Chron . | Lat. . | Long. . | Ω . | Scaled covariances . | |||||
---|---|---|---|---|---|---|---|---|---|
. | (°N) . | (°E) . | (degrees) . | a . | b . | c . | d . | e . | f . |
1n | 9.53 | −56.96 | −0.104 | 0.8 | −0.1 | 0.2 | 0.4 | −0.5 | 0.6 |
2n | 10.55 | −57.15 | −0.242 | 0.9 | 0.0 | 0.0 | 0.4 | −0.6 | 0.7 |
2An.1 | 11.35 | −57.21 | −0.357 | 1.0 | 0.0 | −0.1 | 0.5 | −0.7 | 0.9 |
2An.3 | 12.57 | −57.04 | −0.512 | 1.2 | 0.1 | −0.3 | 0.6 | −0.8 | 1.2 |
3n.1 | 13.21 | −56.87 | −0.606 | 1.4 | 0.2 | −0.5 | 0.7 | −0.9 | 1.4 |
3n.4 | 14.04 | −56.55 | −0.776 | 1.6 | 0.4 | −0.9 | 0.8 | −1.2 | 1.9 |
3An.1 | 14.48 | −56.30 | −0.907 | 2.0 | 0.5 | −1.0 | 1.0 | −1.5 | 2.5 |
3An.2 | 15.10 | −56.02 | −1.033 | 2.3 | 0.5 | −1.2 | 1.2 | −1.7 | 3.0 |
4n.1 | 15.49 | −55.75 | −1.186 | 2.7 | 0.5 | −1.2 | 1.1 | −1.7 | 3.3 |
4n.2 | 15.51 | −55.62 | −1.300 | 3.3 | 0.4 | −1.0 | 1.2 | −1.8 | 3.7 |
4A | 15.50 | −55.41 | −1.498 | 5.0 | 0.3 | −0.7 | 1.5 | −2.2 | 5.1 |
5n.1 | 15.55 | −55.27 | −1.637 | 6.8 | 0.3 | −0.3 | 1.9 | −2.7 | 6.7 |
5n.2 | 16.14 | −54.97 | −1.911 | 10.3 | 0.4 | −0.4 | 2.8 | −3.9 | 10.3 |
5An.2 | 17.47 | −54.72 | −2.246 | 13.9 | 1.0 | −1.2 | 3.6 | −5.4 | 14.3 |
5AC | 18.05 | −54.82 | −2.536 | 16.9 | 1.7 | −1.0 | 3.8 | −5.8 | 16.3 |
5AD | 17.75 | −55.15 | −2.712 | 19.7 | 1.5 | 1.2 | 3.6 | −5.3 | 16.3 |
5Cn.1 | 17.37 | −55.75 | −2.958 | 20.9 | −0.5 | 3.1 | 3.2 | −5.3 | 15.4 |
5D | 17.24 | −56.15 | −3.175 | 20.0 | −2.0 | 3.2 | 3.2 | −5.7 | 14.8 |
5E | 17.36 | −56.30 | −3.318 | 19.8 | −2.6 | 3.0 | 3.3 | −6.0 | 14.7 |
6ny | 17.57 | −56.36 | −3.438 | 21.9 | −3.5 | 4.1 | 3.8 | −6.9 | 16.5 |
6no | 17.98 | −56.42 | −3.582 | 25.4 | −6.5 | 6.4 | 6.9 | −11.1 | 21.9 |
Chron . | Lat. . | Long. . | Ω . | Scaled covariances . | |||||
---|---|---|---|---|---|---|---|---|---|
. | (°N) . | (°E) . | (degrees) . | a . | b . | c . | d . | e . | f . |
1n | 9.53 | −56.96 | −0.104 | 0.8 | −0.1 | 0.2 | 0.4 | −0.5 | 0.6 |
2n | 10.55 | −57.15 | −0.242 | 0.9 | 0.0 | 0.0 | 0.4 | −0.6 | 0.7 |
2An.1 | 11.35 | −57.21 | −0.357 | 1.0 | 0.0 | −0.1 | 0.5 | −0.7 | 0.9 |
2An.3 | 12.57 | −57.04 | −0.512 | 1.2 | 0.1 | −0.3 | 0.6 | −0.8 | 1.2 |
3n.1 | 13.21 | −56.87 | −0.606 | 1.4 | 0.2 | −0.5 | 0.7 | −0.9 | 1.4 |
3n.4 | 14.04 | −56.55 | −0.776 | 1.6 | 0.4 | −0.9 | 0.8 | −1.2 | 1.9 |
3An.1 | 14.48 | −56.30 | −0.907 | 2.0 | 0.5 | −1.0 | 1.0 | −1.5 | 2.5 |
3An.2 | 15.10 | −56.02 | −1.033 | 2.3 | 0.5 | −1.2 | 1.2 | −1.7 | 3.0 |
4n.1 | 15.49 | −55.75 | −1.186 | 2.7 | 0.5 | −1.2 | 1.1 | −1.7 | 3.3 |
4n.2 | 15.51 | −55.62 | −1.300 | 3.3 | 0.4 | −1.0 | 1.2 | −1.8 | 3.7 |
4A | 15.50 | −55.41 | −1.498 | 5.0 | 0.3 | −0.7 | 1.5 | −2.2 | 5.1 |
5n.1 | 15.55 | −55.27 | −1.637 | 6.8 | 0.3 | −0.3 | 1.9 | −2.7 | 6.7 |
5n.2 | 16.14 | −54.97 | −1.911 | 10.3 | 0.4 | −0.4 | 2.8 | −3.9 | 10.3 |
