I'm trying to find the best way to get the most distant point of a circle from a specified point in 2D space. What I have found so far, is how to get the distance between the point and the circle position, but I'm not entirely sure how to expand this to find the most distant point of the circle.
The known variables are:
Point a
Point b (circle position)
Radius r (circle radius)
To find the distance between the point and the circle position, I have found this:
xd = x2 - x1
yd = y2 - y1
Distance = SquareRoot(xd * xd + yd * yd)
It seems to me, this is part of the solution. How would this be expanded to get the position of Point x in the below image?
As an additional but optional part of the question: I have read in some places that it would be possible to get the distance portion without using the Square Root, which is very performance intensive and should be avoided if fast code is necessary. In my case, I would be doing this calculation quite often; Any comments on this within the context of the main question would be welcome too.
What about this?
Calculate A-B.
We now have a vector pointing from the center of the circle towards A (if B is the origin, skip this and just consider point A a vector).
Normalize.
Now we have a well defined length (the length is 1)
If the circle is not of unit radius, multiply by radius. If it is unit radius, skip this.
Now we have the correct length.
Invert sign (can be done in one step with 3., just multiply with the negative radius)
Now our vector points in the correct direction.
Add B (if B is the origin, skip this).
Now our vector is offset correctly so its endpoint is the point we want.
(Alternatively, you could calculate B-A to save the negation, but then you have to do one more operation to offset the origin correctly.)
By the way, it works the same in 3D, except the circle would be a sphere, and the vectors would have 3 components (or 4, if you use homogenous coords, in this case remember -- for correctness -- setting w to 0 when "turning points into vectors" and to 1 at the end when making a point from the vector).
EDIT:
(in reply of pseudocode)
Assuming you have a vec2 class which is a struct of two float numbers with operators for vector subtraction and scalar multiplicaion (pretty trivial, around a dozen lines of code) and a function normalize which needs to be no more than a shorthand for multiplying with inv_sqrt(x*x+y*y), the pseudocode (my pseudocode here is something like a C++/GLSL mix) could look something like this:
vec2 most_distant_on_circle(vec2 const& B, float r, vec2 const& A)
{
vec2 P(A - B);
normalize(P);
return -r * P + B;
}
Most math libraries that you'd use should have all of these functions and types built-in. HLSL and GLSL have them as first type primitives and intrinsic functions. Some GPUs even have a dedicated normalize instruction.
Related
I have this seemingly simple but very confusing problem.
Given I have a set of vertices (x1,y1), (x2,y2), (x3,y3)...... representing an arc. The points can either be clockwise or counter clockwise, but are all similarly ordered.
And I know the center of the arc (xc,yc).
How can I tell if the arc subtends an acute/obtuse or reflex angle?
One obvious solution is to take the difference of atan2((last_pt)-(center)) and atan2((first_pt)-(center))). But if the arc goes through the point where PI become -PI, this method breaks down.
Also, since the arc points are derived from a rather noisy pixelated picture, the vertices are not exactly smooth.
Picture of a acute and reflex arc
I cant wrap my brain around solving this problem.
Thanks for your help!
Working with 2D angles is a pain for the reason you described, so it's better to work with vector math instead, which is rotationally invariant.
Define the 2D cross-product, A ^ B = Ax * By - Ay * Bx. This is positive if A is clockwise rotated relative to B, and vice versa.
The logic:
Compute C = (last_pt - center) ^ (first_pt - center)
If C = 0, the arc is either closed or 180-degree (forgot the name for this)
If C > 0, the arc must either be (i) clockwise and acute/obtuse or (ii) anti-clockwise and reflex
If C < 0, the opposite applies
Pseudocode:
int arc_type(Point first, Point last, Point center, bool clockwise)
{
// cross-product
float C = (last.x - center.x) * (first.y - center.y)
- (last.y - center.y) * (first.x - center.x);
if (Math.abs(C) < /* small epsilon */)
return 0; // 180-degree
return ((C > 0) ^ clockwise) ? 1 // reflex
: -1; // acute / obtuse
}
Note that if you don't have prior knowledge of whether the arc is clockwise or anti-, you can use the same cross-product method on adjacent points. You need to ensure that the order of the points is consistent - if not you can, again using the cross-product, sort them by (relative) angle.
