From rotation matrix to yaw angle and vice-versa: +/- 180deg offset? - matrix

I have a general 3D rotation matrix like this:
|R11 R12 R13|
|R21 R22 R23|
|R31 R32 R33|
From this rotation matrix, I know I can get the yaw Tait-Bryan Euler angle with this:
yaw = atan2(R21, R11)
In my system I have:
R21 = Asin(r) + Bcos(r)
R11 = Ccos(r) + Dsin(r)
with:
r = RZ - 90deg
A = -0.01775
B = 0.9997
C = -0.01714
D = -0.99924
leading to:
yaw = atan2(-0.01775sin(RZ - 90) + 0.9997cos(RZ - 90) , -0.01714cos(RZ - 90) - 0.99924sin(RZ - 90))
Ex.: if RZ = -136.01355deg, I get yaw = -135.0deg which is what I expect given my system.
Now what I really want to do is the opposite: find RZ given a known yaw value. But for some reason this does not always work. I sometimes am +/- 180deg off. Here is how I re-arranged the equation:
atan2(Asin(r) + Bcos(r), Ccos(r) + Dsin(r)) = Y
(Asin(r) + Bcos(r)) / (Ccos(r) + Dsin(r)) = tan(Y)
Asin(r) + Bcos(r) = tan(Y)Ccos(r) + tan(Y)Dsin(r)
(A - tan(Y)D)sin(r) + (B - tan(Y)C)cos(r) = 0
(A - tan(Y)D)tan(r) + (B - tan(Y)C) = 0
(A - tan(Y)D)tan(r) = tan(Y)C - B
tan(r) = (tan(Y)C - B) / (A - tan(Y)D)
r = atan2(tan(Y)C - B, A - tan(Y)D)
With my system's values:
RZ = atan2(-0.01714tan(yaw) - 0.9997 , 0.99924tan(yaw) - 0.01775) + 90deg
So for yaw = -135deg, I get RZ = 43.98645 which is exactly 180 more than the expected value of -136.01355 (ie it looks like I need to subtract 180 from my result).
It seems that for yaw angles between -90 to 90deg, RZ is good; for yaw < 90deg, I need to do RZ - 180deg; and for yaw > 90deg, I need to do RZ + 180deg.
Does this make sense ? Is my math ok ? Is this solution good and what is the explanation for it ? Is it somehow related to tan(yaw) ? I would definitely prefer a solution that always yields the correct result without the extra step !! Thanks for any insights !!

Related

Calculating a location on a circle given an angle of rotation

Okay algebra and trig are not my strong suit by any means so here is what I need to do.
I have a circle which is measured in degrees from +180 to -180 (360 total)
Given the center point of the circle stays the same, Cx , Cy.
The angle varies from -180 to +180
I need to locate a point that regardless the given angle is + 3 units away that is at the 90 degree position and the 270 degree position (from the given degrees)
So like...
Angle = 0
Point 1 -> x = 0, y -3
Point 2 -> x = 0, y + 3
And if the angle was say 90 (provided its measured Clockwise)
Point 1 -> x = -3, y = 0
Point 2 -> x = 3, y = 0
What I need is a forumla that will accept Angle, then tell me what my x/y should be 3 units away from the origin.
I have tried: EDIT Updated to double precision using Java.
`double x = Cx + 3 * Math.cos((d + 90) * Math.PI / 180);'
'double y = Cy + 3 * Math.sin((d + 90) * Math.PI / 180);`
this gives me mixed results, I mean sometimes it's where I think it should be and other times its quite wrong.
Assuming Cx = 0.500, Cy = 0.500
Sample Data: Result:
Deg = 0 x = 2 / y = 5
Deg = 90 x = -1 / y = 2
Deg = 125 x = -0.457 / y = 0.297
Deg = 159 x = 0.924 / y = -0.800
I realize I am only calculating one point at this point but do you have any suggestions on how to get the first point working? at say 90 degrees from whatever degree I start with?
x = Cx + r * Math.cos( (d+90) * Math.PI / 180 );
y = Cy + r * Math.sin( (d+90) * Math.PI / 180 );
Seems that this is the correct formula for what I was trying to accomplish. This will take any value for Cx/Cy's origin add the Radius r, then calculate the degrees + 90 and convert to radians.. Once all that magic takes place, you're left with an x/y coord that is 90 degrees of where you started.