5An.2 | 17.47 | −54.72 | −2.246 | 13.9 | 1.0 | −1.2 | 3.6 | −5.4 | 14.3 |
5AC | 18.05 | −54.82 | −2.536 | 16.9 | 1.7 | −1.0 | 3.8 | −5.8 | 16.3 |
5AD | 17.75 | −55.15 | −2.712 | 19.7 | 1.5 | 1.2 | 3.6 | −5.3 | 16.3 |
5Cn.1 | 17.37 | −55.75 | −2.958 | 20.9 | −0.5 | 3.1 | 3.2 | −5.3 | 15.4 |
5D | 17.24 | −56.15 | −3.175 | 20.0 | −2.0 | 3.2 | 3.2 | −5.7 | 14.8 |
5E | 17.36 | −56.30 | −3.318 | 19.8 | −2.6 | 3.0 | 3.3 | −6.0 | 14.7 |
6ny | 17.57 | −56.36 | −3.438 | 21.9 | −3.5 | 4.1 | 3.8 | −6.9 | 16.5 |
6no | 17.98 | −56.42 | −3.582 | 25.4 | −6.5 | 6.4 | 6.9 | −11.1 | 21.9 |
These finite rotations, which reconstruct the North America plate onto the South America plate, were determined by combining North America–Nubia noise-reduced rotations from DeMets et al. (2015a) with Nubia–South America noise-reduced rotations from Table 1. Rotation angles Ω are positive anticlockwise. The Cartesian rotation covariances, which are tied to the North America plate, specify the 2-D uncertainty in the location of the North America plate upon its rotation onto the South America plate. The covariances, which have units of 10−8 radians2, have been reduced by a factor of 16 so as to approximate the scatter in results obtained from the best-fitting North America–South America rotations. Instructions for reconstructing the covariance matrix are found in the Table 1 footnotes.
Chron . | Lat. . | Long. . | Ω . | Scaled covariances . | |||||
---|---|---|---|---|---|---|---|---|---|
. | (°N) . | (°E) . | (degrees) . | a . | b . | c . | d . | e . | f . |
1n | 9.53 | −56.96 | −0.104 | 0.8 | −0.1 | 0.2 | 0.4 | −0.5 | 0.6 |
2n | 10.55 | −57.15 | −0.242 | 0.9 | 0.0 | 0.0 | 0.4 | −0.6 | 0.7 |
2An.1 | 11.35 | −57.21 | −0.357 | 1.0 | 0.0 | −0.1 | 0.5 | −0.7 | 0.9 |
2An.3 | 12.57 | −57.04 | −0.512 | 1.2 | 0.1 | −0.3 | 0.6 | −0.8 | 1.2 |
3n.1 | 13.21 | −56.87 | −0.606 | 1.4 | 0.2 | −0.5 | 0.7 | −0.9 | 1.4 |
3n.4 | 14.04 | −56.55 | −0.776 | 1.6 | 0.4 | −0.9 | 0.8 | −1.2 | 1.9 |
3An.1 | 14.48 | −56.30 | −0.907 | 2.0 | 0.5 | −1.0 | 1.0 | −1.5 | 2.5 |
3An.2 | 15.10 | −56.02 | −1.033 | 2.3 | 0.5 | −1.2 | 1.2 | −1.7 | 3.0 |
4n.1 | 15.49 | −55.75 | −1.186 | 2.7 | 0.5 | −1.2 | 1.1 | −1.7 | 3.3 |
4n.2 | 15.51 | −55.62 | −1.300 | 3.3 | 0.4 | −1.0 | 1.2 | −1.8 | 3.7 |
4A | 15.50 | −55.41 | −1.498 | 5.0 | 0.3 | −0.7 | 1.5 | −2.2 | 5.1 |
5n.1 | 15.55 | −55.27 | −1.637 | 6.8 | 0.3 | −0.3 | 1.9 | −2.7 | 6.7 |
5n.2 | 16.14 | −54.97 | −1.911 | 10.3 | 0.4 | −0.4 | 2.8 | −3.9 | 10.3 |
5An.2 | 17.47 | −54.72 | −2.246 | 13.9 | 1.0 | −1.2 | 3.6 | −5.4 | 14.3 |
5AC | 18.05 | −54.82 | −2.536 | 16.9 | 1.7 | −1.0 | 3.8 | −5.8 | 16.3 |
5AD | 17.75 | −55.15 | −2.712 | 19.7 | 1.5 | 1.2 | 3.6 | −5.3 | 16.3 |
5Cn.1 | 17.37 | −55.75 | −2.958 | 20.9 | −0.5 | 3.1 | 3.2 | −5.3 | 15.4 |
