X and Y direction constraints enforce a
# "no-slip" condition, and the Z direction constraint forces the front
# wheel contact point to not move away from the ground frame, essentially
# replicating the holonomic constraint which does not allow the frame pitch
# to change in an invalid fashion.
conlist_speed = [WF_cont.vel(N) & Y.x, WF_cont.vel(N) & Y.y, WF_cont.vel(N) & Y.z]
# The holonomic constraint is that the position from the rear wheel contact
# point to the front wheel contact point when dotted into the
# normal-to-ground plane direction must be zero; effectively that the front
# and rear wheel contact points are always touching the ground plane. This
# is actually not part of the dynamic equations, but instead is necessary
# for the lineraization process.
conlist_coord = [WF_cont.pos_from(WR_cont) & Y.z]
# The force list; each body has the appropriate gravitational force applied
# at its mass center.
FL = [(Frame_mc, -mframe * g * Y.z),
(Fork_mc, -mfork * g * Y.z),
(WF_mc, -mwf * g * Y.z),
(WR_mc, -mwr * g * Y.z)]
BL = [BodyFrame, BodyFork, BodyWR, BodyWF]
# The N frame is the inertial frame, coordinates are supplied in the order
# of independent, dependent coordinates, as are the speeds. The kinematic
# differential equation are also entered here. Here the dependent speeds
# are specified, in the same order they were provided in earlier, along
# with the non-holonomic constraints. The dependent coordinate is also
# provided, with the holonomic constraint. Again, this is only provided
# for the linearization process.
KM = KanesMethod(N, q_ind=[q1, q2, q5],
q_dependent=[q4], configuration_constraints=conlist_coord,
u_ind=[u2, u3, u5],
u_dependent=[u1, u4, u6], velocity_constraints=conlist_speed,
kd_eqs=kd)
(fr, frstar) = KM.kanes_equations(FL, BL)
# This is the start of entering in the numerical values from the benchmark
# paper to validate the eigen values of the linearized equations from this
# model to the reference eigen values. Look at the aforementioned paper for
# more information. Some of these are intermediate values, used to
# transform values from the paper into the coordinate systems used in this
# model.
PaperRadRear = 0.3
PaperRadFront = 0.35
HTA = evalf.N(pi / 2 - pi / 10)
TrailPaper = 0.08
rake = evalf.N(-(TrailPaper*sin(HTA)-(PaperRadFront*cos(HTA))))
PaperWb = 1.02
PaperFrameCgX = 0.3
PaperFrameCgZ = 0.9
PaperForkCgX = 0.9
PaperForkCgZ = 0.7
FrameLength = evalf.N(PaperWb*sin(HTA)-(rake-(PaperRadFront-PaperRadRear)*cos(HTA)))
FrameCGNorm = evalf.N((PaperFrameCgZ - PaperRadRear-(PaperFrameCgX/sin(HTA))*cos(HTA))*sin(HTA))
FrameCGPar = evalf.N((PaperFrameCgX / sin(HTA) + (PaperFrameCgZ - PaperRadRear - PaperFrameCgX / sin(HTA) * cos(HTA)) * cos(HTA)))
tempa = evalf.N((PaperForkCgZ - PaperRadFront))
tempb = evalf.N((PaperWb-PaperForkCgX))
tempc = evalf.N(sqrt(tempa**2+tempb**2))
PaperForkL = evalf.N((PaperWb*cos(HTA)-(PaperRadFront-PaperRadRear)*sin(HTA)))
ForkCGNorm = evalf.N(rake+(tempc * sin(pi/2-HTA-acos(tempa/tempc))))
ForkCGPar = evalf.N(tempc * cos((pi/2-HTA)-acos(tempa/tempc))-PaperForkL)