Question:
I need to calculate intersection shape (purple) of plane defined by Ax + By + Cz + D = 0 and frustum defined by 4 rays emitting from corners of rectangle (red arrows). The result shoud be quadrilateral (4 points) and important requirement is that result shape must be in plane's local space. Plane is created with transformation matrix T (planes' normal is vec3(0, 0, 1) in T's space).
Explanation:
This is perspective form of my rectangle projection to another space (transformation / matrix / node). I am able to calculate intersection shape of any rectangle without perspective rays (all rays are parallel) by plane-line intersection algorithm (pseudocode):
Definitions:
// Plane defined by normal (A, B, C) and D
struct Plane { vec3 n; float d; };
// Line defined by 2 points
struct Line { vec3 a, b; };
Intersection:
vec3 PlaneLineIntersection(Plane plane, Line line) {
vec3 ba = normalize(line.b, line.a);
float dotA = dot(plane.n, l.a);
float dotBA = dot(plane.n, ba);
float t = (plane.d - dotA) / dotBA;
return line.a + ba * t;
}
Perspective form comes with some problems, because some of rays could be parallel with plane (intersection point is in infinite) or final shape is self-intersecting. Its works in some cases, but it's not enough for arbitary transformation. How to get correct intersection part of plane wtih perspective?
Simply, I need to get visible part of arbitary plane by arbitary perspective "camera".
Thank you for suggestions.
Intersection between a plane (one Ax+By+Cx+D equation) and a line (two planes equations) is a matter of solving the 3x3 matrix for x,y,z.
Doing all calculations on T-space (origin is at the top of the pyramid) is easier as some A,B,C are 0.
What I don't know if you are aware of is that perspective is a kind of projection that distorts the z ("depth", far from the origin). So if the plane that contains the rectangle is not perpendicular to the axis of the fustrum (z-axis) then it's not a rectangle when projected into the plane, but a trapezoid.
Anyhow, using the projection perspective matrix you can get projected coordinates for the four rectangle corners.
To tell if a point is in one side of a plane or in the other just put the point coordinates in the plane equation and get the sign, as shown here
Your question seems inherently mathematic so excuse my mathematical solution on StackOverflow. If your four arrows emit from a single point and the formed side planes share a common angle, then you are looking for a solution to the frustum projection problem. Your requirements simplify the problem quite a bit because you define the plane with a normal, not two bounded vectors, thus if you agree to the definitions...
then I can provide you with the mathematical solution here (Internet Explorer .mht file, possibly requiring modern Windows OS). If you are thinking about an actual implementation then I can only direct you to a very similar frustum projection implementation that I have implemented/uploaded here (Lua): https://github.com/quiret/mta_lua_3d_math
The roadmap for the implementation could be as follows: creation of condition container classes for all sub-problems (0 < k1*a1 + k2, etc) plus the and/or chains, writing algorithms for the comparisions across and-chains as well as normal-form creation, optimization of object construction/memory allocation. Since each check for frustum intersection requires just a fixed amount of algebraic objects you can implement an efficient cache.
I think there is a pretty straightForward answer to this, but i cant find it. My geometry lessons are too far away for this. the problem is:
Given 2 points A and B (coordinates Ax Ay Bx and By), I want to find the coordinates of points C and D so that [AB] and [CD] segments intersect at their center and [CD] has a length of d (a variable).
I want to find the equation giving me Cx,Cy,Dx and Dy from Ax,Ay,Bx,By and d.
Here is a little schema of the problem:
and an image of the intended result:
I already know how to find the center point of [AB] (Ax+Bx/2, Ay+By/2), how to find the slope of the [AB] segment (By-Ay/Bx-Ax) and then one of the [CD] segment (Ax-Bx/By-Ay). But then i get stuck on how to get my two points. I thought i could calculate the angle from the slope, then use it with some trigonometry to get the coordinates but it sounds like a quite heavy, ugly and unnecessary calculation...
It feels so close, but i still cant get it.
I also found this post, which is almost perfect, but the length cannot be defined: it must be the same as the first segment.
I dont think this is language-dependent, but if you must know, i'm doing a mini prototype on processing and will probably get it on javascript later.
Thanks for any help.
The basic trick here is that, in 2d, the perpendicular to a vector (x, y) is merely ± (-y, x). (One gets this by computing the cross product with the (0, 0, 1) vector in 3d, and projecting to 2d.) So what you need to do is:
Get the midpoint between A and B (you have done that).