How to find endpoint coordinates with given start, length, and euler angles

I'm working on some 3d fractals... If I take any arbitrary point (x,y,z), start from there, and then draw a line of given length "d", in a direction defined by Euler angles... (by rotation A about the x-axis, B about the y-axis, and C about the z-axis) -- and then calculate the resulting endpoint of the line.
This would be simple in 2 dimensions, as I could find the endpoint like:
endX = beginX + d * cos(angle)
endY = beginY + d * sin(angle)
Basically, I need to fill in the blanks here:
endX = beginX + d * (??)
endY = beginY + d * (??)
endZ = beginZ + d * (??)
Where I only know angles defined by 3 rotations, 1 about each axis

How to transform mouse location in isometric tiling map?

So I've managed myself to write the first part (algorithm) to calculate each tile's position where should it be placed while drawing this map (see bellow). However I need to be able to convert mouse location to the appropriate cell and I've been almost pulling my hair off because I can't figure out a way how to get the cell from mouse location. My concern is that it involves some pretty high math or something i'm just something easy i'm not capable to notice.
For example if the mouse position is 112;35 how do i calculate/transform it to to get that the cell is 2;3 at that position?
Maybe there is some really good math-thinking programmer here who would help me on this or someone who knows how to do it or can give some information?
var cord:Point = new Point();
cord.x = (x - 1) * 28 + (y - 1) * 28;
cord.y = (y - 1) * 14 + (x - 1) * (- 14);
Speaking of the map, each cell (transparent tile 56x28 pixels) is placed in the center of the previous cell (or at zero position for the cell 1;1), above is the code I use for converting cell-to-position. I tried lot of things and calculations for position-to-cell but each of them failed.
Edit:
After reading lot of information it seems that using off screen color map (where colors are mapped to tiles) is the fastest and most efficient solution?
I know this is an old post, but I want to update this since some people might still look for answers to this issue, just like I was earlier today. However, I figured this out myself. There is also a much better way to render this so you don't get tile overlapping issues.
The code is as simple as this:
mouse_grid_x = floor((mouse_y / tile_height) + (mouse_x / tile_width));
mouse_grid_y = floor((-mouse_x / tile_width) + (mouse_y / tile_height));
mouse_x and mouse_y are mouse screen coordinates.
tile_height and tile_width are actual tile size, not the image itself. As you see on my example picture I've added dirt under my tile, this is just for easier rendering, actual size is 24 x 12. The coordinates are also "floored" to keep the result grid x and y rounded down.
Also notice that I render these tiles from the y=0 and x=tile_with / 2 (red dot). This means my 0,0 actually starts at the top corner of the tile (tilted) and not out in open air. See these tiles as rotated squares, you still want to start from the 0,0 pixel.
Tiles will be rendered beginning with the Y = 0 and X = 0 to map size. After first row is rendered you skip a few pixels down and to the left. This will make the next line of tiles overlap the first one, which is a great way to keep the layers overlapping coorectly. You should render tiles, then whatever in on that tile before moving on to the next.
I'll add a render example too:
for (yy = 0; yy < map_height; yy++)
{
for (xx = 0; xx < map_width; xx++)
{
draw tiles here with tile coordinates:
tile_x = (xx * 12) - (yy * 12) - (tile_width / 2)
tile_y = (yy * 6) + (xx * 6)
also draw whatever is on this tile here before moving on
}
}
(1) x` = 28x -28 + 28y -28 = 28x + 28y -56
(2) y` = -14x +14 +14y -14 = -14x + 14y
Transformation table:
[x] [28 28 -56 ] = [x`]
[y] [-14 14 0 ] [y`]
[1] [0 0 1 ] [1 ]
[28 28 -56 ] ^ -1
[-14 14 0 ]
[0 0 1 ]
Calculate that with a plotter ( I like wims )
[1/56 -1/28 1 ]
[1/56 1/28 1 ]
[0 0 1 ]
x = 1/56*x` - 1/28y` + 1
y = 1/56*x` + 1/28y` + 1
I rendered the tiles like above.
the sollution is VERY simple!
first thing:
my Tile width and height are both = 32
this means that in isometric view,
the width = 32 and height = 16!
Mapheight in this case is 5 (max. Y value)
y_iso & x_iso == 0 when y_mouse=MapHeight/tilewidth/2 and x_mouse = 0
when x_mouse +=1, y_iso -=1
so first of all I calculate the "per-pixel transformation"
TileY = ((y_mouse*2)-((MapHeight*tilewidth)/2)+x_mouse)/2;
TileX = x_mouse-TileY;
to find the tile coordinates I just devide both by tilewidth
TileY = TileY/32;
TileX = TileX/32;
DONE!!
never had any problems!
I've found algorithm on this site http://www.tonypa.pri.ee/tbw/tut18.html. I couldn't get it to work for me properly, but I change it by trial and error to this form and it works for me now.
int x = mouse.x + offset.x - tile[0;0].x; //tile[0;0].x is the value of x form witch map was drawn
int y = mouse.y + offset.y;
double _x =((2 * y + x) / 2);
double _y= ((2 * y - x) / 2);
double tileX = Math.round(_x / (tile.height - 1)) - 1;
double tileY = Math.round(_y / (tile.height - 1));
This is my map generation
for(int x=0;x<max_X;x++)
for(int y=0;y<max_Y;y++)
map.drawImage(image, ((max_X - 1) * tile.width / 2) - ((tile.width - 1) / 2 * (y - x)), ((tile.height - 1) / 2) * (y + x));
One way would be to rotate it back to a square projection:
First translate y so that the dimensions are relative to the origin:
x0 = x_mouse;
y0 = y_mouse-14
Then scale by your tile size:
x1 = x/28; //or maybe 56?
y1 = y/28
Then rotate by the projection angle
a = atan(2/1);
x_tile = x1 * cos(a) - y1 * sin(a);
y_tile = y1 * cos(a) + x1 * sin(a);
I may be missing a minus sign, but that's the general idea.
Although you didn't mention it in your original question, in comments I think you said you're programming this in Flash. In which case Flash comes with Matrix transformation functions. The most robust way to convert between coordinate systems (eg. to isometric coordinates) is using Matrix transformations:
http://help.adobe.com/en_US/FlashPlatform/reference/actionscript/3/flash/geom/Matrix.html
You would want to rotate and scale the matrix in the inverse of how you rotated and scaled the graphics.

