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====== Electric Drift ====== | ====== Electric Drift ====== | ||
- | A charged particle will move in a circular path in a magnetic field if there is no component of its velocity along the field. If there is a component | + | |
+ | A charged particle will rotate | ||
===== - E-cross-B Drift ===== | ===== - E-cross-B Drift ===== | ||
- | Consider | + | |
+ | Suppose | ||
m˙v∥=qE∥m˙v∥=qE∥ | m˙v∥=qE∥m˙v∥=qE∥ | ||
- | which results in acceleration along the magnetic field. However, in most plasmas of the solar system, | + | which results in an acceleration along the magnetic field. However, in most plasmas of the solar system, |
$$\begin{align*} | $$\begin{align*} | ||
Line 14: | Line 16: | ||
\end{align*}$$ | \end{align*}$$ | ||
- | where ˙vx=(qB/m)vy+qEx/m˙vx=(qB/m)vy+qEx/m and ωg=qB/mωg=qB/m. For the y-component, there is no electric field. By differentiating | + | because |
$$\begin{align*} | $$\begin{align*} | ||
& \ddot{v}_x = - \omega_g^2 v_x \\ | & \ddot{v}_x = - \omega_g^2 v_x \\ | ||
- | & \ddot{v}_y = - \omega_g^2 \left(v_y + \frac{E_x}{B}\right) | + | & \ddot{v}_y = - \omega_g^2 \left(v_y+\frac{E_x}{B}\right) |
\end{align*}$$ | \end{align*}$$ | ||
- | These equations resemble the [[em-gyration|gyration | + | which looks identical to [[em-gyration|the gyration |
- | vE=E×BB2vE=E×BB2 | + | vE=E×BB2vE=E×BB2 |
- | which does not depend on the electric charge, | + | which does not depend on the electric charge, |
{{https:// | {{https:// | ||
- | Here, the E-field is perpendicular to the B-field, and the plane of gyration for both an ion and an electron | + | Here, the E-field is perpendicular to the B-field, and we see the gyration planes |
- | The true explanation of the drift lies in the Lorentz transformation of the electric field in the frame of the moving charge. In the moving | + | The actual |
- | E′=E+v×B=0E′=E+v×B=0 | + | E′=E+v×B=0E′=E+v×B=0 |
- | because the charge is considered | + | because the charge is assumed to be free. Therefore, |
- | E=−v×BE=−v×B | + | E=−v×BE=−v×B |
- | Taking the cross product of both sides with the B-field | + | Taking the cross product of both sides with the B-field |
===== - Polarization Drift ===== | ===== - Polarization Drift ===== | ||
- | Another drift relation can be derived directly from the equation of motion of a charge in the presence of E and B fields. Taking the cross product of both sides of the equation of motion with B/B2B/B2, | ||
- | $$\begin{align*} | + | From the equation of motion of a charge in E and B fields, the above equation and another drift relation can be derived directly. Taking the cross product of both sides of the equation of motion with $\mathbf{B}/B^2$, we get |
- | & m\frac{d\mathbf{v}}{dt} \times \frac{\mathbf{B}}{B^2} = q\frac{\mathbf{E} \times \mathbf{B}}{B^2} + \frac{q}{B^2} (\mathbf{B} | + | |
- | & \Rightarrow \frac{m}{q} \frac{d\mathbf{v}}{dt} \times \frac{\mathbf{B}}{B^2} = \frac{\mathbf{E} \times \mathbf{B}}{B^2} + \frac{q}{B^2}[(\mathbf{B} \cdot \mathbf{B})\mathbf{B} - (\mathbf{B} \cdot \mathbf{v})\mathbf{B}] \\ | + | |
- | & \Rightarrow \mathbf{v} - \frac{\mathbf{B} (\mathbf{v} \cdot \mathbf{B})}{B^2} = \frac{\mathbf{E} \times \mathbf{B}}{B^2} - \frac{m}{q} \frac{d\mathbf{v}}{dt} \times \frac{\mathbf{B}}{B^2} | + | |
- | \end{align*}$$ | + | |
