Magnetic field outside a semi-infinite solenoid

In summary, the magnetic field outside a semi-infinite solenoid is characterized by its dependence on the solenoid's current and physical parameters. Unlike a finite solenoid, which has a diminishing external magnetic field, the semi-infinite solenoid produces a relatively uniform magnetic field in the region outside its ends. The field strength decreases with distance from the solenoid and can be calculated using Ampère's law, which highlights the influence of the solenoid's internal magnetic field on the surrounding space. This unique behavior is significant for applications in magnetic field manipulation and electromagnetic theory.
  • #1
Bling Fizikst
85
10
Homework Statement
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Relevant Equations
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The solenoid can be assumed to be a stack of rings of width ##dz## each where ##z:0\to-\infty## . $$i=nIdz$$ $$\sin\theta=\frac{R-r}{l}$$ $$\cos\theta=\frac{z+x}{l}$$ $$dB=\frac{\mu_{\circ}nIR d\varphi dz}{4\pi l^2}$$ Call ##\frac{\mu_{\circ}nIR}{4\pi}=\alpha## $$ B_y =\int dB\cos\theta , B_x=\int dB\sin\theta$$ Doing the computation gives : $$B_y=\frac{2\pi\alpha}{\sqrt{(R-r)^2+x^2}}$$ Similarly , $$B_x=\frac{2\pi\alpha}{R-r}\left(1-\frac{x}{\sqrt{(R-r)^2+x^2}}\right)$$ But it happens to be wrong , not sure where??
 
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  • #2
Surely ##\theta## is a function of ##\phi##.
 
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  • #3
Say Origin O(0,0,0), point of observation ##P(x,y,0)##, the point on a current ring which consistus of the solenoid ##Q(X,R \cos\phi,R\sin\phi)## where X<0
[tex]PQ^2=(x-X)^2+(y-R\cos\phi)^2+(R\sin\phi)^2=(x-X)^2+y^2+R^2-2yR\cos\phi[/tex]
Does it go well with your treatment ? In order to apply Biot Savart law, current vector is proportinal to
[tex](0, -\sin\phi, \cos\phi)[/tex]
Its vector product with vector PQ is proportional to
[tex]\mathbf{e}_x(R \cos 2\phi + y \ \cos \phi)+\mathbf{e_r} (x-X)[/tex]
if my math is good. So we can apply Biot Savart law with integration of ##\phi## and X.
 
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  • #4
haruspex said:
Surely ##\theta## is a function of ##\phi##.
I am absolutely unable to figure out how :cry: . Isn't ##\varphi## present in a plane perpendicular to where ##\theta## is?
 
  • #5
Bling Fizikst said:
I am absolutely unable to figure out how :cry: . Isn't ##\varphi## present in a plane perpendicular to where ##\theta## is?
It's just Pythagoras.
To avoid confusion, I will take the point of interest as being at z' from the solenoid, instead of at x.
In (x,y,z) coordinates, where the negative z axis is the axis of the cylinder, you have a fixed point at (0,r,z'). Your solenoid element is at ##(R\cos(\phi), R\sin(\phi),z)##, where z is negative.
The distance between the two is ##h=\sqrt{R^2\cos^2(\phi)+( R\sin(\phi)-r)^2+(z-z')^2}##. The components of the force are proportional to ##(R\cos(\phi),R\sin(\phi)-r,z-z')h^{-\frac 32}##.
Edit: correction, I doubled up on the square-rooting:
The components of the force are proportional to ##(R\cos(\phi),R\sin(\phi)-r,z-z')h^{-3}##.
 
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  • #6
I would approach this problem differently and exploit the information that we are looking for the field "at a very small distance ##r## from the axis."

I would first integrate the expression for the on-axis field due to a single current loop to find the on-axis field ##B_z(0,z_0)## outside the solenoid at distance ##z_0## from the end. At an off-axis point but at a very small distance ##r## from the axis, one can expect a non-zero radial component and an essentially unchanged axial component, i.e. ##B_z(r,z_0)\approx B_z(0,z_0).## This gives the axial component of the field at the off-axis point ##~(r,z_0)##.

I would then invoke the on-axis divergence relation in cylindrical coordinates $$0=\mathbf {\nabla}\cdot\mathbf B=\frac{1}{r}\left. \frac{\partial(rB_r)}{\partial r}\right |_{z=z_0}+\left. \dfrac{\partial B_z(0,z)}{\partial z}\right |_{z=z_0}$$from which $$d(r B_r)=-\left. \dfrac{\partial B_z(0,z)}{\partial z}\right |_{z=z_0}r~dr.$$ To find the radial component, note that the derivative on the right-hand side can be treated as constant and one can integrate, $$r B_r=-\left. \dfrac{\partial B_z(0,z)}{\partial z}\right |_{z=z_0}\int_0^r r~dr$$to get the radial component of the field at the off-axis point ##~(r,z_0)##.
 
