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1 | // This file is part of INSTINCT, the INS Toolkit for Integrated | ||
2 | // Navigation Concepts and Training by the Institute of Navigation of | ||
3 | // the University of Stuttgart, Germany. | ||
4 | // | ||
5 | // This Source Code Form is subject to the terms of the Mozilla Public | ||
6 | // License, v. 2.0. If a copy of the MPL was not distributed with this | ||
7 | // file, You can obtain one at https://mozilla.org/MPL/2.0/. | ||
8 | |||
9 | #include "GPSEphemeris.hpp" | ||
10 | |||
11 | #include "Navigation/Constants.hpp" | ||
12 | #include "Navigation/GNSS/Functions.hpp" | ||
13 | |||
14 | #include "util/Logger.hpp" | ||
15 | |||
16 | namespace NAV | ||
17 | { | ||
18 | |||
19 | 19 | GPSEphemeris::GPSEphemeris(const InsTime& toc) | |
20 | 19 | : SatNavData(SatNavData::GPSEphemeris, toc) {} | |
21 | |||
22 | 1173 | GPSEphemeris::GPSEphemeris(const InsTime& toc, const InsTime& toe, | |
23 | const size_t& IODE, const size_t& IODC, | ||
24 | const std::array<double, 3>& a, | ||
25 | const double& sqrt_A, const double& e, const double& i_0, const double& Omega_0, const double& omega, const double& M_0, | ||
26 | const double& delta_n, const double& Omega_dot, const double& i_dot, const double& Cus, const double& Cuc, | ||
27 | const double& Cis, const double& Cic, const double& Crs, const double& Crc, | ||
28 | const double& svAccuracy, uint8_t svHealth, | ||
29 | uint8_t L2ChannelCodes, bool L2DataFlagPCode, | ||
30 | const double& T_GD, | ||
31 | 1173 | const double& fitInterval) | |
32 | : SatNavData(SatNavData::GPSEphemeris, toc), | ||
33 | 1173 | toc(toc), | |
34 | 1173 | toe(toe), | |
35 | 1173 | IODE(IODE), | |
36 | 1173 | IODC(IODC), | |
37 | 1173 | a(a), | |
38 | 1173 | sqrt_A(sqrt_A), | |
39 | 1173 | e(e), | |
40 | 1173 | i_0(i_0), | |
41 | 1173 | Omega_0(Omega_0), | |
42 | 1173 | omega(omega), | |
43 | 1173 | M_0(M_0), | |
44 | 1173 | delta_n(delta_n), | |
45 | 1173 | Omega_dot(Omega_dot), | |
46 | 1173 | i_dot(i_dot), | |
47 | 1173 | Cus(Cus), | |
48 | 1173 | Cuc(Cuc), | |
49 | 1173 | Cis(Cis), | |
50 | 1173 | Cic(Cic), | |
51 | 1173 | Crs(Crs), | |
52 | 1173 | Crc(Crc), | |
53 | 1173 | svAccuracy(svAccuracy), | |
54 | 1173 | svHealth(svHealth), | |
55 | 1173 | L2ChannelCodes(L2ChannelCodes), | |
56 | 1173 | L2DataFlagPCode(L2DataFlagPCode), | |
57 | 1173 | T_GD(T_GD), | |
58 | 1173 | fitInterval(fitInterval) {} | |
59 | |||
60 | #ifdef TESTING | ||
61 | |||
62 | 8251 | GPSEphemeris::GPSEphemeris(int32_t year, int32_t month, int32_t day, int32_t hour, int32_t minute, double second, double svClockBias, double svClockDrift, double svClockDriftRate, | |
63 | double IODE, double Crs, double delta_n, double M_0, | ||
64 | double Cuc, double e, double Cus, double sqrt_A, | ||
65 | double Toe, double Cic, double Omega_0, double Cis, | ||
66 | double i_0, double Crc, double omega, double Omega_dot, | ||
67 | double i_dot, double L2ChannelCodes, double GPSWeek, double L2DataFlagPCode, | ||
68 | double svAccuracy, double svHealth, double T_GD, double IODC, | ||
