How Do Non-Perpendicular Unit Vectors Affect Coordinate Transformation?

unscientific
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Homework Statement



The x-y coordinates are being transformed into the u-v coordinates.

Based on the diagram, u lies along x while v makes an angle α with x.

The Attempt at a Solution



The answer defined u and v weirdly..

Shouldn't

x = u

and

y = v sin α

??
 

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unscientific said:
Shouldn't

x = u

and

y = v sin α

??

No. Consider the position vector \mathbf{r}= x\mathbf{e}_x + y\mathbf{e}_y = u\mathbf{e}_u + v\mathbf{e}_v:

You have \mathbf{e}_u = \mathbf{e}_x since the two axes are parallel, but \mathbf{e}_v has both a vertical and a horizontal component and is given by \mathbf{e}_v = \cos\alpha \mathbf{e}_x + \sin\alpha \mathbf{e}_y. Plugging this into the position vector definition gives x\mathbf{e}_x + y\mathbf{e}_y= u \mathbf{e}_x + v( \cos\alpha \mathbf{e}_x + \sin\alpha \mathbf{e}_y), which gives you the relations in your image.
 
Also, does the region of integration R change if we change the variables from (x,y) to (u,v)?


According to the answer, the region R → R', where R' is only σ/2∏ of the original R..
 

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unscientific said:
According to the answer, the region R → R', where R' is only σ/2∏ of the original R..

No, that's not what they are saying. Read it again more carefully, what they are actually claiming is that \int_{0}^{\infty} \int_{0}^{\infty} e^{-r^2} \left| \frac{\partial(x,y)}{\partial(u,v)} \right|dudv = \frac{\alpha}{2\pi} \int_{-\infty}^{\infty} \int_{-\infty}^{\infty} e^{-r^2}dxdy

The integral on the left is only over positive u & y, while the integral on the right is over all (R2) space.
 
gabbagabbahey said:
No, that's not what they are saying. Read it again more carefully, what they are actually claiming is that \int_{0}^{\infty} \int_{0}^{\infty} e^{-r^2} \left| \frac{\partial(x,y)}{\partial(u,v)} \right|dudv = \frac{\alpha}{2\pi} \int_{-\infty}^{\infty} \int_{-\infty}^{\infty} e^{-r^2}dxdy

The integral on the left is only over positive u & y, while the integral on the right is over all (R2) space.

Yup, if you only consider x,y,u,v > 0,

it would be α/(∏/2) for ∫ 0 to infinity..
 
gabbagabbahey said:
No. Consider the position vector \mathbf{r}= x\mathbf{e}_x + y\mathbf{e}_y = u\mathbf{e}_u + v\mathbf{e}_v:

You have \mathbf{e}_u = \mathbf{e}_x since the two axes are parallel, but \mathbf{e}_v has both a vertical and a horizontal component and is given by \mathbf{e}_v = \cos\alpha \mathbf{e}_x + \sin\alpha \mathbf{e}_y. Plugging this into the position vector definition gives x\mathbf{e}_x + y\mathbf{e}_y= u \mathbf{e}_x + v( \cos\alpha \mathbf{e}_x + \sin\alpha \mathbf{e}_y), which gives you the relations in your image.

I don't really understand what you mean...

My main problem here is why do they define u and v as such in the picture?

I thought u and v are defined when you drop a perpendicular line onto the axis?

And it's pretty clear that the lengths u, v they define are shorter than the ones in my picture..
 
unscientific said:
I thought u and v are defined when you drop a perpendicular line onto the axis?

That's the case when your coordinate lines are perpendicular. When they are not, you get what you see in this picture.
 
voko said:
That's the case when your coordinate lines are perpendicular. When they are not, you get what you see in this picture.

Are they defined this way?
 
A coordinate system (on an plane) is defined by its origin and unit vectors \vec{a} and \vec{b}. Any point \vec{p} = u\vec{a} + v\vec{b}. u and v are coordinates. Now if the coordinate unit vectors are not perpendicular, what do you get? Try it on a piece of paper.
 
  • #10
voko said:
A coordinate system (on an plane) is defined by its origin and unit vectors \vec{a} and \vec{b}. Any point \vec{p} = u\vec{a} + v\vec{b}. u and v are coordinates. Now if the coordinate unit vectors are not perpendicular, what do you get? Try it on a piece of paper.

Ah, using vectors everything seems much simpler now! Thank you! :smile:
 
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