# Here is the final assembly of the numerical values. The symbol 'v' is the
# forward speed of the bicycle (a concept which only makes sense in the
# upright, static equilibrium case?). These are in a dictionary which will
# later be substituted in. Again the sign on the *product* of inertia
# values is flipped here, due to different orientations of coordinate
# systems.
v = symbols('v')
val_dict = {WFrad: PaperRadFront,
WRrad: PaperRadRear,
htangle: HTA,
forkoffset: rake,
forklength: PaperForkL,
framelength: FrameLength,
forkcg1: ForkCGPar,
forkcg3: ForkCGNorm,
framecg1: FrameCGNorm,
framecg3: FrameCGPar,
Iwr11: 0.0603,
Iwr22: 0.12,
Iwf11: 0.1405,
Iwf22: 0.28,
Ifork11: 0.05892,
Ifork22: 0.06,
Ifork33: 0.00708,
Ifork31: 0.00756,
Iframe11: 9.2,
Iframe22: 11,
Iframe33: 2.8,
Iframe31: -2.4,
mfork: 4,
mframe: 85,
mwf: 3,
mwr: 2,
g: 9.81,
q1: 0,
q2: 0,
q4: 0,
q5: 0,
u1: 0,
u2: 0,
u3: v / PaperRadRear,
u4: 0,
u5: 0,
u6: v / PaperRadFront}
# Linearizes the forcing vector; the equations are set up as MM udot =
# forcing, where MM is the mass matrix, udot is the vector representing the
# time derivatives of the generalized speeds, and forcing is a vector which
# contains both external forcing terms and internal forcing terms, such as
# centripital or coriolis forces. This actually returns a matrix with as
# many rows as *total* coordinates and speeds, but only as many columns as
# independent coordinates and speeds.
forcing_lin = KM.linearize()[0]
# As mentioned above, the size of the linearized forcing terms is expanded
# to include both q's and u's, so the mass matrix must have this done as
# well. This will likely be changed to be part of the linearized process,
# for future reference.
MM_full = KM.mass_matrix_full
MM_full_s = MM_full.subs(val_dict)
forcing_lin_s = forcing_lin.subs(KM.kindiffdict()).subs(val_dict)
MM_full_s = MM_full_s.evalf()
forcing_lin_s = forcing_lin_s.evalf()
# Finally, we construct an "A" matrix for the form xdot = A x (x being the
# state vector, although in this case, the sizes are a little off). The
# following line extracts only the minimum entries required for eigenvalue
# analysis, which correspond to rows and columns for lean, steer, lean
# rate, and steer rate.
Amat = MM_full_s.inv() * forcing_lin_s
A = Amat.extract([1, 2, 4, 6], [1, 2, 3, 5])
# Precomputed for comparison
Res = Matrix([[ 0, 0, 1.0, 0],
[ 0, 0, 0, 1.0],
[9.48977444677355, -0.891197738059089*v**2 - 0.571523173729245, -0.105522449805691*v, -0.330515398992311*v],
[11.7194768719633, -1.97171508499972*v**2 + 30.9087533932407, 3.67680523332152*v, -3.08486552743311*v]])
# Actual eigenvalue comparison
eps = 1.e-12
for i in range(6):
error = Res.subs(v, i) - A.subs(v, i)
assert all(abs(x) < eps for x in error)
class Linkage(MultiBodySystem):
"""TODO
"""
def __init__(self, name):
self._name = name
self._root = RootLink(self) # TODO maybe don't need backpointer
self._constants = dict()
self._constant_descs = dict()
self._forces = dict()
self._gravity_vector = None
self._gravity_vector_updated = Event(
'Update gravity forces when gravity vector is changed.')
self._gravity_vector_updated.subscriber_new(
self._manage_gravity_forces)
def _get_name(self):
return self._name
def _set_name(self, name):
self._name = name
name = property(_get_name, _set_name)
def _get_root(self):
return self._root
root = property(_get_root)
def constant_new(self, name, description):
self._constants[name] = symbols(name)
self._constant_descs[name] = description
return self._constants[name]
def force_new(self, name, point_of_application, vec):
"""TODO
reserved names: '_gravity'
"""
# TODO
#if name in self._forces:
# # TODO
# raise Exception("Force with name '{}' already exists.".format(name))
self._forces[name] = (point_of_application, vec)
def force_del(self, name):
self._forces.pop(name)
def _manage_gravity_forces(self):
