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184_notes:examples:week9_detecting_b [2017/10/24 00:39] – dmcpadden | 184_notes:examples:week9_detecting_b [2021/07/05 21:58] (current) – [Solution] schram45 | ||
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=====Magnetic Field near a Moving Charge===== | =====Magnetic Field near a Moving Charge===== | ||
You are a collector of magnetic field detectors. A fellow detector collector is trying to trim down her collection, and so it's your job to see if an old detector is still working properly, in which case it's yours! Today, you are a magnetic field detector collector, inspector, and hopefully a selector. First, you run a test in which a charged particle (q=15 nC) is sent through the detector, and you look at the detector' | You are a collector of magnetic field detectors. A fellow detector collector is trying to trim down her collection, and so it's your job to see if an old detector is still working properly, in which case it's yours! Today, you are a magnetic field detector collector, inspector, and hopefully a selector. First, you run a test in which a charged particle (q=15 nC) is sent through the detector, and you look at the detector' | ||
- | {{ 184_notes: | + | [{{ 184_notes: |
===Facts=== | ===Facts=== | ||
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===Approximations & Assumptions=== | ===Approximations & Assumptions=== | ||
- | | + | * We are only interested in the B-field at this specific moment in time: As the particle moves some its parameters may change (i.e. velocity, charge...). This assumption gives use fixed variables to work with at this snapshot in time, simplifying down the complexity of the model. |
- | | + | |
===Representations=== | ===Representations=== | ||
* We represent the Biot-Savart Law for magnetic field from a moving point charge as | * We represent the Biot-Savart Law for magnetic field from a moving point charge as | ||
→B=μ04πq→v×→rr3 | →B=μ04πq→v×→rr3 | ||
+ | <WRAP TIP> | ||
+ | ===Approximation=== | ||
+ | We must approximate the particle as a point particle in order to use the magnetic field equation above. Since the problem doesn' | ||
+ | </ | ||
* We represent the situation with diagram given above. | * We represent the situation with diagram given above. | ||
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For Location 2, the →r2 is perpendicular to the velocity vector →v (the angle between them is 90 degrees). When we take this cross product, then: | For Location 2, the →r2 is perpendicular to the velocity vector →v (the angle between them is 90 degrees). When we take this cross product, then: | ||
- | →v×→r2=|→v||→r2|sin(90)=2∗0.5∗1=1 m2s−1 | + | $$\vec{v}\times \vec{r}_2 = |\vec{v}||\vec{r}_2|sin(90)=2*0.5*1= 1 \text{ m}^2\text{s}^{-1} \text{ } \hat{z}$$ |
- | Now we just need to figure out the direction | + | Note that the ˆz comes from using the right hand rule (or rather from taking the cross product of a vector in the ˆx and a vector in the ˆy). If you point your fingers in the direction of the velocity and curl them toward location 2 your thumb would point out of the page (or in the +ˆx direction). |
- | \begin{align*} | + | Finally, for Location 3, we can think about $\vec{r}_3intermsofit′scomponents−thepartthatisparalleltothevelocity(whichwouldbethesameas\vec{r}_1)andthepartthatisperpendiculartothevelocity(whichwouldbethesameas\vec{r}_2$). We just learned if the vectors are parallel, the cross product will give zero - so the horizontal component of $\vec{r}_3$ will not contribute to the magnetic field at Location 3. The only part that will contribute will be the vertical component (which is the same as what we just calculated for magnetic field at Location 2). So, we know already that this cross product will give: |
- | \\ | + | |
- | \vec{v}\times | + | $$\vec{v}\times \vec{r}_3 = 1 \text{ m}^2\text{s}^{-1} \hat{z}$$ |
- | \vec{v}\times \vec{r}_3 | + | |
- | \end{align*} | + | Next, we find the magnitudes of r3, since that is another quantity we need to know in the Biot-Savart Law. Note that even though the cross products |
- | The other two cross-products | + | |
- | Next, we find the magnitudes of r3, since that is another quantity we need to know in the Biot-Savart Law. | ||
\begin{align*} | \begin{align*} | ||
{r_2}^3 &= 0.125 \text{ m}^3 \\ | {r_2}^3 &= 0.125 \text{ m}^3 \\ | ||
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\end{align*} | \end{align*} | ||
- | We don't including location 1 above since we already know the magnetic field is 0 at that location! Below, we give the magnetic field at all three locations. | + | We don't including location 1 above since we already know the magnetic field is 0 at that location! Below, we give the magnetic field at all three locations |
\begin{align*} | \begin{align*} | ||
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\vec{B}_3 &= \frac{\mu_0}{4 \pi}\frac{q\vec{v}\times \vec{r}_3}{{r_3}^3} = 4.2 \text{ nT } \hat{z} | \vec{B}_3 &= \frac{\mu_0}{4 \pi}\frac{q\vec{v}\times \vec{r}_3}{{r_3}^3} = 4.2 \text{ nT } \hat{z} | ||
\end{align*} | \end{align*} | ||
+ | |||
+ | Observation location 3 is the furthest away from our moving point charge and we would expect it to have a smaller magnetic field than location 2, this is reflected in our solution. We also expected the magnetic field at location 1 to be 0 since the velocity and separation vector are parallel for this point (this is always a good thing to look for when approaching a problem with cross products). |