Calculate largest inscribed rectangle in a rotated rectangle

I'm trying to find the best way to calculate the biggest (in area) rectangle which can be contained inside a rotated rectangle.
Some pictures should help (I hope) in visualizing what I mean:
The width and height of the input rectangle is given and so is the angle to rotate it. The output rectangle is not rotated or skewed.
I'm going down the longwinded route which I'm not even sure if it will handle the corner cases (no pun intended). I'm certain there is an elegant solution to this. Any tips?
EDIT: The output rectangle points don't necessarily have to touch the input rectangles edges. (Thanks to Mr E)
I just came here looking for the same answer. After shuddering at the thought of so much math involved, I thought I would resort to a semi-educated guess. Doodling a bit I came to the (intuitive and probably not entirely exact) conclusion that the largest rectangle is proportional to the outer resulting rectangle, and its two opposing corners lie at the intersection of the diagonals of the outer rectangle with the longest side of the rotated rectangle. For squares, any of the diagonals and sides would do... I guess I am happy enough with this and will now start brushing the cobwebs off my rusty trig skills (pathetic, I know).
Minor update... Managed to do some trig calculations. This is for the case when the Height of the image is larger than the Width.
Update. Got the whole thing working. Here is some js code. It is connected to a larger program, and most variables are outside the scope of the functions, and are modified directly from within the functions. I know this is not good, but I am using this in an isolated situation, where there will be no confusion with other scripts: redacted
I took the liberty of cleaning the code and extracting it to a function:
function getCropCoordinates(angleInRadians, imageDimensions) {
var ang = angleInRadians;
var img = imageDimensions;
var quadrant = Math.floor(ang / (Math.PI / 2)) & 3;
var sign_alpha = (quadrant & 1) === 0 ? ang : Math.PI - ang;
var alpha = (sign_alpha % Math.PI + Math.PI) % Math.PI;
var bb = {
w: img.w * Math.cos(alpha) + img.h * Math.sin(alpha),
h: img.w * Math.sin(alpha) + img.h * Math.cos(alpha)
};
var gamma = img.w < img.h ? Math.atan2(bb.w, bb.h) : Math.atan2(bb.h, bb.w);
var delta = Math.PI - alpha - gamma;
var length = img.w < img.h ? img.h : img.w;
var d = length * Math.cos(alpha);
var a = d * Math.sin(alpha) / Math.sin(delta);
var y = a * Math.cos(gamma);
var x = y * Math.tan(gamma);
return {
x: x,
y: y,
w: bb.w - 2 * x,
h: bb.h - 2 * y
};
}
I encountered some problems with the gamma-calculation, and modified it to take into account in which direction the original box is the longest.
-- Magnus Hoff
Trying not to break tradition putting the solution of the problem as a picture:)
Edit:
Third equations is wrong. The correct one is:
3.w * cos(α) * X + w * sin(α) * Y - w * w * sin(α) * cos(α) - w * h = 0
To solve the system of linear equations you can use Cramer rule, or Gauss method.
First, we take care of the trivial case where the angle is zero or a multiple of pi/2. Then the largest rectangle is the same as the original rectangle.
In general, the inner rectangle will have 3 points on the boundaries of the outer rectangle. If it does not, then it can be moved so that one vertex will be on the bottom, and one vertex will be on the left. You can then enlarge the inner rectangle until one of the two remaining vertices hits a boundary.
We call the sides of the outer rectangle R1 and R2. Without loss of generality, we can assume that R1 <= R2. If we call the sides of the inner rectangle H and W, then we have that
H cos a + W sin a <= R1
H sin a + W cos a <= R2
