brahe 1.4.0

Brahe is a modern satellite dynamics library for research and engineering applications designed to be easy-to-learn, high-performance, and quick-to-deploy. The north-star of the development is enabling users to solve meaningful problems and answer questions quickly, easily, and correctly.
Documentation
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
141
142
143
144
145
146
147
148
149
150
151
152
153
154
155
156
157
158
159
160
161
162
163
164
165
166
167
168
169
170
171
172
173
174
175
176
177
178
179
180
181
182
183
184
185
186
187
188
189
190
191
192
193
194
195
196
197
198
199
200
201
202
203
204
205
206
207
208
209
210
211
212
213
214
215
216
217
218
219
220
221
222
223
224
225
226
227
228
229
230
231
232
233
234
235
236
237
238
239
240
241
242
243
244
245
246
247
248
249
250
251
252
253
254
255
256
257
258
259
260
261
262
263
264
265
266
267
268
269
270
271
272
273
274
275
276
277
278
279
280
281
282
283
284
285
286
287
288
289
290
291
292
293
294
295
296
297
298
299
300
301
302
303
304
305
306
307
308
309
310
311
312
313
314
315
316
317
318
319
320
321
322
323
324
325
326
327
328
329
330
331
332
333
334
335
336
337
338
339
340
341
342
343
344
345
346
347
348
349
350
351
352
353
354
355
356
357
358
359
360
361
362
363
364
365
366
367
368
369
370
371
372
373
374
375
376
377
378
379
380
381
382
383
384
385
386
387
388
389
390
391
392
393
394
395
396
397
398
399
400
401
402
403
404
405
406
407
408
409
410
411
412
413
414
415
416
417
418
419
420
421
422
423
424
425
426
427
428
429
430
431
432
433
434
435
436
437
438
439
440
441
442
443
444
445
446
447
448
449
450
451
452
453
454
455
456
457
458
459
460
461
462
463
464
465
466
467
468
469
470
471
472
473
474
475
476
477
478
479
480
481
482
483
484
485
486
487
488
489
490
491
492
493
494
495
496
497
498
499
500
501
502
503
504
505
506
507
508
509
510
511
512
513
514
515
516
517
518
519
520
521
522
523
524
525
526
527
528
529
530
531
532
533
534
535
536
537
538
539
540
541
542
543
544
545
546
547
548
549
550
551
552
553
554
555
556
557
558
559
560
561
562
563
564
565
566
567
568
569
570
571
572
573
574
575
576
577
578
579
580
581
582
583
584
585
586
587
588
589
590
591
592
593
594
595
596
597
598
599
600
601
602
603
604
605
606
607
608
609
610
611
612
613
614
615
616
617
618
619
620
621
622
623
624
625
626
627
628
629
630
631
632
633
634
635
636
637
638
639
640
641
642
643
644
645
646
647
648
649
650
651
652
653
654
655
656
657
658
659
660
661
662
663
664
665
666
667
668
669
670
671
672
673
674
675
676
677
678
679
680
681
682
683
684
685
686
687
688
689
690
691
692
693
694
695
696
697
698
699
700
701
702
703
704
705
706
707
708
709
710
711
712
713
714
715
716
717
718
719
720
721
722
723
724
725
726
727
728
729
730
731
732
733
734
735
736
737
738
739
740
741
742
743
744
745
746
747
748
749
750
751
752
753
754
755
756
757
758
759
760
761
762
763
764
765
766
767
768
769
770
771
772
773
774
775
776
777
778
779
780
781
782
783
784
785
786
787
788
789
790
791
792
793
794
795
796
797
798
799
800
801
802
803
804
805
806
807
808
809
810
811
812
813
814
815
816
817
818
819
820
821
822
823
824
825
826
827
828
829
830
831
832
833
834
835
836
837
838
839
840
841
842
843
844
845
846
847
848
849
850
851
852
853
854
855
856
857
858
859
860
861
862
/*!
 * Provides topocentric coordiante transformations.
 */

use std::f64::consts::PI;

use nalgebra::Vector3;

use crate::math::SMatrix3;

use crate::constants;
use crate::constants::AngleFormat;
use crate::coordinates::coordinate_types::EllipsoidalConversionType;
use crate::coordinates::geocentric::position_ecef_to_geocentric;
use crate::coordinates::geodetic::position_ecef_to_geodetic;

