INSTINCT Code Coverage Report


Directory: src/
File: Navigation/GNSS/Satellite/Ephemeris/GalileoEphemeris.cpp
Date: 2025-02-07 16:54:41
Exec Total Coverage
Lines: 150 152 98.7%
Functions: 6 7 85.7%
Branches: 54 86 62.8%

Line Branch Exec Source
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 "GalileoEphemeris.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 28 GalileoEphemeris::GalileoEphemeris(const InsTime& toc)
20 28 : SatNavData(SatNavData::GalileoEphemeris, toc) {}
21
22 1607 GalileoEphemeris::GalileoEphemeris(const InsTime& toc, const InsTime& toe,
23 const size_t& IODnav,
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 std::bitset<10>& dataSource, const double& signalAccuracy, const SvHealth& svHealth,
29 1607 const double& BGD_E1_E5a, const double& BGD_E1_E5b)
30 : SatNavData(SatNavData::GalileoEphemeris, toc),
31 1607 toc(toc),
32 1607 toe(toe),
33 1607 IODnav(IODnav),
34 1607 a(a),
35 1607 sqrt_A(sqrt_A),
36 1607 e(e),
37 1607 i_0(i_0),
38 1607 Omega_0(Omega_0),
39 1607 omega(omega),
40 1607 M_0(M_0),
41 1607 delta_n(delta_n),
42 1607 Omega_dot(Omega_dot),
43 1607 i_dot(i_dot),
44 1607 Cus(Cus),
45 1607 Cuc(Cuc),
46 1607 Cis(Cis),
47 1607 Cic(Cic),
48 1607 Crs(Crs),
49 1607 Crc(Crc),
50 1607 dataSource(dataSource),
51 1607 signalAccuracy(signalAccuracy),
52 1607 svHealth(svHealth),
53 1607 BGD_E1_E5a(BGD_E1_E5a),
54 1607 BGD_E1_E5b(BGD_E1_E5b) {}
55
56 #ifdef TESTING
57
58 7802 GalileoEphemeris::GalileoEphemeris(int32_t year, int32_t month, int32_t day, int32_t hour, int32_t minute, double second, double svClockBias, double svClockDrift, double svClockDriftRate,
59 double IODnav, double Crs, double delta_n, double M_0,
60 double Cuc, double e, double Cus, double sqrt_A,
61 double Toe, double Cic, double Omega_0, double Cis,
62 double i_0, double Crc, double omega, double Omega_dot,
63 double i_dot, double dataSource, double GALWeek, double /* spare1 */,
64 double signalAccuracy, double svHealth, double BGD_E1_E5a, double BGD_E1_E5b,
65 7802 double /* TransmissionTimeOfMessage */, double /* spare2 */, double /* spare3 */, double /* spare4 */)
66
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7802 : SatNavData(SatNavData::GalileoEphemeris, InsTime(year, month, day, hour, minute, second, GST)),
67 7802 toc(refTime),
68
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7802 toe(InsTime(0, static_cast<int32_t>(GALWeek), Toe, GST)),
69 7802 IODnav(static_cast<size_t>(IODnav)),
70 7802 a({ svClockBias, svClockDrift, svClockDriftRate }),
71 7802 sqrt_A(sqrt_A),
72 7802 e(e),
73 7802 i_0(i_0),
74 7802 Omega_0(Omega_0),
75 7802 omega(omega),
76 7802 M_0(M_0),
77 7802 delta_n(delta_n),
78 7802 Omega_dot(Omega_dot),
79 7802 i_dot(i_dot),
80 7802 Cus(Cus),
81 7802 Cuc(Cuc),
82 7802 Cis(Cis),
83 7802 Cic(Cic),
84 7802 Crs(Crs),
85 7802 Crc(Crc),
86 7802 dataSource(static_cast<uint16_t>(dataSource)),
87 7802 signalAccuracy(signalAccuracy),
88 7802 svHealth({ .E5a_DataValidityStatus = static_cast<GalileoEphemeris::SvHealth::DataValidityStatus>((static_cast<uint16_t>(svHealth) & 0b000001000) >> 3),
89 7802 .E5b_DataValidityStatus = static_cast<GalileoEphemeris::SvHealth::DataValidityStatus>((static_cast<uint16_t>(svHealth) & 0b001000000) >> 6),
