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Long term stability of N-body simulations: the case of Trappist-1
Conserving first integrals via manifold projection
Box control in satellite Formation Flying
Comparing coordinate systems
Inverting Kepler’s equation in ODEs
Planetary embryos in the inner Solar System
Mercury’s relativistic precession
Calculating transit timing variations
Introduction to the VSOP2013 planetary theory
Introduction to the ELP2000 lunar theory
Elastic tides
Lagrange propagation and the state transition matrix
Gravity-gradient stabilization
A differentiable SGP4 propagator
Working with EOP data
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torch
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heyoka.py
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The Tolman–Oppenheimer–Volkoff equations (Lindblom’s form)
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The variational equations
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heyoka.expression
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heyoka.sum
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Numerical integrators
heyoka.taylor_adaptive
heyoka.taylor_adaptive_batch
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heyoka.var_ode_sys
heyoka.var_args
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heyoka.lagrangian
heyoka.hamiltonian
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heyoka.model.sgp4_propagator_dbl
heyoka.model.sgp4_propagator_flt
heyoka.model.cart2geo
heyoka.model.nrlmsise00_tn
heyoka.model.jb08_tn
heyoka.model.fixed_centres
heyoka.model.pendulum
heyoka.model.sgp4
heyoka.model.gpe_is_deep_space
heyoka.model.sgp4_propagator
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heyoka.model.rot_icrs_fk5j2000
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heyoka.eop_data
heyoka.eop_data_row
JIT compilation
heyoka.code_model
Repository
Open issue
.rst
.pdf
heyoka.taylor_adaptive
Contents
taylor_adaptive()
heyoka.taylor_adaptive
#
heyoka.
taylor_adaptive
(
sys
,
state
=
[]
,
**
kwargs
)
#
Contents
taylor_adaptive()