/// Compute the rotation matrix from body-fixed to East-North-Zenith (ENZ)
/// Cartesian coordinates for a given set of coordinates on an ellipsoidal body.
/// The ellipsoidal coordinates can either be geodetic or geocentric.
///
/// # Args:
/// - `x_ellipsoid`: Ellipsoidal coordinates.  Expected format (lon, lat, alt)
/// - `angle_format`: Format for angular coordinates (Radians or Degrees)
///
/// # Returns:
/// - `E`: Earth-fixed to Topocentric rotation matrix
///
/// # Examples:
/// ```
/// use brahe::constants::DEGREES;
/// use brahe::vector3_from_array;
/// use brahe::coordinates::*;
///
/// let x_geo = vector3_from_array([30.0, 60.0, 0.0]);
/// let rot = rotation_ellipsoid_to_enz(x_geo, DEGREES);
/// ```
pub fn rotation_ellipsoid_to_enz(x_ellipsoid: Vector3<f64>, angle_format: AngleFormat) -> SMatrix3 {
    let lon = match angle_format {
        AngleFormat::Degrees => x_ellipsoid[0] * constants::DEG2RAD,
        AngleFormat::Radians => x_ellipsoid[0],
    };
    let lat = match angle_format {
        AngleFormat::Degrees => x_ellipsoid[1] * constants::DEG2RAD,
        AngleFormat::Radians => x_ellipsoid[1],
    };

    // Construct Rotation matrix
    SMatrix3::new(
        -lon.sin(),
        lon.cos(),
        0.0, // E-base vector
        -lat.sin() * lon.cos(),
        -lat.sin() * lon.sin(),
        lat.cos(), // N-base vector
        lat.cos() * lon.cos(),
        lat.cos() * lon.sin(),
        lat.sin(), // Z-base vector
    )
}

/// Compute the rotation matrix from East-North-Zenith (ENZ) to body-fixed
/// Cartesian coordinates for a given set of coordinates on an ellipsoidal body.
/// The ellipsoidal coordinates can either be geodetic or geocentric.
///
/// # Args:
/// - `x_ellipsoid`: Ellipsoidal coordinates.  Expected format (lon, lat, alt)
/// - `angle_format`: Format for angular coordinates (Radians or Degrees)
///
/// # Returns:
/// - `E`: Topocentric to Earth-fixed rotation matrix
///
/// # Examples:
/// ```
/// use brahe::constants::DEGREES;
/// use brahe::vector3_from_array;
/// use brahe::coordinates::*;
///
/// let x_geo = vector3_from_array([30.0, 60.0, 0.0]);
/// let rot = rotation_enz_to_ellipsoid(x_geo, DEGREES);
/// ```
pub fn rotation_enz_to_ellipsoid(x_ellipsoid: Vector3<f64>, angle_format: AngleFormat) -> SMatrix3 {
    rotation_ellipsoid_to_enz(x_ellipsoid, angle_format).transpose()
}

/// Computes the relative state in East-North-Zenith (ENZ) coordinates for a target
/// object in the ECEF frame with respect to a fixed location (station) also in
/// the ECEF frame.
///
/// # Args:
/// - `location_ecef`: Cartesian position of the observing station in the ECEF frame.
/// - `x_ecef`: Cartesian position of the observed object in the ECEF frame
/// - `conversion_type`: Type of conversion to apply for computing the topocentric frame based on station coordinates.
///
/// # Returns:
/// - `r_rel`: Relative position of object in ENZ coordinates based on the station location.
///
/// # Examples:
/// ```
/// use brahe::constants::R_EARTH;
/// use brahe::vector3_from_array;
/// use brahe::coordinates::*;
///
/// let x_station = vector3_from_array([R_EARTH, 0.0, 0.0]);
/// let x_sat = vector3_from_array([R_EARTH + 500.0e3, 0.0, 0.0]);
///
/// let r_enz = relative_position_ecef_to_enz(
///     x_station, x_sat, EllipsoidalConversionType::Geocentric
/// );
/// ```
#[allow(non_snake_case)]
pub fn relative_position_ecef_to_enz(
    location_ecef: Vector3<f64>,
    r_ecef: Vector3<f64>,
    conversion_type: EllipsoidalConversionType,
) -> Vector3<f64> {
    // Create ENZ rotation matrix
    let E = match conversion_type {
        EllipsoidalConversionType::Geocentric => rotation_ellipsoid_to_enz(
            position_ecef_to_geocentric(location_ecef, AngleFormat::Radians),
            AngleFormat::Radians,
        ),
        EllipsoidalConversionType::Geodetic => rotation_ellipsoid_to_enz(
            position_ecef_to_geodetic(location_ecef, AngleFormat::Radians),
            AngleFormat::Radians,
        ),
    };