90 7802 .E1B_DataValidityStatus = static_cast<GalileoEphemeris::SvHealth::DataValidityStatus>((static_cast<uint16_t>(svHealth) & 0b000000001) >> 0),
91 7802 .E5a_SignalHealthStatus = static_cast<GalileoEphemeris::SvHealth::SignalHealthStatus>((static_cast<uint16_t>(svHealth) & 0b000110000) >> 4),
92 7802 .E5b_SignalHealthStatus = static_cast<GalileoEphemeris::SvHealth::SignalHealthStatus>((static_cast<uint16_t>(svHealth) & 0b110000000) >> 7),
93 7802 .E1B_SignalHealthStatus = static_cast<GalileoEphemeris::SvHealth::SignalHealthStatus>((static_cast<uint16_t>(svHealth) & 0b000000110) >> 1) }),
94 7802 BGD_E1_E5a(BGD_E1_E5a),
95
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15604 BGD_E1_E5b(BGD_E1_E5b)
96 7802 {}
97
98 #endif
99
100 1987 Clock::Corrections GalileoEphemeris::calcClockCorrections(const InsTime& recvTime, double dist, const Frequency& freq) const
101 {
102 LOG_DATA("Calc Sat Clock corrections at receiver time {}", recvTime.toGPSweekTow());
103 // Earth gravitational constant [m³/s²] (WGS 84 value of the earth's gravitational constant for GPS user)
104 1987 const auto mu = InsConst::GAL::MU;
105 // Relativistic constant F for clock corrections [s/√m] (-2*√µ/c²)
106 1987 const auto F = InsConst::GAL::F;
107
108 LOG_DATA(" toe {} (Time of ephemeris)", toe.toGPSweekTow());
109
110 1987 const auto A = sqrt_A * sqrt_A; // Semi-major axis [m]
111 LOG_DATA(" A {} [m] (Semi-major axis)", A);
112 1987 auto n_0 = std::sqrt(mu / std::pow(A, 3)); // Computed mean motion [rad/s]
113 LOG_DATA(" n_0 {} [rad/s] (Computed mean motion)", n_0);
114 1987 auto n = n_0 + delta_n; // Corrected mean motion [rad/s]
115 LOG_DATA(" n {} [rad/s] (Corrected mean motion)", n);
116
117 // Time at transmission
118
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1987 InsTime transTime0 = recvTime - std::chrono::duration<double>(dist / InsConst::C);
119
120 1987 InsTime transTime = transTime0;
121 LOG_DATA(" Iterating Time at transmission");
122 1987 double dt_sv = 0.0;
123 1987 double clkDrift = 0.0;
124
125
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5961 for (size_t i = 0; i < 2; i++)
126 {
127 LOG_DATA(" transTime {} (Time at transmission)", transTime.toGPSweekTow());
128
129 // [s]
130
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3974 auto t_minus_toc = static_cast<double>((transTime - toc).count());
131 LOG_DATA(" transTime - toc {} [s]", t_minus_toc);
132
133 // Time difference from ephemeris reference epoch [s]
134
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3974 double t_k = static_cast<double>((transTime - toe).count());
135 LOG_DATA(" transTime - toe {} [s] (t_k = Time difference from ephemeris reference epoch)", t_k);
136
137 // Mean anomaly [rad]
138 3974 auto M_k = M_0 + n * t_k;
139 LOG_DATA(" M_k {} [s] (Mean anomaly)", M_k);
140
141 // Eccentric anomaly [rad]
142 3974 double E_k = M_k;
143 3974 double E_k_old = 0.0;
144
145
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19524 for (size_t i = 0; std::abs(E_k - E_k_old) > 1e-13 && i < 10; i++)
146 {
147 15550 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:
148 15550 E_k = M_k + e * sin(E_k);
149 }
150
151 // Relativistic correction term [s]
152 3974 double dt_r = F * e * sqrt_A * std::sin(E_k);