69 | 8251 | double /* TransmissionTimeOfMessage */, double fitInterval, double /* spare1 */, double /* spare2 */) | |
70 |
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8251 | : SatNavData(SatNavData::GPSEphemeris, InsTime(year, month, day, hour, minute, second, SatelliteSystem(GPS).getTimeSystem())), |
71 | 8251 | toc(refTime), | |
72 |
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8251 | toe(InsTime(0, static_cast<int32_t>(GPSWeek), Toe, SatelliteSystem(GPS).getTimeSystem())), |
73 | 8251 | IODE(static_cast<size_t>(IODE)), | |
74 | 8251 | IODC(static_cast<size_t>(IODC)), | |
75 | 8251 | a({ svClockBias, svClockDrift, svClockDriftRate }), | |
76 | 8251 | sqrt_A(sqrt_A), | |
77 | 8251 | e(e), | |
78 | 8251 | i_0(i_0), | |
79 | 8251 | Omega_0(Omega_0), | |
80 | 8251 | omega(omega), | |
81 | 8251 | M_0(M_0), | |
82 | 8251 | delta_n(delta_n), | |
83 | 8251 | Omega_dot(Omega_dot), | |
84 | 8251 | i_dot(i_dot), | |
85 | 8251 | Cus(Cus), | |
86 | 8251 | Cuc(Cuc), | |
87 | 8251 | Cis(Cis), | |
88 | 8251 | Cic(Cic), | |
89 | 8251 | Crs(Crs), | |
90 | 8251 | Crc(Crc), | |
91 | 8251 | svAccuracy(svAccuracy), | |
92 | 8251 | svHealth(static_cast<uint8_t>(svHealth)), | |
93 | 8251 | L2ChannelCodes(static_cast<uint8_t>(L2ChannelCodes)), | |
94 | 8251 | L2DataFlagPCode(static_cast<bool>(L2DataFlagPCode)), | |
95 | 8251 | T_GD(T_GD), | |
96 |
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16502 | fitInterval(fitInterval) |
97 | 8251 | {} | |
98 | |||
99 | #endif | ||
100 | |||
101 | 43417 | Clock::Corrections GPSEphemeris::calcClockCorrections(const InsTime& recvTime, double dist, const Frequency& freq) const | |
102 | { | ||
103 | LOG_DATA("Calc Sat Clock corrections at receiver time {}", recvTime.toGPSweekTow()); | ||
104 | // Earth gravitational constant [m³/s²] (WGS 84 value of the earth's gravitational constant for GPS user) | ||
105 | 43417 | const auto mu = InsConst::GPS::MU; | |
106 | // Relativistic constant F for clock corrections [s/√m] (-2*√µ/c²) | ||
107 | 43417 | const auto F = InsConst::GPS::F; | |
108 | |||
109 | LOG_DATA(" toe {} [{}] (Time of ephemeris)", toe.toGPSweekTow(), toe.toYMDHMS(GPST)); | ||
110 | |||
111 | 43417 | const auto A = sqrt_A * sqrt_A; // Semi-major axis [m] | |
112 | LOG_DATA(" A {} [m] (Semi-major axis)", A); | ||
113 | 43417 | auto n_0 = std::sqrt(mu / std::pow(A, 3)); // Computed mean motion [rad/s] | |
114 | LOG_DATA(" n_0 {} [rad/s] (Computed mean motion)", n_0); | ||
115 | 43417 | auto n = n_0 + delta_n; // Corrected mean motion [rad/s] | |
116 | LOG_DATA(" n {} [rad/s] (Corrected mean motion)", n); | ||
117 | |||
118 | // Time at transmission | ||
119 |
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43417 | InsTime transTime0 = recvTime - std::chrono::duration<double>(dist / InsConst::C); |
120 | |||
121 | 43417 | InsTime transTime = transTime0; | |
122 | LOG_DATA(" Iterating Time at transmission"); | ||
123 | 43417 | double dt_sv = 0.0; | |
124 | 43417 | double clkDrift = 0.0; | |
125 | |||
126 |
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130251 | for (size_t i = 0; i < 2; i++) |
127 | { | ||
128 | LOG_DATA(" [{}]", i); | ||