# TODO must modify to account for gravity_force being modified more
# than once.
for body in self.body_list():
self.force_new('%s_gravity', body.masscenter,
body.mass * self.gravity_vector)
def _get_gravity_vector(self):
return self._gravity_vector
def _set_gravity_vector(self, vec):
_check_vector(vec)
self._gravity_vector = vec
self._gravity_vector_updated.fire()
gravity_vector = property(_get_gravity_vector, _set_gravity_vector)
def independent_coordinates(self):
return self.root.independent_coordinates_in_subtree()
def independent_speeds(self):
return self.root.independent_speeds_in_subtree()
def kinematic_differential_equations(self):
return self.root.kinematic_differential_equations_in_subtree()
def body_list(self):
return self.root.body_list_in_subtree()
def force_list(self):
return self._forces.values()
#TODO def _init_kanes_method(self):
#TODO # TODO move the creation of Kane's Method somewhere else.
#TODO self._kanes_method = KanesMethod(self.independent_coordinates,
#TODO self.independent_speeds, self.kinematic_diffeqs)
#TODO # TODO must make this call to get the mass matrix, etc.?
#TODO self._kanes_method.kanes_equations(self.force_list, self.body_list)
def mass_matrix(self):
#if not (self._kanes_method and self.up_to_date):
# self._init_kanes_method()
# TODO move the creation of Kane's Method somewhere else.
self._kanes_method = KanesMethod(
self.root.frame,
q_ind=self.independent_coordinates(),
u_ind=self.independent_speeds(),
kd_eqs=self.kinematic_differential_equations())
# TODO must make this call to get the mass matrix, etc.?
self._kanes_method.kanes_equations(self.force_list(), self.body_list())
return self._kanes_method.mass_matrix
def state_derivatives(self):
# TODO find a way to use a cached mass matrix.
kin_diff_eqns = self._kanes_method.kindiffdict()
state_derivatives = self.mass_matrix.inv() * self._kanes_method.forcing
state_derivatives = state_derivatives.subs(kin_diff_eqns)
state_derivatives.simplify()
return state_derivatives
def _check_link_name(self):
# TODO
pass
def test_linearize_rolling_disc_kane():
# Symbols for time and constant parameters
t, r, m, g, v = symbols('t r m g v')
# Configuration variables and their time derivatives
q1, q2, q3, q4, q5, q6 = q = dynamicsymbols('q1:7')
q1d, q2d, q3d, q4d, q5d, q6d = qd = [qi.diff(t) for qi in q]
# Generalized speeds and their time derivatives
u = dynamicsymbols('u:6')
u1, u2, u3, u4, u5, u6 = u = dynamicsymbols('u1:7')
u1d, u2d, u3d, u4d, u5d, u6d = [ui.diff(t) for ui in u]
# Reference frames
N = ReferenceFrame('N') # Inertial frame
NO = Point('NO') # Inertial origin
A = N.orientnew('A', 'Axis', [q1, N.z]) # Yaw intermediate frame
B = A.orientnew('B', 'Axis', [q2, A.x]) # Lean intermediate frame
C = B.orientnew('C', 'Axis', [q3, B.y]) # Disc fixed frame
CO = NO.locatenew('CO', q4 * N.x + q5 * N.y + q6 * N.z) # Disc center
# Disc angular velocity in N expressed using time derivatives of coordinates
w_c_n_qd = C.ang_vel_in(N)
w_b_n_qd = B.ang_vel_in(N)
# Inertial angular velocity and angular acceleration of disc fixed frame
C.set_ang_vel(N, u1 * B.x + u2 * B.y + u3 * B.z)
# Disc center velocity in N expressed using time derivatives of coordinates
v_co_n_qd = CO.pos_from(NO).dt(N)