    // Compute range transformation
    let r = r_ecef - location_ecef;
    E * r
}

/// Computes the absolute Earth-fixed coordinates for an object given its relative
/// position in East-North-Zenith (ENZ) coordinates and the Cartesian body-fixed
/// coordinates of the observing location/station.
///
/// # Args:
/// - `location_ecef`: Cartesian position of the observing station in the ECEF frame.
/// - `r_rel`: Relative position of object in ENZ coordinates based on the station location.
/// - `conversion_type`: Type of conversion to apply for computing the topocentric frame based on station coordinates.
///
/// # Returns:
/// - `r_ecef`: Cartesian position of the observed object in the ECEF frame
///
/// # Examples:
/// ```
/// use brahe::constants::R_EARTH;
/// use brahe::vector3_from_array;
/// use brahe::coordinates::*;
///
/// let x_station = vector3_from_array([R_EARTH, 0.0, 0.0]);
/// let r_enz = vector3_from_array([0.0, 0.0, 500.0e3]);
///
/// let r_ecef = relative_position_enz_to_ecef(
///     x_station, r_enz, EllipsoidalConversionType::Geocentric
/// );
/// ```
#[allow(non_snake_case)]
pub fn relative_position_enz_to_ecef(
    location_ecef: Vector3<f64>,
    r_enz: Vector3<f64>,
    conversion_type: EllipsoidalConversionType,
) -> Vector3<f64> {
    // Create ENZ rotation matrix
    let Et = match conversion_type {
        EllipsoidalConversionType::Geocentric => rotation_enz_to_ellipsoid(
            position_ecef_to_geocentric(location_ecef, AngleFormat::Radians),
            AngleFormat::Radians,
        ),
        EllipsoidalConversionType::Geodetic => rotation_enz_to_ellipsoid(
            position_ecef_to_geodetic(location_ecef, AngleFormat::Radians),
            AngleFormat::Radians,
        ),
    };

    // Compute range transformation
    let r = r_enz;
    location_ecef + Et * r
}

/// Compute the rotation matrix from body-fixed to South-East-Zenith (SEZ)
/// Cartesian coordinates for a given set of coordinates on an ellipsoidal body.
/// The ellipsoidal coordinates can either be geodetic or geocentric.
///
/// # Args:
/// - `x_ellipsoid`: Ellipsoidal coordinates.  Expected format (lon, lat, alt)
/// - `angle_format`: Format for angular coordinates (Radians or Degrees)
///
/// # Returns:
/// - `E`: Earth-fixed to Topocentric rotation matrix
///
/// # Examples:
/// ```
/// use brahe::constants::DEGREES;
/// use brahe::vector3_from_array;
/// use brahe::coordinates::*;
///
/// let x_geo = vector3_from_array([30.0, 60.0, 0.0]);
/// let rot = rotation_sez_to_ellipsoid(x_geo, DEGREES);
/// ```
pub fn rotation_ellipsoid_to_sez(x_ellipsoid: Vector3<f64>, angle_format: AngleFormat) -> SMatrix3 {
    let lon = match angle_format {
        AngleFormat::Degrees => x_ellipsoid[0] * constants::DEG2RAD,
        AngleFormat::Radians => x_ellipsoid[0],
    };
    let lat = match angle_format {
        AngleFormat::Degrees => x_ellipsoid[1] * constants::DEG2RAD,
        AngleFormat::Radians => x_ellipsoid[1],
    };

    // Construct Rotation matrix
    SMatrix3::new(
        lat.sin() * lon.cos(),
        lat.sin() * lon.sin(),
        -lat.cos(), // S-base vector
        -lon.sin(),
        lon.cos(),
        0.0, // E-base vector
        lat.cos() * lon.cos(),
        lat.cos() * lon.sin(),
        lat.sin(), // Z-base vector
    )
}

/// Compute the rotation matrix from South-East-Zenith (SEZ) to body-fixed
/// Cartesian coordinates for a given set of coordinates on an ellipsoidal body.
/// The ellipsoidal coordinates can either be geodetic or geocentric.
///
/// # Args:
/// - `x_ellipsoid`: Ellipsoidal coordinates. Expected format (lon, lat, alt)
/// - `angle_format`: Format for angular coordinates (Radians or Degrees)
///
/// # Returns:
/// - `E`: Topocentric to Earth-fixed rotation matrix
///
/// # Examples:
/// ```
/// use brahe::constants::DEGREES;
/// use brahe::vector3_from_array;
/// use brahe::coordinates::*;
///
/// let x_geo = vector3_from_array([30.0, 60.0, 0.0]);
/// let rot = rotation_sez_to_ellipsoid(x_geo, DEGREES);
/// ```
pub fn rotation_sez_to_ellipsoid(x_ellipsoid: Vector3<f64>, angle_format: AngleFormat) -> SMatrix3 {
    rotation_ellipsoid_to_sez(x_ellipsoid, angle_format).transpose()
}

/// Computes the relative state in South-East-Zenith (SEZ) coordinates for a target
/// object in the ECEF frame with respect to a fixed location (station) also in
/// the ECEF frame.
///
/// # Args:
/// - `location_ecef`: Cartesian position of the observing station in the ECEF frame.
/// - `r_ecef`: Cartesian position of the observed object in the ECEF frame
/// - `conversion_type`: Type of conversion to apply for computing the topocentric frame based on station coordinates.
///
/// # Returns:
/// - `r_rel`: Relative position of object in ENZ coordinates based on the station location.
///
/// # Examples:
/// ```
/// use brahe::constants::R_EARTH;
/// use brahe::vector3_from_array;
/// use brahe::coordinates::*;
///
/// let x_station = vector3_from_array([R_EARTH, 0.0, 0.0]);
/// let x_sat = vector3_from_array([R_EARTH + 500.0e3, 0.0, 0.0]);
///
/// let r_enz = relative_position_ecef_to_enz(
///     x_station, x_sat, EllipsoidalConversionType::Geocentric
/// );
/// ```
#[allow(non_snake_case)]
pub fn relative_position_ecef_to_sez(
    location_ecef: Vector3<f64>,
    r_ecef: Vector3<f64>,
    conversion_type: EllipsoidalConversionType,
) -> Vector3<f64> {
    // Create ENZ rotation matrix
    let E = match conversion_type {
        EllipsoidalConversionType::Geocentric => rotation_ellipsoid_to_sez(
            position_ecef_to_geocentric(location_ecef, AngleFormat::Radians),
            AngleFormat::Radians,
        ),
        EllipsoidalConversionType::Geodetic => rotation_ellipsoid_to_sez(
            position_ecef_to_geodetic(location_ecef, AngleFormat::Radians),
            AngleFormat::Radians,
        ),
    };