129 | LOG_DATA(" transTime {} [{}] (Time at transmission)", transTime.toGPSweekTow(), transTime.toYMDHMS(GPST)); | ||
130 | |||
131 | // [s] | ||
132 |
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86834 | auto t_minus_toc = static_cast<double>((transTime - toc).count()); |
133 | LOG_DATA(" transTime - toc {} [s]", t_minus_toc); | ||
134 | |||
135 | // Time difference from ephemeris reference epoch [s] | ||
136 |
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86834 | double t_k = static_cast<double>((transTime - toe).count()); |
137 | LOG_DATA(" transTime - toe {} [s] (t_k = Time difference from ephemeris reference epoch)", t_k); | ||
138 | |||
139 | // Mean anomaly [rad] | ||
140 | 86834 | auto M_k = M_0 + n * t_k; | |
141 | LOG_DATA(" M_k {} [s] (Mean anomaly)", M_k); | ||
142 | |||
143 | // Eccentric anomaly [rad] | ||
144 | 86834 | double E_k = M_k; | |
145 | 86834 | double E_k_old = 0.0; | |
146 | |||
147 |
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596966 | for (size_t i = 0; std::abs(E_k - E_k_old) > 1e-13 && i < 10; i++) |
148 | { | ||
149 | 510132 | E_k_old = E_k; // Kepler’s equation ( Mk = E_k − e sin E_k ) may be solved for Eccentric anomaly (E_k) by iteration: | |
150 | 510132 | E_k = M_k + e * sin(E_k); | |
151 | } | ||
152 | |||
153 | // Relativistic correction term [s] | ||
154 | 86834 | double dt_r = F * e * sqrt_A * std::sin(E_k); | |
155 | LOG_DATA(" dt_r {} [s] (Relativistic correction term)", dt_r); | ||
156 | |||
157 | // SV PRN code phase time offset [s] | ||
158 | 86834 | dt_sv = a[0] + a[1] * t_minus_toc + a[2] * std::pow(t_minus_toc, 2) + dt_r; | |
159 | |||
160 | // See IS-GPS-200M GPS ICD L1/L2, ch. 20.3.3.3.3.2, p.99 | ||
161 | // See IS-GPS-705J GPS ICD L5, ch. 20.3.3.3.2.1, p.78 | ||
162 |
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86834 | dt_sv -= freq & (G01 | G05) ? T_GD : ratioFreqSquared(G01, freq, -128, -128) * T_GD; |
163 | |||
164 | LOG_DATA(" dt_sv {} [s] (SV PRN code phase time offset)", dt_sv); | ||
165 | |||
166 | // Groves ch. 9.3.1, eq. 9.78, p. 391 | ||
167 | 86834 | clkDrift = a[1] + a[2] / 2.0 * t_minus_toc; | |
168 | |||
169 | // Correct transmit time for the satellite clock bias | ||
170 |
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86834 | transTime = transTime0 - std::chrono::duration<double>(dt_sv); |
171 | } | ||
172 | LOG_DATA(" transTime {} [{}] (Time at transmission)", transTime.toGPSweekTow(), transTime.toYMDHMS(GPST)); | ||
173 | |||
174 | 43417 | return { .transmitTime = transTime, .bias = dt_sv, .drift = clkDrift }; | |
175 | } | ||
176 | |||
177 | 48997 | Orbit::PosVelAccel GPSEphemeris::calcSatelliteData(const InsTime& transTime, Orbit::Calc calc) const | |
178 | { | ||
179 |
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48997 | Eigen::Vector3d e_pos = Eigen::Vector3d::Zero(); |
180 |
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48997 | Eigen::Vector3d e_vel = Eigen::Vector3d::Zero(); |
181 |
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48997 | Eigen::Vector3d e_accel = Eigen::Vector3d::Zero(); |
182 | |||
183 | LOG_DATA("Calc Sat Position at transmit time {}", transTime.toGPSweekTow()); | ||
