@@ -396,7 +396,7 @@ and a rotation matrix.
396
396
It optionally returns three rotation matrices, one for each axis, and the three Euler angles in
397
397
degrees (as the return value) that could be used in OpenGL. Note, there is always more than one
398
398
sequence of rotations about the three principal axes that results in the same orientation of an
399
- object, eg . see @cite Slabaugh . Returned tree rotation matrices and corresponding three Euler angles
399
+ object, e.g . see @cite Slabaugh . Returned tree rotation matrices and corresponding three Euler angles
400
400
are only one of the possible solutions.
401
401
*/
402
402
CV_EXPORTS_W Vec3d RQDecomp3x3 ( InputArray src, OutputArray mtxR, OutputArray mtxQ,
@@ -421,8 +421,8 @@ matrix and the position of a camera.
421
421
422
422
It optionally returns three rotation matrices, one for each axis, and three Euler angles that could
423
423
be used in OpenGL. Note, there is always more than one sequence of rotations about the three
424
- principal axes that results in the same orientation of an object, eg . see @cite Slabaugh . Returned
425
- tree rotation matrices and corresponding three Euler angules are only one of the possible solutions.
424
+ principal axes that results in the same orientation of an object, e.g . see @cite Slabaugh . Returned
425
+ tree rotation matrices and corresponding three Euler angles are only one of the possible solutions.
426
426
427
427
The function is based on RQDecomp3x3 .
428
428
*/
@@ -1205,7 +1205,7 @@ findFundamentalMat .
1205
1205
@param threshold Optional threshold used to filter out the outliers. If the parameter is greater
1206
1206
than zero, all the point pairs that do not comply with the epipolar geometry (that is, the points
1207
1207
for which \f$|\texttt{points2[i]}^T*\texttt{F}*\texttt{points1[i]}|>\texttt{threshold}\f$ ) are
1208
- rejected prior to computing the homographies. Otherwise,all the points are considered inliers.
1208
+ rejected prior to computing the homographies. Otherwise, all the points are considered inliers.
1209
1209
1210
1210
The function computes the rectification transformations without knowing intrinsic parameters of the
1211
1211
cameras and their relative position in the space, which explains the suffix "uncalibrated". Another
@@ -1249,7 +1249,7 @@ assumed.
1249
1249
@param alpha Free scaling parameter between 0 (when all the pixels in the undistorted image are
1250
1250
valid) and 1 (when all the source image pixels are retained in the undistorted image). See
1251
1251
stereoRectify for details.
1252
- @param newImgSize Image size after rectification. By default,it is set to imageSize .
1252
+ @param newImgSize Image size after rectification. By default, it is set to imageSize .
1253
1253
@param validPixROI Optional output rectangle that outlines all-good-pixels region in the
1254
1254
undistorted image. See roi1, roi2 description in stereoRectify .
1255
1255
@param centerPrincipalPoint Optional flag that indicates whether in the new camera matrix the
@@ -1260,7 +1260,7 @@ best fit a subset of the source image (determined by alpha) to the corrected ima
1260
1260
The function computes and returns the optimal new camera matrix based on the free scaling parameter.
1261
1261
By varying this parameter, you may retrieve only sensible pixels alpha=0 , keep all the original
1262
1262
image pixels if there is valuable information in the corners alpha=1 , or get something in between.
1263
- When alpha\>0 , the undistortion result is likely to have some black pixels corresponding to
1263
+ When alpha\>0 , the undistorted result is likely to have some black pixels corresponding to
1264
1264
"virtual" pixels outside of the captured distorted image. The original camera matrix, distortion
1265
1265
coefficients, the computed new camera matrix, and newImageSize should be passed to
1266
1266
initUndistortRectifyMap to produce the maps for remap .
@@ -1456,7 +1456,7 @@ floating-point (single or double precision).
1456
1456
Note that this function assumes that points1 and points2 are feature points from cameras with the
1457
1457
same camera matrix.
1458
1458
@param R Recovered relative rotation.
1459
- @param t Recoverd relative translation.
1459
+ @param t Recovered relative translation.
1460
1460
@param mask Input/output mask for inliers in points1 and points2.
1461
1461
: If it is not empty, then it marks inliers in points1 and points2 for then given essential
1462
1462
matrix E. Only these inliers will be used to recover pose. In the output mask only inliers
@@ -1499,7 +1499,7 @@ CV_EXPORTS_W int recoverPose( InputArray E, InputArray points1, InputArray point
1499
1499
floating-point (single or double precision).
1500
1500
@param points2 Array of the second image points of the same size and format as points1 .
1501
1501
@param R Recovered relative rotation.
1502
- @param t Recoverd relative translation.
1502
+ @param t Recovered relative translation.
1503
1503
@param focal Focal length of the camera. Note that this function assumes that points1 and points2
1504
1504
are feature points from cameras with same focal length and principal point.
1505
1505
@param pp principal point of the camera.
@@ -1532,7 +1532,7 @@ floating-point (single or double precision).
1532
1532
Note that this function assumes that points1 and points2 are feature points from cameras with the
1533
1533
same camera matrix.
1534
1534
@param R Recovered relative rotation.
1535
- @param t Recoverd relative translation.
1535
+ @param t Recovered relative translation.
1536
1536
@param distanceThresh threshold distance which is used to filter out far away points (i.e. infinite points).
1537
1537
@param mask Input/output mask for inliers in points1 and points2.
1538
1538
: If it is not empty, then it marks inliers in points1 and points2 for then given essential
0 commit comments