    // Compute range transformation
    let r = r_ecef - location_ecef;
    E * r
}

/// Computes the absolute Earth-fixed coordinates for an object given its relative
/// position in East-North-Zenith (ENZ) coordinates and the Cartesian body-fixed
/// coordinates of the observing location/station.
///
/// # Args:
/// - `location_ecef`: Cartesian position of the observing station in the ECEF frame.
/// - `r_rel`: Relative position of object in ENZ coordinates based on the station location.
/// - `conversion_type`: Type of conversion to apply for computing the topocentric frame based on station coordinates.
///
/// # Returns:
/// - `r_ecef`: Cartesian position of the observed object in the ECEF frame
///
/// # Examples:
/// ```
/// use brahe::constants::R_EARTH;
/// use brahe::vector3_from_array;
/// use brahe::coordinates::*;
///
/// let x_station = vector3_from_array([R_EARTH, 0.0, 0.0]);
/// let r_sez = vector3_from_array([0.0, 0.0, 500.0e3]);
///
/// let r_ecef = relative_position_sez_to_ecef(
///     x_station, r_sez, EllipsoidalConversionType::Geocentric
/// );
/// ```
#[allow(non_snake_case)]
pub fn relative_position_sez_to_ecef(
    location_ecef: Vector3<f64>,
    x_sez: Vector3<f64>,
    conversion_type: EllipsoidalConversionType,
) -> Vector3<f64> {
    // Create SEZ rotation matrix
    let Et = match conversion_type {
        EllipsoidalConversionType::Geocentric => rotation_sez_to_ellipsoid(
            position_ecef_to_geocentric(location_ecef, AngleFormat::Radians),
            AngleFormat::Radians,
        ),
        EllipsoidalConversionType::Geodetic => rotation_sez_to_ellipsoid(
            position_ecef_to_geodetic(location_ecef, AngleFormat::Radians),
            AngleFormat::Radians,
        ),
    };

    // Compute range transformation
    let r = x_sez;
    location_ecef + Et * r
}

/// Converts East-North-Zenith topocentric coordinates of an location
/// into azimuth, elevation, and range from that same location. Azimuth is measured
/// clockwise from North.
///
/// # Args:
/// - `x_enz`: Relative Cartesian position of object to location East-North-Up coordinates. Units: (*m*)
/// - `angle_format`: Format for angular output (Radians or Degrees)
///
/// # Returns:
/// - `x_azel`: Azimuth, elevation and range. Units: (*angle*, *angle*, *m*)
///
/// # Examples:
/// ```
/// use brahe::constants::{R_EARTH, DEGREES};
/// use brahe::vector3_from_array;
/// use brahe::coordinates::*;
///
/// let x_enz = vector3_from_array([100.0, 0.0, 0.0]);
///
/// let x_azel = position_enz_to_azel(x_enz, DEGREES);
/// // x_azel = [90.0, 0.0, 100.0]
/// ```
pub fn position_enz_to_azel(x_enz: Vector3<f64>, angle_format: AngleFormat) -> Vector3<f64> {
    // Range
    let rho = x_enz.norm();

    // Elevation
    let el = x_enz[2].atan2((x_enz[0].powi(2) + x_enz[1].powi(2)).sqrt());

    // Azimuth
    let az = if el != PI / 2.0 {
        let azt = x_enz[0].atan2(x_enz[1]);

        if azt >= 0.0 { azt } else { azt + 2.0 * PI }
    } else {
        // If at peak elevation azimuth is ambiguous so define as 0.0
        0.0
    };

    match angle_format {
        AngleFormat::Degrees => Vector3::new(az * constants::RAD2DEG, el * constants::RAD2DEG, rho),
        AngleFormat::Radians => Vector3::new(az, el, rho),
    }
}