184 | // Earth gravitational constant [m³/s²] (WGS 84 value of the earth's gravitational constant for GPS user) | ||
185 | 48997 | const auto mu = InsConst::GPS::MU; | |
186 | // Earth angular velocity [rad/s] (WGS 84 value of the earth's rotation rate) | ||
187 | 48997 | const auto Omega_e_dot = InsConst::GPS::omega_ie; | |
188 | |||
189 | LOG_DATA(" toe {} (Time of ephemeris)", toe.toGPSweekTow()); | ||
190 | |||
191 | 48997 | const auto A = sqrt_A * sqrt_A; // Semi-major axis [m] | |
192 | LOG_DATA(" A {} [m] (Semi-major axis)", A); | ||
193 | 48997 | auto n_0 = std::sqrt(mu / std::pow(A, 3)); // Computed mean motion [rad/s] | |
194 | LOG_DATA(" n_0 {} [rad/s] (Computed mean motion)", n_0); | ||
195 | 48997 | auto n = n_0 + delta_n; // Corrected mean motion [rad/s] | |
196 | LOG_DATA(" n {} [rad/s] (Corrected mean motion)", n); | ||
197 | |||
198 | // Eccentric anomaly [rad] | ||
199 | 48997 | double E_k = 0.0; | |
200 | |||
201 | // Time difference from ephemeris reference epoch [s] | ||
202 |
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48997 | double t_k = static_cast<double>((transTime - toe).count()); |
203 | LOG_DATA(" t_k {} [s] (Time difference from ephemeris reference epoch)", t_k); | ||
204 | |||
205 | // Mean anomaly [rad] | ||
206 | 48997 | auto M_k = M_0 + n * t_k; | |
207 | LOG_DATA(" M_k {} [s] (Mean anomaly)", M_k); | ||
208 | |||
209 | 48997 | E_k = M_k; // Initial Value [rad] | |
210 | 48997 | double E_k_old = 0.0; | |
211 | LOG_DATA(" Iterating E_k"); | ||
212 | LOG_DATA(" E_k {} [rad] (Eccentric anomaly)", E_k); | ||
213 |
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198482 | for (size_t i = 0; std::abs(E_k - E_k_old) > 1e-13 && i < 10; i++) |
214 | { | ||
215 | 149485 | E_k_old = E_k; // Kepler’s equation ( Mk = E_k − e sin E_k ) may be solved for Eccentric anomaly (E_k) by iteration: | |
216 | 149485 | E_k = E_k + (M_k - E_k + e * std::sin(E_k)) / (1 - e * std::cos(E_k)); // - Refined Value, minimum of three iterations, (j=1,2,3) | |
217 | LOG_DATA(" E_k {} [rad] (Eccentric anomaly)", E_k); // - Final Value (radians) | ||
218 | } | ||
219 | |||
220 | // auto v_k = 2.0 * std::atan(std::sqrt((1.0 + e) / (1.0 - e)) * std::tan(E_k / 2.0)); // True Anomaly (unambiguous quadrant) [rad] (GPS ICD algorithm) | ||
221 | // auto v_k = std::atan2(std::sqrt(1 - e * e) * std::sin(E_k) / (1 - e * std::cos(E_k)), (std::cos(E_k) - e) / (1 - e * std::cos(E_k))); // True Anomaly [rad] (GALILEO ICD algorithm) | ||
222 | 48997 | auto v_k = std::atan2(std::sqrt(1 - e * e) * std::sin(E_k), (std::cos(E_k) - e)); // True Anomaly [rad] // simplified, since the denominators cancel out | |
223 | LOG_DATA(" v_k {} [rad] (True Anomaly (unambiguous quadrant))", v_k); | ||
224 | 48997 | auto Phi_k = v_k + omega; // Argument of Latitude [rad] | |
225 | LOG_DATA(" Phi_k {} [rad] (Argument of Latitude)", Phi_k); | ||
226 | |||
227 | // Second Harmonic Perturbations | ||
228 | 48997 | auto delta_u_k = Cus * std::sin(2 * Phi_k) + Cuc * std::cos(2 * Phi_k); // Argument of Latitude Correction [rad] | |
