The goal for the solution of Kepler's Equation is to determine the eccentric anomaly accurately, given the mean anomaly and eccentricity. This study presents a new approach to solve this very well documented problem. It is found that by means of a series approximation, an angle identity, the...
Parallel Algorithm for Solving Kepler's Equation on Graphics Processing Units: Application to Analysis of Doppler Exoplanet Searches We present the results of a highly parallel Kepler equation solver using the Graphics Processing Unit (GPU) on a commercial nVidia GeForce 280GTX and the "... EB Fo...
5. Accurate Kepler equation solver without transcendental function evaluations. [D] . Pimienta-Penalver, Adonis Reinier. 2013 机译:无需先验函数评估的精确开普勒方程求解器。 6. A boundary value approach for solving three-dimensional elliptic and hyperbolic partial differential equations [O] . T. ...
Accurate Kepler equation solver without transcendental function evaluationsAdonis Pimienta PenalverJohn Crassidis
We present the results of a highly parallel Kepler equation solver using the Graphics Processing Unit (GPU) on a commercial nVidia GeForce 280GTX and the "Compute Unified Device Architecture" (CUDA) programming environment. We apply this to evaluate a goodness-of-fit statistic (e.g., ) for ...
[Abridged] We present the results of a highly parallel Kepler equation solver\nusing the Graphics Processing Unit (GPU) on a commercial nVidia GeForce 280GTX\nand the "Compute Unified Device Architecture" programming environment. We apply\nthis to evaluate a goodness-of-fit statistic (e.g., ...
An improved algorithm due tO Laguerre for the solution of Kepler's equation.Celes Mech,1986,39:199～ 211 Taff L G,Brennan T A.On solving Kepler'S equation.Celes M ech,1989,46:163～ 176 M arkley F L.Kepler equation solver.Celes Mech,1995,63:101～ 111 Jackson E Atlee.Perspectives of ...
gravitational constant; Ri(t) reflects the distance at any time t between each object Xi and the sun Xs; and ai denotes the semimajor axis of the object i elliptical orbit at time t, and it is determined by Kepler’s third law, which is described in Equation (20), in the following ...