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//! PVT Solutions
use crate::prelude::{Filter, Vector3, SV};
use crate::solver::{FilterState, LSQState};
use crate::Error;
use std::collections::HashMap;
pub(crate) mod validator;
#[derive(Debug, Copy, Clone, Default)]
pub enum PVTSolutionType {
/// Default, complete solution with Position,
/// Velocity and Time components. Requires either
/// 4 vehicles in sight, or 3 if you're working in fixed altitude
/// (provided ahead of time).
#[default]
PositionVelocityTime,
/// Resolve Time component only. Requires 1 vehicle to resolve.
TimeOnly,
}
impl std::fmt::Display for PVTSolutionType {
/*
* Prints self
*/
fn fmt(&self, f: &mut std::fmt::Formatter) -> std::fmt::Result {
match self {
Self::PositionVelocityTime => write!(f, "PVT"),
Self::TimeOnly => write!(f, "TimeOnly"),
}
}
}
use nalgebra::base::{DMatrix, DVector, Matrix3, Matrix4, MatrixXx4};
use nyx::cosmic::SPEED_OF_LIGHT;
#[cfg(feature = "serde")]
use serde::{Deserialize, Serialize};
/// Modeled (estimated) or measured Time Delay.
#[derive(Debug, Copy, Clone, Default)]
#[cfg_attr(feature = "serde", derive(Serialize, Deserialize))]
pub struct PVTBias {
/// Measured delay [meters of delay]
pub measured: Option<f64>,
/// Modeled delay [meters of delay]
pub modeled: Option<f64>,
}
impl PVTBias {
/// Time Delay in [s], whether it was modeled
/// or physically measured (prefered).
pub fn value(&self) -> Option<f64> {
if self.measured.is_none() {
self.modeled
} else {
self.measured
}
}
/// Builds a measured Time Delay from a measurement in [s]
pub fn measured(measurement: f64) -> Self {
Self {
measured: Some(measurement),
modeled: None,
}
}
/// Builds a modeled Time Delay from a model in [s]
pub fn modeled(model: f64) -> Self {
Self {
modeled: Some(model),
measured: None,
}
}
}
/// Data attached to each individual SV that helped form the PVT solution.
#[derive(Debug, Copy, Clone, Default)]
#[cfg_attr(feature = "serde", derive(Serialize, Deserialize))]
pub struct PVTSVData {
/// Azimuth angle at resolution time
pub azimuth: f64,
/// Elevation angle at resolution time
pub elevation: f64,
/// Either measured or modeled Tropospheric Delay
/// that impacted L1 signal
pub tropo_bias: PVTBias,
/// Either measured or modeled Ionospheric Delay
/// that impacted L1 signal
pub iono_bias: PVTBias,
}
/// PVT Solution, always expressed as the correction to apply
/// to an Apriori / static position.
#[derive(Debug, Clone, Default)]
// #[cfg_attr(feature = "serde", derive(Serialize))]
pub struct PVTSolution {
/// Position errors (in [m] ECEF)
pub pos: Vector3<f64>,
/// Absolute Velocity (in [m/s] ECEF).