# Disc center velocity in N expressed using generalized speeds
CO.set_vel(N, u4 * C.x + u5 * C.y + u6 * C.z)
# Disc Ground Contact Point
P = CO.locatenew('P', r * B.z)
P.v2pt_theory(CO, N, C)
# Configuration constraint
f_c = Matrix([q6 - dot(CO.pos_from(P), N.z)])
# Velocity level constraints
f_v = Matrix([dot(P.vel(N), uv) for uv in C])
# Kinematic differential equations
kindiffs = Matrix([dot(w_c_n_qd - C.ang_vel_in(N), uv) for uv in B] +
[dot(v_co_n_qd - CO.vel(N), uv) for uv in N])
qdots = solve(kindiffs, qd)
# Set angular velocity of remaining frames
B.set_ang_vel(N, w_b_n_qd.subs(qdots))
C.set_ang_acc(
N,
C.ang_vel_in(N).dt(B) + cross(B.ang_vel_in(N), C.ang_vel_in(N)))
# Active forces
F_CO = m * g * A.z
# Create inertia dyadic of disc C about point CO
I = (m * r**2) / 4
J = (m * r**2) / 2
I_C_CO = inertia(C, I, J, I)
Disc = RigidBody('Disc', CO, C, m, (I_C_CO, CO))
BL = [Disc]
FL = [(CO, F_CO)]
KM = KanesMethod(N, [q1, q2, q3, q4, q5], [u1, u2, u3],
kd_eqs=kindiffs,
q_dependent=[q6],
configuration_constraints=f_c,
u_dependent=[u4, u5, u6],
velocity_constraints=f_v)
(fr, fr_star) = KM.kanes_equations(BL, FL)
# Test generalized form equations
linearizer = KM.to_linearizer()
assert linearizer.f_c == f_c
assert linearizer.f_v == f_v
assert linearizer.f_a == f_v.diff(t).subs(KM.kindiffdict())
sol = solve(linearizer.f_0 + linearizer.f_1, qd)
for qi in qdots.keys():
assert sol[qi] == qdots[qi]
assert simplify(linearizer.f_2 + linearizer.f_3 - fr - fr_star) == Matrix(
[0, 0, 0])
# Perform the linearization
# Precomputed operating point
q_op = {q6: -r * cos(q2)}
u_op = {
u1: 0,
u2: sin(q2) * q1d + q3d,
u3: cos(q2) * q1d,
u4: -r * (sin(q2) * q1d + q3d) * cos(q3),
u5: 0,
u6: -r * (sin(q2) * q1d + q3d) * sin(q3)
}
qd_op = {
q2d: 0,
q4d: -r * (sin(q2) * q1d + q3d) * cos(q1),
q5d: -r * (sin(q2) * q1d + q3d) * sin(q1),
q6d: 0
}
ud_op = {
u1d:
4 * g * sin(q2) / (5 * r) + sin(2 * q2) * q1d**2 / 2 +
6 * cos(q2) * q1d * q3d / 5,
u2d:
0,
u3d:
0,
u4d:
r * (sin(q2) * sin(q3) * q1d * q3d + sin(q3) * q3d**2),
u5d:
r * (4 * g * sin(q2) /
(5 * r) + sin(2 * q2) * q1d**2 / 2 + 6 * cos(q2) * q1d * q3d / 5),
u6d:
-r * (sin(q2) * cos(q3) * q1d * q3d + cos(q3) * q3d**2)
}
A, B = linearizer.linearize(op_point=[q_op, u_op, qd_op, ud_op],
A_and_B=True,
simplify=True)
upright_nominal = {q1d: 0, q2: 0, m: 1, r: 1, g: 1}
# Precomputed solution
A_sol = Matrix([[0, 0, 0, 0, 0, 0, 0, 1], [0, 0, 0, 0, 0, 1, 0, 0],
[0, 0, 0, 0, 0, 0, 1, 0],
[sin(q1) * q3d, 0, 0, 0, 0, -sin(q1), -cos(q1), 0],
[-cos(q1) * q3d, 0, 0, 0, 0,
cos(q1), -sin(q1), 0],
[0, Rational(4, 5), 0, 0, 0, 0, 0, 6 * q3d / 5],
[0, 0, 0, 0, 0, 0, 0, 0], [0, 0, 0, 0, 0, -2 * q3d, 0, 0]])
B_sol = Matrix([])
# Check that linearization is correct
assert A.subs(upright_nominal) == A_sol
assert B.subs(upright_nominal) == B_sol
# Check eigenvalues at critical speed are all zero:
assert sympify(A.subs(upright_nominal).subs(q3d,
1 / sqrt(3))).eigenvals() == {
0: 8
}
class Linkage(MultiBodySystem):
"""TODO
"""
def __init__(self, name):
self._name = name
self._root = RootLink(self) # TODO maybe don't need backpointer
self._constants = dict()
self._constant_descs = dict()
self._forces = dict()
self._gravity_vector = None
self._gravity_vector_updated = Event(
'Update gravity forces when gravity vector is changed.')