/// Converts South-East-Zenith topocentric coordinates of an location
/// into azimuth, elevation, and range from that same location. Azimuth is measured
/// clockwise from North.
///
/// # Args:
/// - `x_sez`: Relative Cartesian position of object to location South-East-Zenith coordinates. Units: (*m*)
/// - `angle_format`: Format for angular output (Radians or Degrees)
///
/// # Returns:
/// - `x_azel`: Azimuth, elevation and range. Units: (*angle*, *angle*, *m*)
///
/// # Examples:
/// ```
/// use brahe::constants::{R_EARTH, DEGREES};
/// use brahe::vector3_from_array;
/// use brahe::coordinates::*;
///
/// let x_enz = vector3_from_array([0.0, 100.0, 0.0]);
///
/// let x_azel = position_sez_to_azel(x_enz, DEGREES);
/// // x_azel = [90.0, 0.0, 100.0]
/// ```
pub fn position_sez_to_azel(x_sez: Vector3<f64>, angle_format: AngleFormat) -> Vector3<f64> {
    // Range
    let rho = x_sez.norm();

    // Elevation
    let el = x_sez[2].atan2((x_sez[0].powi(2) + x_sez[1].powi(2)).sqrt());

    // Azimuth
    let az = if el != PI / 2.0 {
        let azt = (x_sez[1]).atan2(-x_sez[0]);

        if azt >= 0.0 { azt } else { azt + 2.0 * PI }
    } else {
        // If at peak elevation azimuth is ambiguous so define as 0.0
        0.0
    };

    match angle_format {
        AngleFormat::Degrees => Vector3::new(az * constants::RAD2DEG, el * constants::RAD2DEG, rho),
        AngleFormat::Radians => Vector3::new(az, el, rho),
    }
}

#[cfg(test)]
#[cfg_attr(coverage_nightly, coverage(off))]
mod tests {
    use approx::assert_abs_diff_eq;

    use crate::constants::DEGREES;
    use crate::{R_EARTH, position_geocentric_to_ecef, position_geodetic_to_ecef};

    use super::*;

    #[test]
    fn test_rotation_ellipsoid_to_enz() {
        // Epsilon Tolerance
        let tol = f64::EPSILON;

        // Test aligned coordinates
        let x_sta = Vector3::new(0.0, 0.0, 0.0);
        let rot1 = rotation_ellipsoid_to_enz(x_sta, DEGREES);

        // ECEF input X - [1, 0, 0] - Expected output is ENZ Z-dir
        assert_abs_diff_eq!(rot1[(0, 0)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 0)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 0)], 1.0, epsilon = tol);

        // ECEF input Y - [0, 1, 0] - Expected output is ENZ E-dir
        assert_abs_diff_eq!(rot1[(0, 1)], 1.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 1)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 1)], 0.0, epsilon = tol);

        // ECEF input Z - [0, 0, 1] - Expected output is ENZ N-dir
        assert_abs_diff_eq!(rot1[(0, 2)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 2)], 1.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 2)], 0.0, epsilon = tol);

        assert_abs_diff_eq!(rot1.determinant(), 1.0, epsilon = tol);

        // Test 90 degree longitude
        let x_sta = Vector3::new(90.0, 0.0, 0.0);
        let rot1 = rotation_ellipsoid_to_enz(x_sta, DEGREES);

        // ECEF input X - [1, 0, 0] - Expected output is ENZ -E-dir
        assert_abs_diff_eq!(rot1[(0, 0)], -1.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 0)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 0)], 0.0, epsilon = tol);

        // ECEF input Y - [0, 1, 0] - Expected output is ENZ Z-dir
        assert_abs_diff_eq!(rot1[(0, 1)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 1)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 1)], 1.0, epsilon = tol);

        // ECEF input Z - [0, 0, 1] - Expected output is ENZ N-dir
        assert_abs_diff_eq!(rot1[(0, 2)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 2)], 1.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 2)], 0.0, epsilon = tol);

        assert_abs_diff_eq!(rot1.determinant(), 1.0, epsilon = tol);

        // Test 90 degree latitude
        let x_sta = Vector3::new(00.0, 90.0, 0.0);
        let rot1 = rotation_ellipsoid_to_enz(x_sta, DEGREES);

        // ECEF input X - [1, 0, 0] - Expected output is ENZ -N-dir
        assert_abs_diff_eq!(rot1[(0, 0)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 0)], -1.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 0)], 0.0, epsilon = tol);

        // ECEF input Y - [0, 1, 0] - Expected output is ENZ E-dir
        assert_abs_diff_eq!(rot1[(0, 1)], 1.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 1)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 1)], 0.0, epsilon = tol);

        // ECEF input Z - [0, 0, 1] - Expected output is ENZ Z-dir
        assert_abs_diff_eq!(rot1[(0, 2)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 2)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 2)], 1.0, epsilon = tol);

        assert_abs_diff_eq!(rot1.determinant(), 1.0, epsilon = tol);
    }

    #[test]
    fn test_rotation_enz_to_ellipsoid() {
        let tol = f64::EPSILON;

        let x_sta = Vector3::new(42.1, 53.9, 100.0);
        let rot = rotation_ellipsoid_to_enz(x_sta, DEGREES);
        let rot_t = rotation_enz_to_ellipsoid(x_sta, DEGREES);

        let r = rot * rot_t;