pub vel: Vector3<f64>,
/// Time correction in [s]
pub dt: f64,
/// Space Vehicles that helped form this solution
/// and data associated to each individual SV
pub sv: HashMap<SV, PVTSVData>,
// Q matrix
q: Matrix4<f64>,
}
impl PVTSolution {
/// Builds a new PVTSolution from
/// "g": the navigation matrix
/// "w": diagonal weight matrix
/// "y": the navigation vector
/// "sv": attached SV data
pub(crate) fn new(
g: MatrixXx4<f64>,
w: DMatrix<f64>,
y: DVector<f64>,
sv: HashMap<SV, PVTSVData>,
filter: Filter,
p_state: Option<FilterState>,
) -> Result<(Self, Option<FilterState>), Error> {
let (q, x, new_state) = match filter {
Filter::None => {
let g_prime = g.clone().transpose();
let q = (g_prime.clone() * g.clone())
.try_inverse()
.ok_or(Error::MatrixInversionError)?;
let p = (g_prime.clone() * w.clone() * g.clone())
.try_inverse()
.ok_or(Error::MatrixInversionError)?;
let x = p * (g_prime.clone() * w.clone() * y);
(q, x, None)
},
Filter::LSQ => {
if let Some(FilterState::LSQState(p_state)) = p_state {
let p_1 = p_state
.p
.try_inverse()
.ok_or(Error::CovarMatrixInversionError)?;
let g_prime = g.clone().transpose();
let q = (g_prime.clone() * g.clone())
.try_inverse()
.ok_or(Error::MatrixInversionError)?;
let p = g_prime.clone() * w.clone() * g.clone();
let p = (p_1 + p)
.try_inverse()
.ok_or(Error::CovarMatrixInversionError)?;
let x = p * (p_1 * p_state.x + (g_prime.clone() * w.clone() * y));
(q, x, Some(FilterState::LSQState(LSQState { x, p })))
} else {
let g_prime = g.clone().transpose();
let q = (g_prime.clone() * g.clone())
.try_inverse()
.ok_or(Error::MatrixInversionError)?;
let p = (g_prime.clone() * w.clone() * g.clone())
.try_inverse()
.ok_or(Error::MatrixInversionError)?;
let x = (p * g_prime.clone()) * w.clone() * y;
(q, x, Some(FilterState::LSQState(LSQState { x, p })))
}
},
Filter::KF => {
panic!("kalman filter not available yet");
//if let Some(FilterState::KfState(p_state)) = p_state {
// let g_prime = g.clone().transpose();
// let q = (g_prime.clone() * g.clone())
// .try_inverse()
// .ok_or(Error::MatrixInversionError)?;
// //let p = (g_prime.clone() * w.clone() * g.clone())
// // .try_inverse()
// // .ok_or(Error::MatrixInversionError)?;
// //
// //let x = (p * g_prime.clone()) * w.clone() * y;
// //
// //(q, x, Some(FilterState::KfState(KfState {
// // x,
// // p,
// //})))
//} else {
// return Err(Error::UninitializedKalmanFilter);
//}
},
};
let dt = x[3] / SPEED_OF_LIGHT;
if dt.is_nan() {
return Err(Error::TimeIsNan);
}
Ok((
(Self {
sv,
pos: Vector3::new(x[0], x[1], x[2]),
vel: Vector3::<f64>::default(),
dt,
q,
}),
new_state,
))
}
/// Returns list of Space Vehicles (SV) that help form this solution.
pub fn sv(&self) -> Vec<SV> {
self.sv.keys().copied().collect()
}
/// Returns Geometric Dilution of Precision of Self
pub fn gdop(&self) -> f64 {
(self.q[(0, 0)] + self.q[(1, 1)] + self.q[(2, 2)] + self.q[(3, 3)]).sqrt()
}
/// Returns Position Diultion of Precision of Self
pub fn pdop(&self) -> f64 {
(self.q[(0, 0)] + self.q[(1, 1)] + self.q[(2, 2)]).sqrt()
}
fn q_enu(&self, lat: f64, lon: f64) -> Matrix3<f64> {
let r = Matrix3::<f64>::new(
-lon.sin(),
-lon.cos() * lat.sin(),
lat.cos() * lon.cos(),
lon.cos(),
-lat.sin() * lon.sin(),
lat.cos() * lon.sin(),
0.0_f64,
lat.cos(),
lon.sin(),
);
let q_3 = Matrix3::<f64>::new(
self.q[(0, 0)],
self.q[(0, 1)],
self.q[(0, 2)],
self.q[(1, 0)],
self.q[(1, 1)],
self.q[(1, 2)],
self.q[(2, 0)],
self.q[(2, 1)],
self.q[(2, 2)],
);
r.clone().transpose() * q_3 * r
}
/// Returns Horizontal Dilution of Precision of Self
pub fn hdop(&self, lat: f64, lon: f64) -> f64 {
let q_enu = self.q_enu(lat, lon);
(q_enu[(0, 0)] + q_enu[(1, 1)]).sqrt()
}
/// Returns Vertical Dilution of Precision of Self
pub fn vdop(&self, lat: f64, lon: f64) -> f64 {
let q_enu = self.q_enu(lat, lon);
q_enu[(2, 2)].sqrt()
}
/// Returns Time Dilution of Precision of Self
pub fn tdop(&self) -> f64 {
self.q[(3, 3)].sqrt()
}
}