self._gravity_vector_updated.subscriber_new(self._manage_gravity_forces)
def _get_name(self):
return self._name
def _set_name(self, name):
self._name = name
name = property(_get_name, _set_name)
def _get_root(self):
return self._root
root = property(_get_root)
def constant_new(self, name, description):
self._constants[name] = symbols(name)
self._constant_descs[name] = description
return self._constants[name]
def force_new(self, name, point_of_application, vec):
"""TODO
reserved names: '_gravity'
"""
# TODO
#if name in self._forces:
# # TODO
# raise Exception("Force with name '{}' already exists.".format(name))
self._forces[name] = (point_of_application, vec)
def force_del(self, name):
self._forces.pop(name)
def _manage_gravity_forces(self):
# TODO must modify to account for gravity_force being modified more
# than once.
for body in self.body_list():
self.force_new('%s_gravity', body.masscenter, body.mass * self.gravity_vector)
def _get_gravity_vector(self):
return self._gravity_vector
def _set_gravity_vector(self, vec):
_check_vector(vec)
self._gravity_vector = vec
self._gravity_vector_updated.fire()
gravity_vector = property(_get_gravity_vector, _set_gravity_vector)
def independent_coordinates(self):
return self.root.independent_coordinates_in_subtree()
def independent_speeds(self):
return self.root.independent_speeds_in_subtree()
def kinematic_differential_equations(self):
return self.root.kinematic_differential_equations_in_subtree()
def body_list(self):
return self.root.body_list_in_subtree()
def force_list(self):
return self._forces.values()
#TODO def _init_kanes_method(self):
#TODO # TODO move the creation of Kane's Method somewhere else.
#TODO self._kanes_method = KanesMethod(self.independent_coordinates,
#TODO self.independent_speeds, self.kinematic_diffeqs)
#TODO # TODO must make this call to get the mass matrix, etc.?
#TODO self._kanes_method.kanes_equations(self.force_list, self.body_list)
def mass_matrix(self):
#if not (self._kanes_method and self.up_to_date):
# self._init_kanes_method()
# TODO move the creation of Kane's Method somewhere else.
self._kanes_method = KanesMethod(self.root.frame,
q_ind=self.independent_coordinates(),
u_ind=self.independent_speeds(),
kd_eqs=self.kinematic_differential_equations()
)
# TODO must make this call to get the mass matrix, etc.?
self._kanes_method.kanes_equations(self.force_list(), self.body_list());
return self._kanes_method.mass_matrix
def state_derivatives(self):
# TODO find a way to use a cached mass matrix.
kin_diff_eqns = self._kanes_method.kindiffdict()
state_derivatives = self.mass_matrix.inv() * self._kanes_method.forcing
state_derivatives = state_derivatives.subs(kin_diff_eqns)
state_derivatives.simplify()
return state_derivatives
def _check_link_name(self):
# TODO
pass
kd_eqs=kd,
q_dependent=[q2],
configuration_constraints=cc,
u_dependent=[u2],
velocity_constraints=vc)
(fr, frstar) = KM.kanes_equations(FL, BL)
# looks like some of the derivative terms were not substituted correctly
forcing_vector = KM.forcing.subs(kd_map)
derivative_generator = (expr.atoms(Derivative)
for expr in find_dynamicsymbols(forcing_vector))
if frozenset().union(*(derivative_generator)):
forcing_vector = forcing_vector.subs(kd_map)
#List apprehension
kdd = KM.kindiffdict()
coord_derivs = Matrix([kdd[c.diff()] for c in KM.q])
#RHS = mass_matrix.LU_solve(forcing_vector)
RHS = generate_ode_function(forcing_vector,
KM.q,
KM.u,
constants,
mass_matrix=KM.mass_matrix,
coordinate_derivatives=coord_derivs,
constants_arg_type='dictionary')
# Initial conditions, time and constant values
# q = [q1,theta,q2,q1dot,omega,q2dot]
q0 = np.deg2rad((45, 0, 60, 0, 0.5, 0))
constants = {
def test_rolling_disc():