Get the vector from A to B, which is B - A = (x, y) = (bx - ax, by - ay).
Get the perpendicular vector: (-y, x).
Normalize it. Let length = sqrt(y*y + x*x), then norm = (-y/length, x/length).
Multiply the normalized perpendicular by your desired distance ± d/2 (since you want the distance between C and D to be d), and add to the center point.
No slopes or trig functions are required.
I have the plane equation describing the points belonging to a plane in 3D and the origin of the normal X, Y, Z. This should be enough to be able to generate something like a 3D arrow. In pcl this is possible via the viewer but I would like to actually store those 3D points inside the cloud. How to generate them then ? A cylinder with a cone on top ?
To generate a line perpendicular to the plane:
You have the plane equation. This gives you the direction of the normal to the plane. If you used PCL to get the plane, this is in ModelCoefficients. See the details here: SampleConsensusModelPerpendicularPlane
The first step is to make a line perpendicular to the normal at the point you mention (X,Y,Z). Let (NORMAL_X,NORMAL_Y,NORMAL_Z) be the normal you got from your plane equation. Something like.
pcl::PointXYZ pnt_on_line;
for(double distfromstart=0.0;distfromstart<LINE_LENGTH;distfromstart+=DISTANCE_INCREMENT){
pnt_on_line.x = X + distfromstart*NORMAL_X;
pnt_on_line.y = Y + distfromstart*NORMAL_Y;
pnt_on_line.z = Z + distfromstart*NORMAL_Z;
my_cloud.points.push_back(pnt_on_line);
}
Now you want to put a hat on your arrow and now pnt_on_line contains the end of the line exactly where you want to put it. To make the cone you could loop over angle and distance along the arrow, calculate a local x and y and z from that and convert them to points in point cloud space: the z part would be converted into your point cloud's frame of reference by multiplying with the normal vector as with above, the x and y would be multiplied into vectors perpendicular to this normal vectorE. To get these, choose an arbitrary unit vector perpendicular to the normal vector (for your x axis) and cross product it with the normal vector to find the y axis.
The second part of this explanation is fairly terse but the first part may be the more important.
Update
So possibly the best way to describe how to do the cone is to start with a cylinder, which is an extension of the line described above. In the case of the line, there is (part of) a one dimensional manifold embedded in 3D space. That is we have one variable that we loop over adding points. The cylinder is a two dimensional object so we have to loop over two dimensions: the angle and the distance. In the case of the line we already have the distance. So the above loop would now look like:
for(double distfromstart=0.0;distfromstart<LINE_LENGTH;distfromstart+=DISTANCE_INCREMENT){
for(double angle=0.0;angle<2*M_PI;angle+=M_PI/8){
//calculate coordinates of point and add to cloud
}
}
Now in order to calculate the coordinates of the new point, well we already have the point on the line, now we just need to add it to a vector to move it away from the line in the appropriate direction of the angle. Let's say the radius of our cylinder will be 0.1, and let's say an orthonormal basis that we have already calculated perpendicular to the normal of the plane (which we will see how to calculate later) is perpendicular_1 and perpendicular_2 (that is, two vectors perpendicular to each other, of length 1, also perpendicular to the vector (NORMAL_X,NORMAL_Y,NORMAL_Z)):
//calculate coordinates of point and add to cloud
pnt_on_cylinder.x = pnt_on_line.x + 0.1 * perpendicular_1.x * 0.1 * cos(angle) + perpendicular_2.x * sin(angle)
pnt_on_cylinder.y = pnt_on_line.y + perpendicular_1.y * 0.1 * cos(angle) + perpendicular_2.y * 0.1 * sin(angle)
pnt_on_cylinder.z = pnt_on_line.z + perpendicular_1.z * 0.1 * cos(angle) + perpendicular_2.z * 0.1 * sin(angle)
my_cloud.points.push_back(pnt_on_cylinder);
Actually, this is a vector summation and if we were to write the operation as vectors it would look like:
pnt_on_line+perpendicular_1*cos(angle)+perpendicular_2*sin(angle)
Now I said I would talk about how to calculate perpendicular_1 and perpendicular_2. Let K be any unit vector that is not parallel to (NORMAL_X,NORMAL_Y,NORMAL_Z) (this can be found by trying e.g. (1,0,0) then (0,1,0)).