229 | LOG_DATA(" delta_u_k {} [rad] (Argument of Latitude Correction)", delta_u_k); | ||
230 | 48997 | auto delta_r_k = Crs * std::sin(2 * Phi_k) + Crc * std::cos(2 * Phi_k); // Radius Correction [m] | |
231 | LOG_DATA(" delta_r_k {} [m] (Radius Correction)", delta_r_k); | ||
232 | 48997 | auto delta_i_k = Cis * std::sin(2 * Phi_k) + Cic * std::cos(2 * Phi_k); // Inclination Correction [rad] | |
233 | LOG_DATA(" delta_i_k {} [rad] (Inclination Correction)", delta_i_k); | ||
234 | |||
235 | 48997 | auto u_k = Phi_k + delta_u_k; // Corrected Argument of Latitude [rad] | |
236 | LOG_DATA(" u_k {} [rad] (Corrected Argument of Latitude)", u_k); | ||
237 | 48997 | auto r_k = A * (1 - e * std::cos(E_k)) + delta_r_k; // Corrected Radius [m] | |
238 | LOG_DATA(" r_k {} [m] (Corrected Radius)", r_k); | ||
239 | 48997 | auto i_k = i_0 + delta_i_k + i_dot * t_k; // Corrected Inclination [rad] | |
240 | LOG_DATA(" i_k {} [rad] (Corrected Inclination)", i_k); | ||
241 | |||
242 | 48997 | auto x_k_op = r_k * std::cos(u_k); // Position in orbital plane [m] | |
243 | LOG_DATA(" x_k_op {} [m] (Position in orbital plane)", x_k_op); | ||
244 | 48997 | auto y_k_op = r_k * std::sin(u_k); // Position in orbital plane [m] | |
245 | LOG_DATA(" y_k_op {} [m] (Position in orbital plane)", y_k_op); | ||
246 | |||
247 | // Corrected longitude of ascending node [rad] | ||
248 |
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48997 | auto Omega_k = Omega_0 + (Omega_dot - Omega_e_dot) * t_k - Omega_e_dot * static_cast<double>(toe.toGPSweekTow().tow); |
249 | LOG_DATA(" Omega_k {} [rad] (Corrected longitude of ascending node)", Omega_k); | ||
250 | |||
251 | // Earth-fixed x coordinates [m] | ||
252 | 48997 | auto x_k = x_k_op * std::cos(Omega_k) - y_k_op * std::cos(i_k) * std::sin(Omega_k); | |
253 | LOG_DATA(" x_k {} [m] (Earth-fixed x coordinates)", x_k); | ||
254 | // Earth-fixed y coordinates [m] | ||
255 | 48997 | auto y_k = x_k_op * std::sin(Omega_k) + y_k_op * std::cos(i_k) * std::cos(Omega_k); | |
256 | LOG_DATA(" y_k {} [m] (Earth-fixed y coordinates)", y_k); | ||
257 | // Earth-fixed z coordinates [m] | ||
258 | 48997 | auto z_k = y_k_op * std::sin(i_k); | |
259 | LOG_DATA(" z_k {} [m] (Earth-fixed z coordinates)", z_k); | ||
260 | |||
261 |
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48997 | e_pos = Eigen::Vector3d{ x_k, y_k, z_k }; |
262 | |||
263 |
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48997 | if (calc & Calc_Velocity || calc & Calc_Acceleration) |
264 | { | ||
265 | // Eccentric Anomaly Rate [rad/s] | ||
266 | 41118 | auto E_k_dot = n / (1 - e * std::cos(E_k)); | |
267 | // True Anomaly Rate [rad/s] | ||
268 | 41118 | auto v_k_dot = E_k_dot * std::sqrt(1 - e * e) / (1 - e * std::cos(E_k)); | |
269 | // Corrected Inclination Angle Rate [rad/s] | ||
270 | 41118 | auto i_k_dot = i_dot + 2 * v_k_dot * (Cis * std::cos(2 * Phi_k) - Cic * std::sin(2 * Phi_k)); | |
271 | // Corrected Argument of Latitude Rate [rad/s] | ||
272 | 41118 | auto u_k_dot = v_k_dot + 2 * v_k_dot * (Cus * std::cos(2 * Phi_k) - Cuc * std::sin(2 * Phi_k)); | |
273 | // Corrected Radius Rate [m/s] | ||