5D | 17.24 | −56.15 | −3.175 | 20.0 | −2.0 | 3.2 | 3.2 | −5.7 | 14.8 |
5E | 17.36 | −56.30 | −3.318 | 19.8 | −2.6 | 3.0 | 3.3 | −6.0 | 14.7 |
6ny | 17.57 | −56.36 | −3.438 | 21.9 | −3.5 | 4.1 | 3.8 | −6.9 | 16.5 |
6no | 17.98 | −56.42 | −3.582 | 25.4 | −6.5 | 6.4 | 6.9 | −11.1 | 21.9 |
Chron . | Lat. . | Long. . | Ω . | Scaled covariances . | |||||
---|---|---|---|---|---|---|---|---|---|
. | (°N) . | (°E) . | (degrees) . | a . | b . | c . | d . | e . | f . |
1n | 9.53 | −56.96 | −0.104 | 0.8 | −0.1 | 0.2 | 0.4 | −0.5 | 0.6 |
2n | 10.55 | −57.15 | −0.242 | 0.9 | 0.0 | 0.0 | 0.4 | −0.6 | 0.7 |
2An.1 | 11.35 | −57.21 | −0.357 | 1.0 | 0.0 | −0.1 | 0.5 | −0.7 | 0.9 |
2An.3 | 12.57 | −57.04 | −0.512 | 1.2 | 0.1 | −0.3 | 0.6 | −0.8 | 1.2 |
3n.1 | 13.21 | −56.87 | −0.606 | 1.4 | 0.2 | −0.5 | 0.7 | −0.9 | 1.4 |
3n.4 | 14.04 | −56.55 | −0.776 | 1.6 | 0.4 | −0.9 | 0.8 | −1.2 | 1.9 |
3An.1 | 14.48 | −56.30 | −0.907 | 2.0 | 0.5 | −1.0 | 1.0 | −1.5 | 2.5 |
3An.2 | 15.10 | −56.02 | −1.033 | 2.3 | 0.5 | −1.2 | 1.2 | −1.7 | 3.0 |
4n.1 | 15.49 | −55.75 | −1.186 | 2.7 | 0.5 | −1.2 | 1.1 | −1.7 | 3.3 |
4n.2 | 15.51 | −55.62 | −1.300 | 3.3 | 0.4 | −1.0 | 1.2 | −1.8 | 3.7 |
4A | 15.50 | −55.41 | −1.498 | 5.0 | 0.3 | −0.7 | 1.5 | −2.2 | 5.1 |
5n.1 | 15.55 | −55.27 | −1.637 | 6.8 | 0.3 | −0.3 | 1.9 | −2.7 | 6.7 |
5n.2 | 16.14 | −54.97 | −1.911 | 10.3 | 0.4 | −0.4 | 2.8 | −3.9 | 10.3 |
5An.2 | 17.47 | −54.72 | −2.246 | 13.9 | 1.0 | −1.2 | 3.6 | −5.4 | 14.3 |
5AC | 18.05 | −54.82 | −2.536 | 16.9 | 1.7 | −1.0 | 3.8 | −5.8 | 16.3 |
5AD | 17.75 | −55.15 | −2.712 | 19.7 | 1.5 | 1.2 | 3.6 | −5.3 | 16.3 |
5Cn.1 | 17.37 | −55.75 | −2.958 | 20.9 | −0.5 | 3.1 | 3.2 | −5.3 | 15.4 |
5D | 17.24 | −56.15 | −3.175 | 20.0 | −2.0 | 3.2 | 3.2 | −5.7 | 14.8 |
5E | 17.36 | −56.30 | −3.318 | 19.8 | −2.6 | 3.0 | 3.3 | −6.0 | 14.7 |
6ny | 17.57 | −56.36 | −3.438 | 21.9 | −3.5 | 4.1 | 3.8 | −6.9 | 16.5 |
6no | 17.98 | −56.42 | −3.582 | 25.4 | −6.5 | 6.4 | 6.9 | −11.1 | 21.9 |
These finite rotations, which reconstruct the North America plate onto the South America plate, were determined by combining North America–Nubia noise-reduced rotations from DeMets et al. (2015a) with Nubia–South America noise-reduced rotations from Table 1. Rotation angles Ω are positive anticlockwise. The Cartesian rotation covariances, which are tied to the North America plate, specify the 2-D uncertainty in the location of the North America plate upon its rotation onto the South America plate. The covariances, which have units of 10−8 radians2, have been reduced by a factor of 16 so as to approximate the scatter in results obtained from the best-fitting North America–South America rotations. Instructions for reconstructing the covariance matrix are found in the Table 1 footnotes.
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