Then
perpendicular_1 = K X (NORMAL_X,NORMAL_Y,NORMAL_Z)
perpendicular_2 = perpendicular_1 X (NORMAL_X,NORMAL_Y,NORMAL_Z)
Here X is the vector cross product and the above are vector equations. Note also that the original calculation of pnt_on_line involved a vector dot product and a vector summation (I am just writing this for completeness of the exposition).
If you can manage this then the cone is easy just by changing a couple of things in the double loop: the radius just changes along its length until it is zero at the end of the loop and in the loop distfromstart will not start at 0.
Given two image buffers (assume it's an array of ints of size width * height, with each element a color value), how can I map an area defined by a quadrilateral from one image buffer into the other (always square) image buffer? I'm led to understand this is called "projective transformation".
I'm also looking for a general (not language- or library-specific) way of doing this, such that it could be reasonably applied in any language without relying on "magic function X that does all the work for me".
An example: I've written a short program in Java using the Processing library (processing.org) that captures video from a camera. During an initial "calibrating" step, the captured video is output directly into a window. The user then clicks on four points to define an area of the video that will be transformed, then mapped into the square window during subsequent operation of the program. If the user were to click on the four points defining the corners of a door visible at an angle in the camera's output, then this transformation would cause the subsequent video to map the transformed image of the door to the entire area of the window, albeit somewhat distorted.
Using linear algebra is much easier than all that geometry! Plus you won't need to use sine, cosine, etc, so you can store each number as a rational fraction and get the exact numerical result if you need it.
What you want is a mapping from your old (x,y) co-ordinates to your new (x',y') co-ordinates. You can do it with matrices. You need to find the 2-by-4 projection matrix P such that P times the old coordinates equals the new co-ordinates. We'll assume that you're mapping lines to lines (not, for instance, straight lines to parabolas). Because you have a projection (parallel lines don't stay parallel) and translation (sliding), you need a factor of (xy) and (1), too. Drawn as matrices:
[x ]
[a b c d]*[y ] = [x']
[e f g h] [x*y] [y']
[1 ]
You need to know a through h so solve these equations:
a*x_0 + b*y_0 + c*x_0*y_0 + d = i_0
a*x_1 + b*y_1 + c*x_1*y_1 + d = i_1
a*x_2 + b*y_2 + c*x_2*y_2 + d = i_2
a*x_3 + b*y_3 + c*x_3*y_3 + d = i_3
e*x_0 + f*y_0 + g*x_0*y_0 + h = j_0
e*x_1 + f*y_1 + g*x_1*y_1 + h = j_1
e*x_2 + f*y_2 + g*x_2*y_2 + h = j_2
e*x_3 + f*y_3 + g*x_3*y_3 + h = j_3
Again, you can use linear algebra:
[x_0 y_0 x_0*y_0 1] [a e] [i_0 j_0]
[x_1 y_1 x_1*y_1 1] * [b f] = [i_1 j_1]
[x_2 y_2 x_2*y_2 1] [c g] [i_2 j_2]
[x_3 y_3 x_3*y_3 1] [d h] [i_3 j_3]
Plug in your corners for x_n,y_n,i_n,j_n. (Corners work best because they are far apart to decrease the error if you're picking the points from, say, user-clicks.) Take the inverse of the 4x4 matrix and multiply it by the right side of the equation. The transpose of that matrix is P. You should be able to find functions to compute a matrix inverse and multiply online.
Where you'll probably have bugs:
When computing, remember to check for division by zero. That's a sign that your matrix is not invertible. That might happen if you try to map one (x,y) co-ordinate to two different points.
If you write your own matrix math, remember that matrices are usually specified row,column (vertical,horizontal) and screen graphics are x,y (horizontal,vertical). You're bound to get something wrong the first time.
EDIT
The assumption below of the invariance of angle ratios is incorrect. Projective transformations instead preserve cross-ratios and incidence. A solution then is:
Find the point C' at the intersection of the lines defined by the segments AD and CP.
Find the point B' at the intersection of the lines defined by the segments AD and BP.
Determine the cross-ratio of B'DAC', i.e. r = (BA' * DC') / (DA * B'C').
Construct the projected line F'HEG'. The cross-ratio of these points is equal to r, i.e. r = (F'E * HG') / (HE * F'G').