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  • #7
haruspex said:
It's just Pythagoras.
To avoid confusion, I will take the point of interest as being at z' from the solenoid, instead of at x.
In (x,y,z) coordinates, where the negative z axis is the axis of the cylinder, you have a fixed point at (0,r,z'). Your solenoid element is at ##(R\cos(\phi), R\sin(\phi),z)##, where z is negative.
The distance between the two is ##h=\sqrt{R^2\cos^2(\phi)+( R\sin(\phi)-r)^2+(z-z')^2}##. The components of the force are proportional to ##(R\cos(\phi),R\sin(\phi)-r,z-z')h^{-\frac 32}##.
Oh yeah! But now that i realize this . It seems impossible to solve it by integration . I end up with : $$dB=\frac{\mu_{\circ}nIR}{4\pi}\frac{d\varphi\cdot dz}{(z-z')^2+R^2-2rR\sin\varphi}$$
 
  • #8
Bling Fizikst said:
Oh yeah! But now that i realize this . It seems impossible to solve it by integration . I end up with : $$dB=\frac{\mu_{\circ}nIR}{4\pi}\frac{d\varphi\cdot dz}{(z-z')^2+R^2-2rR\sin\varphi}$$
Then consider the method I outlined in post #6.
 
  • #9
Bling Fizikst said:
Oh yeah! But now that i realize this . It seems impossible to solve it by integration . I end up with : $$dB=\frac{\mu_{\circ}nIR}{4\pi}\frac{d\varphi\cdot dz}{(z-z')^2+R^2-2rR\sin\varphi}$$
Shouldn't that denominator quadratic be raised to the power of 3/2?
Don't forget to apply an approximation for small r. And as @kuruman notes, it is the field normal to the axis that is interesting.
 
  • #10
kuruman said:
I would approach this problem differently and exploit the information that we are looking for the field "at a very small distance ##r## from the axis."

I would first integrate the expression for the on-axis field due to a single current loop to find the on-axis field ##B_z(0,z_0)## outside the solenoid at distance ##z_0## from the end. At an off-axis point but at a very small distance ##r## from the axis, one can expect a non-zero radial component and an essentially unchanged axial component, i.e. ##B_z(r,z_0)\approx B_z(0,z_0).## This gives the axial component of the field at the off-axis point ##~(r,z_0)##.

I would then invoke the on-axis divergence relation in cylindrical coordinates $$0=\mathbf {\nabla}\cdot\mathbf B=\frac{1}{r}\left. \frac{\partial(rB_r)}{\partial r}\right |_{z=z_0}+\left. \dfrac{\partial B_z(0,z)}{\partial z}\right |_{z=z_0}$$from which $$d(r B_r)=-\left. \dfrac{\partial B_z(0,z)}{\partial z}\right |_{z=z_0}r~dr.$$ To find the radial component, note that the derivative on the right-hand side can be treated as constant and one can integrate, $$r B_r=-\left. \dfrac{\partial B_z(0,z)}{\partial z}\right |_{z=z_0}\int_0^r r~dr$$to get the radial component of the field at the off-axis point ##~(r,z_0)##.
Beautiful! Extremely sorry for my late response .

Let's say the distance from the opening of the solenoid along its axis is at ##x_{\circ}## instead of general ##x## to avoid confusion . From my first post , $$i=nIdz$$ is flowing through ring of width ##dz## at a distance ##z## beyond the origin .

So , the magnetic field at a general ##x## from the origin should be : $$dB_x= \frac{\mu_{\circ}nIR^2 dz}{2\left(R^2+(x+z)^2\right)^{\frac{3}{2}}}$$ Take $$\lambda = \frac{\mu_{\circ}nIR^2}{2}$$ and $$z+x=t , t: x\to -\infty$$ Now , $$B_x=\int_{x}^{-\infty} \lambda (R^2+t^2)^{-\frac{3}{2}} dt =\gamma\int_{x}^{-\infty} -2R^2 t^{-3} (R^2t^{-2}+1)^{-\frac{3}{2}}\cdot dt $$ where $$\gamma= \lambda\cdot\frac{1}{-2R^2}$$ Now , take $$u=R^2t^{-2}+1$$ and integrate to get $$B_{x_{\circ}}=-2\gamma\left(1-\frac{x_{\circ}}{\sqrt{R^2+x_{\circ}^2}}\right)\cdot dt$$

Now , using $$\nabla\cdot B=\frac{1}{r}\frac{\partial rB_r}{\partial r}+\frac{\partial B_x}{\partial x}\mid_{x=x_{\circ}}=0$$ We get : $$ B_r= \frac{-\gamma rR^2}{(R^2+x_{\circ}^2)^{-\frac{3}{2}}}$$

So , the final answer should be : $$\frac{\mu_{\circ} nI}{2}\left(\left(1-\frac{x_{\circ}}{\sqrt{R^2+x_{\circ}^2}}\right)\hat{x} +\frac{rR^2}{2(R^2+x_{\circ}^2)^{-\frac{3}{2}}}\hat{r}\right)$$
 
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  • #11
There is another method discussed in this video using magnetic force :
 
  • #12
Bling Fizikst said:
So , the final answer should be : $$\frac{\mu_{\circ} nI}{2}\left(\left(1-\frac{x_{\circ}}{\sqrt{R^2+x_{\circ}^2}}\right)\hat{x} +\frac{rR^2}{2(R^2+x_{\circ}^2)^{-\frac{3}{2}}}\hat{r}\right)$$
That's the answer I got.
 
  • #13
I just remembered the formula from the video that we can simply use for the magnetic field on the solenoidal axis (which is again derived from integration) : $$ \frac{\mu_{\circ}nI}{2}(\sin\alpha+\sin\beta)$$ where ##\alpha,\beta## are signed values .

In our case : $$\alpha=\frac{\pi}{2}$$ and $$\sin(-\beta)=\frac{x}{\sqrt{R^2+x^2}}$$ and then proceed with $$\nabla\cdot B=0$$ Saves so much time and labour!
 
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