        // Confirm identity
        assert_abs_diff_eq!(r[(0, 0)], 1.0, epsilon = tol);
        assert_abs_diff_eq!(r[(0, 1)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r[(0, 2)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r[(1, 0)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r[(1, 1)], 1.0, epsilon = tol);
        assert_abs_diff_eq!(r[(1, 2)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r[(2, 0)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r[(2, 1)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r[(2, 2)], 1.0, epsilon = tol);
    }

    #[test]
    fn test_relative_position_ecef_to_enz() {
        let tol = f64::EPSILON;

        // 100m Overhead
        let x_sta = Vector3::new(R_EARTH, 0.0, 0.0);
        let r_ecef = Vector3::new(R_EARTH + 100.0, 0.0, 0.0);

        let r_enz =
            relative_position_ecef_to_enz(x_sta, r_ecef, EllipsoidalConversionType::Geocentric);

        assert_abs_diff_eq!(r_enz[0], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r_enz[1], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r_enz[2], 100.0, epsilon = tol);

        // 100m North
        let x_sta = Vector3::new(R_EARTH, 0.0, 0.0);
        let r_ecef = Vector3::new(R_EARTH, 0.0, 100.0);

        let r_enz =
            relative_position_ecef_to_enz(x_sta, r_ecef, EllipsoidalConversionType::Geocentric);

        assert_abs_diff_eq!(r_enz[0], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r_enz[1], 100.0, epsilon = tol);
        assert_abs_diff_eq!(r_enz[2], 0.0, epsilon = tol);

        // 100m East
        let x_sta = Vector3::new(R_EARTH, 0.0, 0.0);
        let r_ecef = Vector3::new(R_EARTH, 100.0, 0.0);

        let r_enz =
            relative_position_ecef_to_enz(x_sta, r_ecef, EllipsoidalConversionType::Geocentric);

        assert_abs_diff_eq!(r_enz[0], 100.0, epsilon = tol);
        assert_abs_diff_eq!(r_enz[1], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r_enz[2], 0.0, epsilon = tol);

        // Confirm higher latitude and longitude is (+E, +N, -Z)
        let x_sta = Vector3::new(R_EARTH, 0.0, 0.0);
        let x_geoc = Vector3::new(0.5, 0.5, 0.0);
        let r_ecef = position_geocentric_to_ecef(x_geoc, DEGREES).unwrap();

        let r_enz_geoc =
            relative_position_ecef_to_enz(x_sta, r_ecef, EllipsoidalConversionType::Geocentric);

        assert!(r_enz_geoc[0] > 0.0);
        assert!(r_enz_geoc[1] > 0.0);
        assert!(r_enz_geoc[2] < 0.0);

        // Confirm difference in geocentric and geodetic conversions
        let x_sta = Vector3::new(R_EARTH, 0.0, 0.0);
        let x_geod = Vector3::new(0.5, 0.5, 0.0);
        let r_ecef = position_geodetic_to_ecef(x_geod, DEGREES).unwrap();

        let r_enz_geod =
            relative_position_ecef_to_enz(x_sta, r_ecef, EllipsoidalConversionType::Geodetic);

        assert!(r_enz_geod[0] > 0.0);
        assert!(r_enz_geod[1] > 0.0);
        assert!(r_enz_geod[2] < 0.0);

        for i in 0..3 {
            assert_ne!(r_enz_geoc[i], r_enz_geod[i]);
        }
    }

    #[test]
    fn test_relative_position_enz_to_ecef() {
        let tol = f64::EPSILON;

        let x_sta = Vector3::new(R_EARTH, 0.0, 0.0);
        let r_enz = Vector3::new(0.0, 0.0, 100.0);

        let r_ecef =
            relative_position_enz_to_ecef(x_sta, r_enz, EllipsoidalConversionType::Geodetic);

        assert_abs_diff_eq!(r_ecef[0], R_EARTH + 100.0, epsilon = tol);
        assert_abs_diff_eq!(r_ecef[1], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r_ecef[2], 0.0, epsilon = tol);
    }

    #[test]
    fn test_rotation_ellipsoid_to_sez() {
        // Epsilon Tolerance
        let tol = f64::EPSILON;

        // Test aligned coordinates
        let x_sta = Vector3::new(0.0, 0.0, 0.0);
        let rot1 = rotation_ellipsoid_to_sez(x_sta, DEGREES);

        // ECEF input X - [1, 0, 0] - Expected output is SEZ Z-dir
        assert_abs_diff_eq!(rot1[(0, 0)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 0)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 0)], 1.0, epsilon = tol);

        // ECEF input Y - [0, 1, 0] - Expected output is SEZ E-dir
        assert_abs_diff_eq!(rot1[(0, 1)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 1)], 1.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 1)], 0.0, epsilon = tol);

        // ECEF input Z - [0, 0, 1] - Expected output is SEZ -S-dir
        assert_abs_diff_eq!(rot1[(0, 2)], -1.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 2)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 2)], 0.0, epsilon = tol);

        assert_abs_diff_eq!(rot1.determinant(), 1.0, epsilon = tol);