F'F and G'G will intersect at the projected point Q so equating the cross-ratios and knowing the length of the side of the square you can determine the position of Q with some arithmetic gymnastics.
Hmmmm....I'll take a stab at this one. This solution relies on the assumption that ratios of angles are preserved in the transformation. See the image for guidance (sorry for the poor image quality...it's REALLY late). The algorithm only provides the mapping of a point in the quadrilateral to a point in the square. You would still need to implement dealing with multiple quad points being mapped to the same square point.
Let ABCD be a quadrilateral where A is the top-left vertex, B is the top-right vertex, C is the bottom-right vertex and D is the bottom-left vertex. The pair (xA, yA) represent the x and y coordinates of the vertex A. We are mapping points in this quadrilateral to the square EFGH whose side has length equal to m.
Compute the lengths AD, CD, AC, BD and BC:
AD = sqrt((xA-xD)^2 + (yA-yD)^2)
CD = sqrt((xC-xD)^2 + (yC-yD)^2)
AC = sqrt((xA-xC)^2 + (yA-yC)^2)
BD = sqrt((xB-xD)^2 + (yB-yD)^2)
BC = sqrt((xB-xC)^2 + (yB-yC)^2)
Let thetaD be the angle at the vertex D and thetaC be the angle at the vertex C. Compute these angles using the cosine law:
thetaD = arccos((AD^2 + CD^2 - AC^2) / (2*AD*CD))
thetaC = arccos((BC^2 + CD^2 - BD^2) / (2*BC*CD))
We map each point P in the quadrilateral to a point Q in the square. For each point P in the quadrilateral, do the following:
Find the distance DP:
DP = sqrt((xP-xD)^2 + (yP-yD)^2)
Find the distance CP:
CP = sqrt((xP-xC)^2 + (yP-yC)^2)
Find the angle thetaP1 between CD and DP:
thetaP1 = arccos((DP^2 + CD^2 - CP^2) / (2*DP*CD))
Find the angle thetaP2 between CD and CP:
thetaP2 = arccos((CP^2 + CD^2 - DP^2) / (2*CP*CD))
The ratio of thetaP1 to thetaD should be the ratio of thetaQ1 to 90. Therefore, calculate thetaQ1:
thetaQ1 = thetaP1 * 90 / thetaD
Similarly, calculate thetaQ2:
thetaQ2 = thetaP2 * 90 / thetaC
Find the distance HQ:
HQ = m * sin(thetaQ2) / sin(180-thetaQ1-thetaQ2)
Finally, the x and y position of Q relative to the bottom-left corner of EFGH is:
x = HQ * cos(thetaQ1)
y = HQ * sin(thetaQ1)
You would have to keep track of how many colour values get mapped to each point in the square so that you can calculate an average colour for each of those points.
I think what you're after is a planar homography, have a look at these lecture notes:
http://www.cs.utoronto.ca/~strider/vis-notes/tutHomography04.pdf
If you scroll down to the end you'll see an example of just what you're describing. I expect there's a function in the Intel OpenCV library which will do just this.
There is a C++ project on CodeProject that includes source for projective transformations of bitmaps. The maths are on Wikipedia here. Note that so far as i know, a projective transformation will not map any arbitrary quadrilateral onto another, but will do so for triangles, you may also want to look up skewing transforms.
If this transformation has to look good (as opposed to the way a bitmap looks if you resize it in Paint), you can't just create a formula that maps destination pixels to source pixels. Values in the destination buffer have to be based on a complex averaging of nearby source pixels or else the results will be highly pixelated.
So unless you want to get into some complex coding, use someone else's magic function, as smacl and Ian have suggested.
Here's how would do it in principle:
map the origin of A to the origin of B via a traslation vector t.
take unit vectors of A (1,0) and (0,1) and calculate how they would be mapped onto the unit vectors of B.
this gives you a transformation matrix M so that every vector a in A maps to M a + t
invert the matrix and negate the traslation vector so for every vector b in B you have the inverse mapping b -> M-1 (b - t)
once you have this transformation, for each point in the target area in B, find the corresponding in A and copy.
The advantage of this mapping is that you only calculate the points you need, i.e. you loop on the target points, not the source points. It was a widely used technique in the "demo coding" scene a few years back.