153 LOG_DATA(" dt_r {} [s] (Relativistic correction term)", dt_r);
154
155 // SV PRN code phase time offset [s]
156 3974 dt_sv = a[0] + a[1] * t_minus_toc + a[2] * std::pow(t_minus_toc, 2) + dt_r;
157
158 // See GAL-ICD-2.0 GAL ICD, ch. 5.1.5, p.47
159
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3974 dt_sv -= ratioFreqSquared(E01, freq, -128, -128) * (freq == E05 ? BGD_E1_E5a : BGD_E1_E5b); // TODO: Check again
160
161 LOG_DATA(" dt_sv {} [s] (SV PRN code phase time offset)", dt_sv);
162
163 // Groves ch. 9.3.1, eq. 9.78, p. 391
164 3974 clkDrift = a[1] + a[2] / 2.0 * t_minus_toc;
165
166 // Correct transmit time for the satellite clock bias
167
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3974 transTime = transTime0 - std::chrono::duration<double>(dt_sv);
168 }
169 LOG_DATA(" transTime {} (Time at transmission)", transTime.toGPSweekTow());
170
171 1987 return { .transmitTime = transTime, .bias = dt_sv, .drift = clkDrift };
172 }
173
174 3655 Orbit::PosVelAccel GalileoEphemeris::calcSatelliteData(const InsTime& transTime, Orbit::Calc calc) const
175 {
176
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3655 Eigen::Vector3d e_pos = Eigen::Vector3d::Zero();
177
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3655 Eigen::Vector3d e_vel = Eigen::Vector3d::Zero();
178
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3655 Eigen::Vector3d e_accel = Eigen::Vector3d::Zero();
179
180 LOG_DATA("Calc Sat Position at transmit time {}", transTime.toGPSweekTow());
181 // Earth gravitational constant [m³/s²] (WGS 84 value of the earth's gravitational constant for GPS user)
182 3655 const auto mu = InsConst::GAL::MU;
183 // Earth angular velocity [rad/s] (WGS 84 value of the earth's rotation rate)
184 3655 const auto Omega_e_dot = InsConst::GAL::omega_ie;
185
186 LOG_DATA(" toe {} (Time of ephemeris)", toe.toGPSweekTow());
187
188 3655 const auto A = sqrt_A * sqrt_A; // Semi-major axis [m]
189 LOG_DATA(" A {} [m] (Semi-major axis)", A);
190 3655 auto n_0 = std::sqrt(mu / std::pow(A, 3)); // Computed mean motion [rad/s]
191 LOG_DATA(" n_0 {} [rad/s] (Computed mean motion)", n_0);
192 3655 auto n = n_0 + delta_n; // Corrected mean motion [rad/s]
193 LOG_DATA(" n {} [rad/s] (Corrected mean motion)", n);
194
195 // Eccentric anomaly [rad]
196 3655 double E_k = 0.0;
197
198 // Time difference from ephemeris reference epoch [s]
199
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3655 double t_k = static_cast<double>((transTime - toe).count());
200 LOG_DATA(" t_k {} [s] (Time difference from ephemeris reference epoch)", t_k);
201
202 // Mean anomaly [rad]
203 3655 auto M_k = M_0 + n * t_k;
204 LOG_DATA(" M_k {} [s] (Mean anomaly)", M_k);
205
206 3655 E_k = M_k; // Initial Value [rad]
207 3655 double E_k_old = 0.0;
208 LOG_DATA(" Iterating E_k");
209 LOG_DATA(" E_k {} [rad] (Eccentric anomaly)", E_k);
210
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13369 for (size_t i = 0; std::abs(E_k - E_k_old) > 1e-13 && i < 10; i++)
211 {
212 9714 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:
213 9714 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)
214 LOG_DATA(" E_k {} [rad] (Eccentric anomaly)", E_k); // – Final Value (radians)