Since we have at least 3 points on the boundaries, at least one of these inequality must actually be an equality. Let's use the first one. It is easy to see that:
W = (R1 - H cos a) / sin a
and so the area is
A = H W = H (R1 - H cos a) / sin a
We can take the derivative wrt. H and require it to equal 0:
dA/dH = ((R1 - H cos a) - H cos a) / sin a
Solving for H and using the expression for W above, we find that:
H = R1 / (2 cos a)
W = R1 / (2 sin a)
Substituting this in the second inequality becomes, after some manipulation,
R1 (tan a + 1/tan a) / 2 <= R2
The factor on the left-hand side is always at least 1. If the inequality is satisfied, then we have the solution. If it isn't satisfied, then the solution is the one that satisfies both inequalities as equalities. In other words: it is the rectangle which touches all four sides of the outer rectangle. This is a linear system with 2 unknowns which is readily solved:
H = (R2 cos a - R1 sin a) / cos 2a
W = (R1 cos a - R2 sin a) / cos 2a
In terms of the original coordinates, we get:
x1 = x4 = W sin a cos a
y1 = y2 = R2 sin a - W sin^2 a
x2 = x3 = x1 + H
y3 = y4 = y2 + W
Edit: My Mathematica answer below is wrong - I was solving a slightly different problem than what I think you are really asking.
To solve the problem you are really asking, I would use the following algorithm(s):
On the Maximum Empty Rectangle Problem
Using this algorithm, denote a finite amount of points that form the boundary of the rotated rectangle (perhaps a 100 or so, and make sure to include the corners) - these would be the set S decribed in the paper.
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For posterity's sake I have left my original post below:
The inside rectangle with the largest area will always be the rectangle where the lower mid corner of the rectangle (the corner near the alpha on your diagram) is equal to half of the width of the outer rectangle.
I kind of cheated and used Mathematica to solve the algebra for me:
From this you can see that the maximum area of the inner rectangle is equal to 1/4 width^2 * cosecant of the angle times the secant of the angle.
Now I need to figure out what is the x value of the bottom corner for this optimal condition. Using the Solve function in mathematica on my area formula, I get the following:
Which shows that the x coordinate of the bottom corner equals half of the width.
Now just to make sure, I'll going to test our answer empirically. With the results below you can see that indeed the highest area of all of my tests (definately not exhaustive but you get the point) is when the bottom corner's x value = half of the outer rectangle's width.
#Andri is not working correctly for image where width > height as I tested.
So, I fixed and optimized his code by such way (with only two trigonometric functions):
calculateLargestRect = function(angle, origWidth, origHeight) {
var w0, h0;
if (origWidth <= origHeight) {
w0 = origWidth;
h0 = origHeight;
}
else {
w0 = origHeight;
h0 = origWidth;
}
// Angle normalization in range [-PI..PI)
var ang = angle - Math.floor((angle + Math.PI) / (2*Math.PI)) * 2*Math.PI;
ang = Math.abs(ang);
if (ang > Math.PI / 2)
ang = Math.PI - ang;
var sina = Math.sin(ang);
var cosa = Math.cos(ang);
var sinAcosA = sina * cosa;
var w1 = w0 * cosa + h0 * sina;
var h1 = w0 * sina + h0 * cosa;
var c = h0 * sinAcosA / (2 * h0 * sinAcosA + w0);
var x = w1 * c;
var y = h1 * c;
var w, h;
if (origWidth <= origHeight) {
w = w1 - 2 * x;
h = h1 - 2 * y;
}
else {
w = h1 - 2 * y;
h = w1 - 2 * x;
}
return {
w: w,
h: h
}
}
UPDATE
Also I decided to post the following function for proportional rectange calculating:
calculateLargestProportionalRect = function(angle, origWidth, origHeight) {
var w0, h0;
if (origWidth <= origHeight) {
w0 = origWidth;
h0 = origHeight;
}
else {
w0 = origHeight;
h0 = origWidth;
}
// Angle normalization in range [-PI..PI)
