Table 3.

South America–North America noise-reduced finite rotations.

ChronLat.Long.ΩScaled covariances
(°N)(°E)(degrees)abcdef
1n9.53−56.96−0.1040.8−0.10.20.4−0.50.6
2n10.55−57.15−0.2420.90.00.00.4−0.60.7
2An.111.35−57.21−0.3571.00.0−0.10.5−0.70.9
2An.312.57−57.04−0.5121.20.1−0.30.6−0.81.2
3n.113.21−56.87−0.6061.40.2−0.50.7−0.91.4
3n.414.04−56.55−0.7761.60.4−0.90.8−1.21.9
3An.114.48−56.30−0.9072.00.5−1.01.0−1.52.5
3An.215.10−56.02−1.0332.30.5−1.21.2−1.73.0
4n.115.49−55.75−1.1862.70.5−1.21.1−1.73.3
4n.215.51−55.62−1.3003.30.4−1.01.2−1.83.7
4A15.50−55.41−1.4985.00.3−0.71.5−2.25.1
5n.115.55−55.27−1.6376.80.3−0.31.9−2.76.7
5n.216.14−54.97−1.91110.30.4−0.42.8−3.910.3
5An.217.47−54.72−2.24613.91.0−1.23.6−5.414.3
5AC18.05−54.82−2.53616.91.7−1.03.8−5.816.3
5AD17.75−55.15−2.71219.71.51.23.6−5.316.3
5Cn.117.37−55.75−2.95820.9−0.53.13.2−5.315.4
5D17.24−56.15−3.17520.0−2.03.23.2−5.714.8
5E17.36−56.30−3.31819.8−2.63.03.3−6.014.7
6ny17.57−56.36−3.43821.9−3.54.13.8−6.916.5
6no17.98−56.42−3.58225.4−6.56.46.9−11.121.9
ChronLat.Long.ΩScaled covariances
(°N)(°E)(degrees)abcdef
1n9.53−56.96−0.1040.8−0.10.20.4−0.50.6
2n10.55−57.15−0.2420.90.00.00.4−0.60.7
2An.111.35−57.21−0.3571.00.0−0.10.5−0.70.9
2An.312.57−57.04−0.5121.20.1−0.30.6−0.81.2
3n.113.21−56.87−0.6061.40.2−0.50.7−0.91.4
3n.414.04−56.55−0.7761.60.4−0.90.8−1.21.9
3An.114.48−56.30−0.9072.00.5−1.01.0−1.52.5
3An.215.10−56.02−1.0332.30.5−1.21.2−1.73.0
4n.115.49−55.75−1.1862.70.5−1.21.1−1.73.3
4n.215.51−55.62−1.3003.30.4−1.01.2−1.83.7
4A15.50−55.41−1.4985.00.3−0.71.5−2.25.1
5n.115.55−55.27−1.6376.80.3−0.31.9−2.76.7
5n.216.14−54.97−1.91110.30.4−0.42.8−3.910.3
5An.217.47−54.72−2.24613.91.0−1.23.6−5.414.3
5AC18.05−54.82−2.53616.91.7−1.03.8−5.816.3
5AD17.75−55.15−2.71219.71.51.23.6−5.316.3
5Cn.117.37−55.75−2.95820.9−0.53.13.2−5.315.4
5D17.24−56.15−3.17520.0−2.03.23.2−5.714.8
5E17.36−56.30−3.31819.8−2.63.03.3−6.014.7
6ny17.57−56.36−3.43821.9−3.54.13.8−6.916.5
6no17.98−56.42−3.58225.4−6.56.46.9−11.121.9

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.

Table 3.

South America–North America noise-reduced finite rotations.

ChronLat.Long.ΩScaled covariances
(°N)(°E)(degrees)abcdef
1n9.53−56.96−0.1040.8−0.10.20.4−0.50.6
2n10.55−57.15−0.2420.90.00.00.4−0.60.7
2An.111.35−57.21−0.3571.00.0−0.10.5−0.70.9
2An.312.57−57.04−0.5121.20.1−0.30.6−0.81.2
3n.113.21−56.87−0.6061.40.2−0.50.7−0.91.4
3n.414.04−56.55−0.7761.60.4−0.90.8−1.21.9
3An.114.48−56.30−0.9072.00.5−1.01.0−1.52.5
3An.215.10−56.02−1.0332.30.5−1.21.2−1.73.0
4n.115.49−55.75−1.1862.70.5−1.21.1−1.73.3
4n.215.51−55.62−1.3003.30.4−1.01.2−1.83.7
4A15.50−55.41−1.4985.00.3−0.71.5−2.25.1
5n.115.55−55.27−1.6376.80.3−0.31.9−2.76.7
5n.216.14−54.97−1.91110.30.4−0.42.8−3.910.3
5An.217.47−54.72−2.24613.91.0−1.23.6−5.414.3
5AC18.05−54.82−2.53616.91.7−1.03.8−5.816.3
5AD17.75−55.15−2.71219.71.51.23.6−5.316.3
5Cn.117.37−55.75−2.95820.9−0.53.13.2−5.315.4
5D17.24−56.15−3.17520.0−2.03.23.2−5.714.8
5E17.36−56.30−3.31819.8−2.63.03.3−6.014.7
6ny17.57−56.36−3.43821.9−3.54.13.8−6.916.5
6no17.98−56.42−3.58225.4−6.56.46.9−11.121.9
ChronLat.Long.ΩScaled covariances
(°N)(°E)(degrees)abcdef
1n9.53−56.96−0.1040.8−0.10.20.4−0.50.6
2n10.55−57.15−0.2420.90.00.00.4−0.60.7
2An.111.35−57.21−0.3571.00.0−0.10.5−0.70.9
2An.312.57−57.04−0.5121.20.1−0.30.6−0.81.2
3n.113.21−56.87−0.6061.40.2−0.50.7−0.91.4
3n.414.04−56.55−0.7761.60.4−0.90.8−1.21.9
3An.114.48−56.30−0.9072.00.5−1.01.0−1.52.5
3An.215.10−56.02−1.0332.30.5−1.21.2−1.73.0
4n.115.49−55.75−1.1862.70.5−1.21.1−1.73.3
4n.215.51−55.62−1.3003.30.4−1.01.2−1.83.7
4A15.50−55.41−1.4985.00.3−0.71.5−2.25.1
5n.115.55−55.27−1.6376.80.3−0.31.9−2.76.7
5n.216.14−54.97−1.91110.30.4−0.42.8−3.910.3
5An.217.47−54.72−2.24613.91.0−1.23.6−5.414.3
5AC18.05−54.82−2.53616.91.7−1.03.8−5.816.3
5AD17.75−55.15−2.71219.71.51.23.6−5.316.3
5Cn.117.37−55.75−2.95820.9−0.53.13.2−5.315.4
5D17.24−56.15−3.17520.0−2.03.23.2−5.714.8
5E17.36−56.30−3.31819.8−2.63.03.3−6.014.7
6ny17.57−56.36−3.43821.9−3.54.13.8−6.916.5
6no17.98−56.42−3.58225.4−6.56.46.9−11.121.9

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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