215 }
216
217 // 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)
218 // 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)
219 3655 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
220 LOG_DATA(" v_k {} [rad] (True Anomaly (unambiguous quadrant))", v_k);
221 3655 auto Phi_k = v_k + omega; // Argument of Latitude [rad]
222 LOG_DATA(" Phi_k {} [rad] (Argument of Latitude)", Phi_k);
223
224 // Second Harmonic Perturbations
225 3655 auto delta_u_k = Cus * std::sin(2 * Phi_k) + Cuc * std::cos(2 * Phi_k); // Argument of Latitude Correction [rad]
226 LOG_DATA(" delta_u_k {} [rad] (Argument of Latitude Correction)", delta_u_k);
227 3655 auto delta_r_k = Crs * std::sin(2 * Phi_k) + Crc * std::cos(2 * Phi_k); // Radius Correction [m]
228 LOG_DATA(" delta_r_k {} [m] (Radius Correction)", delta_r_k);
229 3655 auto delta_i_k = Cis * std::sin(2 * Phi_k) + Cic * std::cos(2 * Phi_k); // Inclination Correction [rad]
230 LOG_DATA(" delta_i_k {} [rad] (Inclination Correction)", delta_i_k);
231
232 3655 auto u_k = Phi_k + delta_u_k; // Corrected Argument of Latitude [rad]
233 LOG_DATA(" u_k {} [rad] (Corrected Argument of Latitude)", u_k);
234 3655 auto r_k = A * (1 - e * std::cos(E_k)) + delta_r_k; // Corrected Radius [m]
235 LOG_DATA(" r_k {} [m] (Corrected Radius)", r_k);
236 3655 auto i_k = i_0 + delta_i_k + i_dot * t_k; // Corrected Inclination [rad]
237 LOG_DATA(" i_k {} [rad] (Corrected Inclination)", i_k);
238
239 3655 auto x_k_op = r_k * std::cos(u_k); // Position in orbital plane [m]
240 LOG_DATA(" x_k_op {} [m] (Position in orbital plane)", x_k_op);
241 3655 auto y_k_op = r_k * std::sin(u_k); // Position in orbital plane [m]
242 LOG_DATA(" y_k_op {} [m] (Position in orbital plane)", y_k_op);
243
244 // Corrected longitude of ascending node [rad]
245
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3655 auto Omega_k = Omega_0 + (Omega_dot - Omega_e_dot) * t_k - Omega_e_dot * static_cast<double>(toe.toGPSweekTow().tow);
246 LOG_DATA(" Omega_k {} [rad] (Corrected longitude of ascending node)", Omega_k);
247
248 // Earth-fixed x coordinates [m]
249 3655 auto x_k = x_k_op * std::cos(Omega_k) - y_k_op * std::cos(i_k) * std::sin(Omega_k);
250 LOG_DATA(" x_k {} [m] (Earth-fixed x coordinates)", x_k);
251 // Earth-fixed y coordinates [m]
252 3655 auto y_k = x_k_op * std::sin(Omega_k) + y_k_op * std::cos(i_k) * std::cos(Omega_k);
253 LOG_DATA(" y_k {} [m] (Earth-fixed y coordinates)", y_k);
254 // Earth-fixed z coordinates [m]
255 3655 auto z_k = y_k_op * std::sin(i_k);
256 LOG_DATA(" z_k {} [m] (Earth-fixed z coordinates)", z_k);
257
258
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3655 e_pos = Eigen::Vector3d{ x_k, y_k, z_k };
259
260
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3655 if (calc & Calc_Velocity || calc & Calc_Acceleration)
261 {
262 // Eccentric Anomaly Rate [rad/s]
263 1668 auto E_k_dot = n / (1 - e * std::cos(E_k));
264 // True Anomaly Rate [rad/s]
265 1668 auto v_k_dot = E_k_dot * std::sqrt(1 - e * e) / (1 - e * std::cos(E_k));
266 // Corrected Inclination Angle Rate [rad/s]
267 1668 auto i_k_dot = i_dot + 2 * v_k_dot * (Cis * std::cos(2 * Phi_k) - Cic * std::sin(2 * Phi_k));
268 // Corrected Argument of Latitude Rate [rad/s]
