Struct kidou::orbit::calc::models::m1::M1

pub struct M1 {}

This model uses the Plummer potential for bulge, the Miyamoto & Nagai potential for disk, and the Navarro-Frenk-White potential for halo. The values of the parameters are taken from Bajkova, Bobylev (2020, v1).

Trait Implementations

impl Model for M1

fn phi(&self, r: F, z: F) -> F

Calculate the value of the Galactic potential $ \Phi(R, Z) $ $[ 100 \, \text{km}^2 \, \text{s}^{-2} ]$

fn phi_dr(&self, r: F, z: F) -> F

Calculate the value of $ \partial \Phi(R, Z) / \partial R $ $[ 100 \, \text{km} \, \text{s}^{-2} ]$

fn phi_dz(&self, r: F, z: F) -> F

Calculate the value of $ \partial \Phi(R, Z) / \partial Z $ $[ 100 \, \text{km} \, \text{s}^{-2} ]$