var ang = angle - Math.floor((angle + Math.PI) / (2*Math.PI)) * 2*Math.PI;
ang = Math.abs(ang);
if (ang > Math.PI / 2)
ang = Math.PI - ang;
var c = w0 / (h0 * Math.sin(ang) + w0 * Math.cos(ang));
var w, h;
if (origWidth <= origHeight) {
w = w0 * c;
h = h0 * c;
}
else {
w = h0 * c;
h = w0 * c;
}
return {
w: w,
h: h
}
}
Coproc solved this problem on another thread (https://stackoverflow.com/a/16778797) in a simple and efficient way. Also, he gave a very good explanation and python code there.
Below there is my Matlab implementation of his solution:
function [ CI, T ] = rotateAndCrop( I, ang )
%ROTATEANDCROP Rotate an image 'I' by 'ang' degrees, and crop its biggest
% inner rectangle.
[h,w,~] = size(I);
ang = deg2rad(ang);
% Affine rotation
R = [cos(ang) -sin(ang) 0; sin(ang) cos(ang) 0; 0 0 1];
T = affine2d(R);
B = imwarp(I,T);
% Largest rectangle
% solution from https://stackoverflow.com/a/16778797
wb = w >= h;
sl = w*wb + h*~wb;
ss = h*wb + w*~wb;
cosa = abs(cos(ang));
sina = abs(sin(ang));
if ss <= 2*sina*cosa*sl
x = .5*min([w h]);
wh = wb*[x/sina x/cosa] + ~wb*[x/cosa x/sina];
else
cos2a = (cosa^2) - (sina^2);
wh = [(w*cosa - h*sina)/cos2a (h*cosa - w*sina)/cos2a];
end
hw = flip(wh);
% Top-left corner
tl = round(max(size(B)/2 - hw/2,1));
% Bottom-right corner
br = tl + round(hw);
% Cropped image
CI = B(tl(1):br(1),tl(2):br(2),:);
sorry for not giving a derivation here, but I solved this problem in Mathematica a few days ago and came up with the following procedure, which non-Mathematica folks should be able to read. If in doubt, please consult http://reference.wolfram.com/mathematica/guide/Mathematica.html
The procedure below returns the width and height for a rectangle with maximum area that fits into another rectangle of width w and height h that has been rotated by alpha.
CropRotatedDimensionsForMaxArea[{w_, h_}, alpha_] :=
With[
{phi = Abs#Mod[alpha, Pi, -Pi/2]},
Which[
w == h, {w,h} Csc[phi + Pi/4]/Sqrt[2],
w > h,
If[ Cos[2 phi]^2 < 1 - (h/w)^2,
h/2 {Csc[phi], Sec[phi]},
Sec[2 phi] {w Cos[phi] - h Sin[phi], h Cos[phi] - w Sin[phi]}],
w < h,
If[ Cos[2 phi]^2 < 1 - (w/h)^2,
w/2 {Sec[phi], Csc[phi]},
Sec[2 phi] {w Cos[phi] - h Sin[phi], h Cos[phi] - w Sin[phi]}]
]
]
Here is the easiest way to do this... :)
Step 1
//Before Rotation
int originalWidth = 640;
int originalHeight = 480;
Step 2
//After Rotation
int newWidth = 701; //int newWidth = 654; //int newWidth = 513;
int newHeight = 564; //int newHeight = 757; //int newHeight = 664;
Step 3
//Difference in height and width
int widthDiff ;
int heightDiff;
int ASPECT_RATIO = originalWidth/originalHeight; //Double check the Aspect Ratio
if (newHeight > newWidth) {
int ratioDiff = newHeight - newWidth;
if (newWidth < Constant.camWidth) {
widthDiff = (int) Math.floor(newWidth / ASPECT_RATIO);
heightDiff = (int) Math.floor((originalHeight - (newHeight - originalHeight)) / ASPECT_RATIO);
}
else {
widthDiff = (int) Math.floor((originalWidth - (newWidth - originalWidth) - ratioDiff) / ASPECT_RATIO);
heightDiff = originalHeight - (newHeight - originalHeight);
}
} else {
widthDiff = originalWidth - (originalWidth);
heightDiff = originalHeight - (newHeight - originalHeight);
}
Step 4
//Calculation
int targetRectanleWidth = originalWidth - widthDiff;
int targetRectanleHeight = originalHeight - heightDiff;
Step 5
int centerPointX = newWidth/2;
int centerPointY = newHeight/2;
Step 6
int x1 = centerPointX - (targetRectanleWidth / 2);
int y1 = centerPointY - (targetRectanleHeight / 2);
int x2 = centerPointX + (targetRectanleWidth / 2);
int y2 = centerPointY + (targetRectanleHeight / 2);
Step 7
x1 = (x1 < 0 ? 0 : x1);
y1 = (y1 < 0 ? 0 : y1);
This is just an illustration of Jeffrey Sax's solution above, for my future reference.
With reference to the diagram above, the solution is:
(I used the identity tan(t) + cot(t) = 2/sin(2t))