269 1668 auto u_k_dot = v_k_dot + 2 * v_k_dot * (Cus * std::cos(2 * Phi_k) - Cuc * std::sin(2 * Phi_k));
270 // Corrected Radius Rate [m/s]
271 1668 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));
272 // Longitude of Ascending Node Rate [rad/s]
273 1668 auto Omega_k_dot = Omega_dot - Omega_e_dot;
274 // In-plane x velocity [m/s]
275 1668 auto vx_k_op = r_k_dot * std::cos(u_k) - r_k * u_k_dot * std::sin(u_k);
276 // In-plane y velocity [m/s]
277 1668 auto vy_k_op = r_k_dot * std::sin(u_k) + r_k * u_k_dot * std::cos(u_k);
278 // Earth-Fixed x velocity [m/s]
279 1668 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)
280 1668 - 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));
281 // Earth-Fixed y velocity [m/s]
282 1668 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)
283 1668 - 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));
284 // Earth-Fixed z velocity [m/s]
285 1668 auto vz_k = vy_k_op * std::sin(i_k) + y_k_op * i_k_dot * std::cos(i_k);
286
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1668 if (calc & Calc_Velocity)
288 {
289
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1668 e_vel = Eigen::Vector3d{ vx_k, vy_k, vz_k };
290 }
291
292
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1668 if (calc & Calc_Acceleration)
293 {
294 // Oblate Earth acceleration Factor [m/s^2]
295 834 auto F = -(3.0 / 2.0) * InsConst::GPS::J2 * (mu / std::pow(r_k, 2)) * std::pow(InsConst::GPS::R_E / r_k, 2);
296 // Earth-Fixed x acceleration [m/s^2]
297 834 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))
298 834 + 2 * vy_k * Omega_e_dot + x_k * std::pow(Omega_e_dot, 2);
299 // Earth-Fixed y acceleration [m/s^2]
300 834 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))
301 834 + 2 * vx_k * Omega_e_dot + y_k * std::pow(Omega_e_dot, 2);
302 // Earth-Fixed z acceleration [m/s^2]
303 834 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));
304
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834 e_accel = Eigen::Vector3d{ ax_k, ay_k, az_k };
306 }
307 }
308
309 return { .e_pos = e_pos,
310 .e_vel = e_vel,
311
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7310 .e_accel = e_accel };
312 }
313
314 2000 bool GalileoEphemeris::isHealthy() const
315 {
316 2000 return svHealth.E5a_DataValidityStatus == SvHealth::DataValidityStatus::NavigationDataValid
317
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1982 && svHealth.E5b_DataValidityStatus == SvHealth::DataValidityStatus::NavigationDataValid
318
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1982 && svHealth.E1B_DataValidityStatus == SvHealth::DataValidityStatus::NavigationDataValid
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1982 && svHealth.E5a_SignalHealthStatus == SvHealth::SignalHealthStatus::SignalOK
320
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1962 && svHealth.E5b_SignalHealthStatus == SvHealth::SignalHealthStatus::SignalOK
321
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3982 && svHealth.E1B_SignalHealthStatus == SvHealth::SignalHealthStatus::SignalOK;
322 }
323
324 double GalileoEphemeris::calcSatellitePositionVariance() const
325 {
326 return std::pow(signalAccuracy, 2);
327 }
328
329 } // namespace NAV
330