# Rolling Disc Example
# Here the rolling disc is formed from the contact point up, removing the
# need to introduce generalized speeds. Only 3 configuration and three
# speed variables are need to describe this system, along with the disc's
# mass and radius, and the local gravity (note that mass will drop out).
q1, q2, q3, u1, u2, u3 = dynamicsymbols('q1 q2 q3 u1 u2 u3')
q1d, q2d, q3d, u1d, u2d, u3d = dynamicsymbols('q1 q2 q3 u1 u2 u3', 1)
r, m, g = symbols('r m g')
# The kinematics are formed by a series of simple rotations. Each simple
# rotation creates a new frame, and the next rotation is defined by the new
# frame's basis vectors. This example uses a 3-1-2 series of rotations, or
# Z, X, Y series of rotations. Angular velocity for this is defined using
# the second frame's basis (the lean frame).
N = ReferenceFrame('N')
Y = N.orientnew('Y', 'Axis', [q1, N.z])
L = Y.orientnew('L', 'Axis', [q2, Y.x])
R = L.orientnew('R', 'Axis', [q3, L.y])
R.set_ang_vel(N, u1 * L.x + u2 * L.y + u3 * L.z)
R.set_ang_acc(N,
R.ang_vel_in(N).dt(R) + (R.ang_vel_in(N) ^ R.ang_vel_in(N)))
# This is the translational kinematics. We create a point with no velocity
# in N; this is the contact point between the disc and ground. Next we form
# the position vector from the contact point to the disc's center of mass.
# Finally we form the velocity and acceleration of the disc.
C = Point('C')
C.set_vel(N, 0)
Dmc = C.locatenew('Dmc', r * L.z)
Dmc.v2pt_theory(C, N, R)
Dmc.a2pt_theory(C, N, R)
# This is a simple way to form the inertia dyadic.
I = inertia(L, m / 4 * r**2, m / 2 * r**2, m / 4 * r**2)
# Kinematic differential equations; how the generalized coordinate time
# derivatives relate to generalized speeds.
kd = [q1d - u3 / cos(q2), q2d - u1, q3d - u2 + u3 * tan(q2)]
# Creation of the force list; it is the gravitational force at the mass
# center of the disc. Then we create the disc by assigning a Point to the
# center of mass attribute, a ReferenceFrame to the frame attribute, and mass
# and inertia. Then we form the body list.
ForceList = [(Dmc, -m * g * Y.z)]
BodyD = RigidBody('BodyD', Dmc, R, m, (I, Dmc))
BodyList = [BodyD]
# Finally we form the equations of motion, using the same steps we did
# before. Specify inertial frame, supply generalized speeds, supply
# kinematic differential equation dictionary, compute Fr from the force
# list and Fr* from the body list, compute the mass matrix and forcing
# terms, then solve for the u dots (time derivatives of the generalized
# speeds).
KM = KanesMethod(N, q_ind=[q1, q2, q3], u_ind=[u1, u2, u3], kd_eqs=kd)
KM.kanes_equations(ForceList, BodyList)
MM = KM.mass_matrix
forcing = KM.forcing
rhs = MM.inv() * forcing
kdd = KM.kindiffdict()
rhs = rhs.subs(kdd)
assert rhs.expand() == Matrix([
(10 * u2 * u3 * r - 5 * u3**2 * r * tan(q2) + 4 * g * sin(q2)) /
(5 * r), -2 * u1 * u3 / 3, u1 * (-2 * u2 + u3 * tan(q2))
]).expand()