        // Test 90 degree longitude
        let x_sta = Vector3::new(90.0, 0.0, 0.0);
        let rot1 = rotation_ellipsoid_to_sez(x_sta, DEGREES);

        // ECEF input X - [1, 0, 0] - Expected output is SEZ -E-dir
        assert_abs_diff_eq!(rot1[(0, 0)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 0)], -1.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 0)], 0.0, epsilon = tol);

        // ECEF input Y - [0, 1, 0] - Expected output is SEZ Z-dir
        assert_abs_diff_eq!(rot1[(0, 1)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 1)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 1)], 1.0, epsilon = tol);

        // ECEF input Z - [0, 0, 1] - Expected output is SEZ -S-dir
        assert_abs_diff_eq!(rot1[(0, 2)], -1.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 2)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 2)], 0.0, epsilon = tol);

        assert_abs_diff_eq!(rot1.determinant(), 1.0, epsilon = tol);

        // Test 90 degree latitude
        let x_sta = Vector3::new(00.0, 90.0, 0.0);
        let rot1 = rotation_ellipsoid_to_sez(x_sta, DEGREES);

        // ECEF input X - [1, 0, 0] - Expected output is SEZ S-dir
        assert_abs_diff_eq!(rot1[(0, 0)], 1.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 0)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 0)], 0.0, epsilon = tol);

        // ECEF input Y - [0, 1, 0] - Expected output is SEZ E-dir
        assert_abs_diff_eq!(rot1[(0, 1)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 1)], 1.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 1)], 0.0, epsilon = tol);

        // ECEF input Z - [0, 0, 1] - Expected output is SEZ Z-dir
        assert_abs_diff_eq!(rot1[(0, 2)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(1, 2)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(rot1[(2, 2)], 1.0, epsilon = tol);

        assert_abs_diff_eq!(rot1.determinant(), 1.0, epsilon = tol);
    }

    #[test]
    fn test_rotation_sez_to_ellipsoid() {
        let tol = f64::EPSILON;

        let x_sta = Vector3::new(42.1, 53.9, 100.0);
        let rot = rotation_ellipsoid_to_sez(x_sta, DEGREES);
        let rot_t = rotation_sez_to_ellipsoid(x_sta, DEGREES);

        let r = rot * rot_t;

        // Confirm identity
        assert_abs_diff_eq!(r[(0, 0)], 1.0, epsilon = tol);
        assert_abs_diff_eq!(r[(0, 1)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r[(0, 2)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r[(1, 0)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r[(1, 1)], 1.0, epsilon = tol);
        assert_abs_diff_eq!(r[(1, 2)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r[(2, 0)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r[(2, 1)], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r[(2, 2)], 1.0, epsilon = tol);
    }

    #[test]
    fn test_relative_position_ecef_to_sez() {
        let tol = f64::EPSILON;

        // 100m Overhead
        let x_sta = Vector3::new(R_EARTH, 0.0, 0.0);
        let r_ecef = Vector3::new(R_EARTH + 100.0, 0.0, 0.0);

        let r_sez =
            relative_position_ecef_to_sez(x_sta, r_ecef, EllipsoidalConversionType::Geocentric);

        assert_abs_diff_eq!(r_sez[0], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r_sez[1], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r_sez[2], 100.0, epsilon = tol);

        // 100m North
        let x_sta = Vector3::new(R_EARTH, 0.0, 0.0);
        let r_ecef = Vector3::new(R_EARTH, 0.0, 100.0);

        let r_sez =
            relative_position_ecef_to_sez(x_sta, r_ecef, EllipsoidalConversionType::Geocentric);

        assert_abs_diff_eq!(r_sez[0], -100.0, epsilon = tol);
        assert_abs_diff_eq!(r_sez[1], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r_sez[2], 0.0, epsilon = tol);

        // 100m East
        let x_sta = Vector3::new(R_EARTH, 0.0, 0.0);
        let r_ecef = Vector3::new(R_EARTH, 100.0, 0.0);

        let r_sez =
            relative_position_ecef_to_sez(x_sta, r_ecef, EllipsoidalConversionType::Geocentric);

        assert_abs_diff_eq!(r_sez[0], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r_sez[1], 100.0, epsilon = tol);
        assert_abs_diff_eq!(r_sez[2], 0.0, epsilon = tol);

        // Confirm higher latitude and longitude is (+E, +N, -Z)
        let x_sta = Vector3::new(R_EARTH, 0.0, 0.0);
        let x_geoc = Vector3::new(0.5, 0.5, 0.0);
        let r_ecef = position_geocentric_to_ecef(x_geoc, DEGREES).unwrap();

        let r_sez_geoc =
            relative_position_ecef_to_sez(x_sta, r_ecef, EllipsoidalConversionType::Geocentric);

        assert!(r_sez_geoc[0] < 0.0);
        assert!(r_sez_geoc[1] > 0.0);
        assert!(r_sez_geoc[2] < 0.0);