- | where the two terms on the left together represent a perpendicular velocity vector, and the first term on the right is the E-cross-B drift. If we assume that all temporal changes during a gyro-period are negligible, this perpendicular velocity can be thought of as the perpendicular drift velocity $\mathbf{v}_d$. Thus, | + | \begin{align*} |
+ | & m\frac{d\mathbf{v}}{dt}\times\frac{\mathbf{B}}{B^2} = q\frac{\mathbf{E}\times\mathbf{B}}{B^2} + \frac{q}{B^2} (\mathbf{B}\times\mathbf{v}\times\mathbf{B}) \\ | ||
+ | & \Rightarrow \frac{m}{q}\frac{d\mathbf{v}}{dt}\times\frac{\mathbf{B}}{B^2} = \frac{\mathbf{E}\times\mathbf{B}}{B^2} + \frac{q}{B^2}[(\mathbf{B}\cdot\mathbf{B})\mathbf{B} | ||
+ | & \Rightarrow | ||
+ | \end{align*} | ||
- | $$ \mathbf{v}_d | + | where the two terms on the left give a perpendicular velocity vector, and the first term on the right is the E-cross-B drift. Assuming any temporal changes within the gyro-period are negligible, this perpendicular velocity can be considered as the perpendicular drift velocity |
- | Since we know from the Lorentz transformation that v×B=−Ev×B=−E and the gyro-frequency ωg=qB/mωg=qB/m, the last term on the right side of the equation is known as polarization drift: | + | vd=vE−mqB2ddt(v×B)=vE+1ωgBdE⊥dtvd=vE−mqB2ddt(v×B)=vE+1ωgBdE⊥dt |
+ | |||
+ | because | ||
vp=1ωgBdE⊥dtvp=1ωgBdE⊥dt | vp=1ωgBdE⊥dtvp=1ωgBdE⊥dt | ||
- | This drift differs from E-cross-B drift in at least two ways: it is proportional to the particle’s mass and also depends on its charge; both of these terms are related to the gyro-frequency. | + | which differs from E-cross-B drift in at least two ways. This drift is proportional to the particle's mass and also depends on its charge; both terms are found in the gyro-frequency. The direction of polarization drift is along the electric field, but it works in opposite directions for electrons and ions. The resulting current is |
+ | |||
+ | jP=nee(vPi−vPe)=ne(mi+me)B2dE⊥dtjP=nee(vPi−vPe)=ne(mi+me)B2dE⊥dt | ||
+ | |||
+ | which drives electrons and ions in opposite directions and ionizes the plasma. Since the mass of ions is much greater than that of electrons, polarization current primarily arises through ions, as the mass of electrons can be considered negligible. | ||
+ | |||
+ | If the electric field is inhomogeneous in both time and space, corrections might be needed in the two terms of the drift velocity vdvd. In that case, the complete relation becomes | ||
+ | |||
+ | \begin{align*} | ||
+ | \mathbf{v}_d & | ||
+ | &= \left(1+\frac{1}{4}r_g^2\nabla^2\right) \frac{\mathbf{E}\times\mathbf{B}}{B^2} + \frac{1}{\omega_g B} \left(\frac{\partial}{\partial t}+\mathbf{v}\cdot\nabla\right) \mathbf{E}_\perp | ||
+ | \end{align*} | ||
+ | |||
+ | where the first term takes the second spatial derivative (∇2∇2) of the cross product of the electric and magnetic fields, and the second term takes both temporal and spatial derivatives of the perpendicular electric field. | ||
+ | The second-order effect is called //finite Larmor radius effect//, which only applies when the electric field is inhomogeneous within the gyration orbit. The notation v⋅∇v⋅∇ indicates a convective derivative, measuring how the field changes due to the motion of the electron within the electric field. These two corrections to the electric field are used here without derivation. |
un/electric-drift.1730266514.txt.gz · Last modified: 2024/10/29 23:35 by asad