274 | 41118 | auto r_k_dot = e * A * E_k_dot * std::sin(E_k) + 2 * v_k_dot * (Crs * std::cos(2 * Phi_k) - Crc * std::sin(2 * Phi_k)); | |
275 | // Longitude of Ascending Node Rate [rad/s] | ||
276 | 41118 | auto Omega_k_dot = Omega_dot - Omega_e_dot; | |
277 | // In-plane x velocity [m/s] | ||
278 | 41118 | auto vx_k_op = r_k_dot * std::cos(u_k) - r_k * u_k_dot * std::sin(u_k); | |
279 | // In-plane y velocity [m/s] | ||
280 | 41118 | auto vy_k_op = r_k_dot * std::sin(u_k) + r_k * u_k_dot * std::cos(u_k); | |
281 | // Earth-Fixed x velocity [m/s] | ||
282 | 41118 | auto vx_k = -x_k_op * Omega_k_dot * std::sin(Omega_k) + vx_k_op * std::cos(Omega_k) - vy_k_op * std::sin(Omega_k) * std::cos(i_k) | |
283 | 41118 | - y_k_op * (Omega_k_dot * std::cos(Omega_k) * std::cos(i_k) - i_k_dot * std::sin(Omega_k) * std::sin(i_k)); | |
284 | // Earth-Fixed y velocity [m/s] | ||
285 | 41118 | auto vy_k = x_k_op * Omega_k_dot * std::cos(Omega_k) + vx_k_op * std::sin(Omega_k) + vy_k_op * std::cos(Omega_k) * std::cos(i_k) | |
286 | 41118 | - y_k_op * (Omega_k_dot * std::sin(Omega_k) * std::cos(i_k) + i_k_dot * std::cos(Omega_k) * std::sin(i_k)); | |
287 | // Earth-Fixed z velocity [m/s] | ||
288 | 41118 | auto vz_k = vy_k_op * std::sin(i_k) + y_k_op * i_k_dot * std::cos(i_k); | |
289 | |||
290 |
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41118 | if (calc & Calc_Velocity) |
291 | { | ||
292 |
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41118 | e_vel = Eigen::Vector3d{ vx_k, vy_k, vz_k }; |
293 | } | ||
294 | |||
295 |
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41118 | if (calc & Calc_Acceleration) |
296 | { | ||
297 | // Oblate Earth acceleration Factor [m/s^2] | ||
298 | 2790 | auto F = -(3.0 / 2.0) * InsConst::GPS::J2 * (mu / std::pow(r_k, 2)) * std::pow(InsConst::GPS::R_E / r_k, 2); | |
299 | // Earth-Fixed x acceleration [m/s^2] | ||
300 | 2790 | auto ax_k = -mu * (x_k / std::pow(r_k, 3)) + F * ((1.0 - 5.0 * std::pow(z_k / r_k, 2)) * (x_k / r_k)) | |
301 | 2790 | + 2 * vy_k * Omega_e_dot + x_k * std::pow(Omega_e_dot, 2); | |
302 | // Earth-Fixed y acceleration [m/s^2] | ||
303 | 2790 | auto ay_k = -mu * (y_k / std::pow(r_k, 3)) + F * ((1.0 - 5.0 * std::pow(z_k / r_k, 2)) * (y_k / r_k)) | |
304 | 2790 | + 2 * vx_k * Omega_e_dot + y_k * std::pow(Omega_e_dot, 2); | |
305 | // Earth-Fixed z acceleration [m/s^2] | ||
306 | 2790 | auto az_k = -mu * (z_k / std::pow(r_k, 3)) + F * ((3.0 - 5.0 * std::pow(z_k / r_k, 2)) * (z_k / r_k)); | |
307 | |||
308 |
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2790 | e_accel = Eigen::Vector3d{ ax_k, ay_k, az_k }; |
309 | } | ||
310 | } | ||
311 | |||
312 | return { .e_pos = e_pos, | ||
313 | .e_vel = e_vel, | ||
314 |
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97994 | .e_accel = e_accel }; |
315 | } | ||
316 | |||
317 | 43392 | bool GPSEphemeris::isHealthy() const | |
318 | { | ||
319 | 43392 | return svHealth == 0; | |
320 | } | ||
321 | |||
322 | 34903 | double GPSEphemeris::calcSatellitePositionVariance() const | |
323 | { | ||
324 | 34903 | return std::pow(svAccuracy, 2); | |
325 | } | ||
326 | |||
327 | } // namespace NAV | ||
328 |