Find if an angle is within X degrees from another

I need an algorithm to figure out if one angle is within a certain amount of degrees from another angle.
My first thought was (a-x < b) && (a+x > b), but it fails when it has to work with angles that wrap around from -179 to 180.
In the diagram above, the region (green) that the angle must be between wraps between the negative and positive sides. How can I determine whether the angle (the red line) falls inside this region?
try this formula:
360-(|a-b|)%360<x || (|a-b|)%360<x
Or, in PHP:
<?php
$b = 10;
$angle1 = -179;
$angle2 = 180;
$diff = $angle1 - $angle2;
if(abs($diff % 360) <= $b || (360-abs($diff % 360))<=$b) {
echo "yes";
} else {
echo "no";
}
?>
As Marcel rightly points out, modulo on negative numbers is potentially problematic. Also, what is the difference between 355 and 5 degrees? It might be worked out to be 350 degrees but 10 degrees is probably what people are expecting. We make the following assumptions:
we want the smallest positive angle between two other angles so 0 <= diff <= 180;
we are working in degrees. If radians, substitute 360 for 2*PI;
angles can be positive or negative can be outside the range -360 < x < 360 where x is an input angle and
order of input angles or the direction of the difference is irrelevant.
Inputs: angles a and b. So the algorithm is simply:
Normalize a and b to 0 <= x < 360;
Compute the shortest angle between the two normal angles.
For the first step, to convert the angle to the desired range, there are two possibilities:
x >= 0: normal = x % 360
x < 0: normal = (-x / 360 + 1) * 360 + x
The second is designed to remove any ambiguity on the difference in interpretation of negative modulus operations. So to give a worked example for x = -400:
-x / 360 + 1
= -(-400) / 360 + 1
= 400 / 360 + 1
= 1 + 1
= 2
then
normal = 2 * 360 + (-400)
= 320
so for inputs 10 and -400 the normal angles are 10 and 320.
Now we calculate the shortest angle between them. As a sanity check, the sum of those two angles must be 360. In this case the possibilities are 50 and 310 (draw it and you'll see this). To work these out:
normal1 = min(normal(a), normal(b))
normal2 = max(normal(a), normal(b))
angle1 = normal2 - normal1
angle2 = 360 + normal1 - normal2
So for our example:
normal1 = min(320, 10) = 10
normal2 = max(320, 10) = 320
angle1 = normal2 - normal1 = 320 - 10 = 310
angle2 = 360 + normal1 - normal2 = 360 + 10 - 320 = 50
You'll note normal1 + normal2 = 360 (and you can even prove this will be the case if you like).
Lastly:
diff = min(normal1, normal2)
or 50 in our case.
You can also use a dot product:
cos(a)*cos(b) + sin(a)*sin(b) >= cos(x)
For a radius of 1, the distance between the line endpoints is 2sin((a-b/2). So throw away the 2 since you are only interested in a comparison, and compare sin(x/2) with sin((a-b)/2). The trig functions take care of all the wrapping.
c++ implementation:
float diff = fabsf(angle1 - angle2);
bool isInRange = fmodf(diff, 360.0f) <= ANGLE_RANGE ||
360.0f - fmodf(diff, 360.0f) <= ANGLE_RANGE;

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