        // Confirm difference in geocentric and geodetic conversions
        let x_sta = Vector3::new(R_EARTH, 0.0, 0.0);
        let x_geod = Vector3::new(0.5, 0.5, 0.0);
        let r_ecef = position_geodetic_to_ecef(x_geod, DEGREES).unwrap();

        let r_sez_geod =
            relative_position_ecef_to_sez(x_sta, r_ecef, EllipsoidalConversionType::Geodetic);

        assert!(r_sez_geod[0] < 0.0);
        assert!(r_sez_geod[1] > 0.0);
        assert!(r_sez_geod[2] < 0.0);

        for i in 0..3 {
            assert_ne!(r_sez_geoc[i], r_sez_geod[i]);
        }
    }

    #[test]
    fn test_relative_position_sez_to_ecef() {
        let tol = f64::EPSILON;

        let x_sta = Vector3::new(R_EARTH, 0.0, 0.0);
        let r_sez = Vector3::new(0.0, 0.0, 100.0);

        let r_ecef =
            relative_position_sez_to_ecef(x_sta, r_sez, EllipsoidalConversionType::Geodetic);

        assert_abs_diff_eq!(r_ecef[0], R_EARTH + 100.0, epsilon = tol);
        assert_abs_diff_eq!(r_ecef[1], 0.0, epsilon = tol);
        assert_abs_diff_eq!(r_ecef[2], 0.0, epsilon = tol);
    }

    #[test]
    fn test_position_enz_to_azel() {
        let tol = f64::EPSILON;

        // Directly above
        let r_enz = Vector3::new(0.0, 0.0, 100.0);
        let x_azel = position_enz_to_azel(r_enz, DEGREES);

        assert_abs_diff_eq!(x_azel[0], 0.0, epsilon = tol);
        assert_abs_diff_eq!(x_azel[1], 90.0, epsilon = tol);
        assert_abs_diff_eq!(x_azel[2], 100.0, epsilon = tol);

        // North
        let r_enz = Vector3::new(0.0, 100.0, 0.0);
        let x_azel = position_enz_to_azel(r_enz, DEGREES);

        assert_abs_diff_eq!(x_azel[0], 0.0, epsilon = tol);
        assert_abs_diff_eq!(x_azel[1], 0.0, epsilon = tol);
        assert_abs_diff_eq!(x_azel[2], 100.0, epsilon = tol);

        // East
        let r_enz = Vector3::new(100.0, 0.0, 0.0);
        let x_azel = position_enz_to_azel(r_enz, DEGREES);

        assert_abs_diff_eq!(x_azel[0], 90.0, epsilon = tol);
        assert_abs_diff_eq!(x_azel[1], 0.0, epsilon = tol);
        assert_abs_diff_eq!(x_azel[2], 100.0, epsilon = tol);

        // North-West
        let r_enz = Vector3::new(-100.0, 100.0, 0.0);
        let x_azel = position_enz_to_azel(r_enz, DEGREES);

        assert_abs_diff_eq!(x_azel[0], 315.0, epsilon = tol);
        assert_abs_diff_eq!(x_azel[1], 0.0, epsilon = tol);
        assert_abs_diff_eq!(x_azel[2], 100.0 * 2.0_f64.sqrt(), epsilon = tol);
    }

    #[test]
    fn test_position_sez_to_azel() {
        let tol = f64::EPSILON;

        // Directly above
        let r_sez = Vector3::new(0.0, 0.0, 100.0);
        let x_azel = position_sez_to_azel(r_sez, DEGREES);

        assert_abs_diff_eq!(x_azel[0], 0.0, epsilon = tol);
        assert_abs_diff_eq!(x_azel[1], 90.0, epsilon = tol);
        assert_abs_diff_eq!(x_azel[2], 100.0, epsilon = tol);

        // North
        let r_sez = Vector3::new(-100.0, 0.0, 0.0);
        let x_azel = position_sez_to_azel(r_sez, DEGREES);

        assert_abs_diff_eq!(x_azel[0], 0.0, epsilon = tol);
        assert_abs_diff_eq!(x_azel[1], 0.0, epsilon = tol);
        assert_abs_diff_eq!(x_azel[2], 100.0, epsilon = tol);

        // East
        let r_sez = Vector3::new(0.0, 100.0, 0.0);
        let x_azel = position_sez_to_azel(r_sez, DEGREES);

        assert_abs_diff_eq!(x_azel[0], 90.0, epsilon = tol);
        assert_abs_diff_eq!(x_azel[1], 0.0, epsilon = tol);
        assert_abs_diff_eq!(x_azel[2], 100.0, epsilon = tol);

        // North-West
        let r_sez = Vector3::new(-100.0, -100.0, 0.0);
        let x_azel = position_sez_to_azel(r_sez, DEGREES);

        assert_abs_diff_eq!(x_azel[0], 315.0, epsilon = tol);
        assert_abs_diff_eq!(x_azel[1], 0.0, epsilon = tol);
        assert_abs_diff_eq!(x_azel[2], 100.0 * 2.0_f64.sqrt(), epsilon = tol);
    }
}