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Ohm's Law and Ambipolar Diffusion

Ohm's Law and Ambipolar Diffusion. Astrophysical Fluid Dynamics E. Battaner. Department of Physics National Tsing Hua University G.T. Chen 2004/12/9. Outline. Basic Properties of Fluid Dynamics Diffusion in Classical Fluid Diffusion in Plasma Fluid

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Ohm's Law and Ambipolar Diffusion

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  1. Ohm's Lawand Ambipolar Diffusion Astrophysical Fluid Dynamics E. Battaner Department of Physics National Tsing Hua University G.T. Chen 2004/12/9

  2. Outline • Basic Properties of Fluid Dynamics • Diffusion in Classical Fluid • Diffusion in Plasma Fluid • Ohm’s Law • Ambipolar Diffusion • Summary

  3. Basic Properties • Boltzmann’s Eq. • Multicomponent fluids • r

  4. Basic Properties • Mean velocity • Peculiar velocity where average then

  5. Basic Properties • Multiply Boltzmann’s eq. by Gi (v) and integrate over velocity space

  6. Basic Properties • This moment eq. is sometimes known as “transfer eq. “ , depending on the choice of Gi • Choosing Gi is a function which has the property of collisional invariance corresponding to the conservation of mass, momentum and energy Mass MomentumEnergy

  7. Basic Properties • According to collisional invariance, the collision term • If Gi=1  continuity eq. • If Gi=mi  continuity eq. of mass • If Gi=(mv2)/2  energy balance eq.

  8. Basic Properties • If Gi=p (momentum) define , of course Sum all species Combine with continuity eq. Eq. of motion

  9. Diffusion in Classical Fluid • To solve the diffusion velocity <Vi>, we take two assumptions where coefficient depending on intermolecular potential for elastic collision model between two rigid sphere reduce mass Sum of the radii of both spheres

  10. Diffusion in Classical Fluid • Define the momentum transfer collision frequency recall

  11. Diffusion in Classical Fluid • For simplicity, take and neglect diffusion acceleration and force consider no viscosity and isothermal

  12. Diffusion in Classical Fluid • Now , solve <Vi> =the friction velocity • For moderate rate of diffusion the procedure converges rapidly, so the friction velocity often can be ignored. where

  13. Diffusion in Classical Fluid • Diffusion coefficient • If consider a binary mixture , let n1<<n2 and isothermal  Di=constant and Fi=0 (Fick’s 1st law) (Fick’s 2nd law) Combine with continuity eq.

  14. Diffusion in Plasma Fluid • Consider plasma fluid, and there are three species ni ,ne ,and nn ( ne = ni ) • Continuity eq.s electrons: (1) ions: (2) neutrals: (3)

  15. Diffusion in Plasma Fluid • (1)x me ,(2)xmi ,(3)xmi individually(mn ~ mi ), and sum all species • (2)-(1) define charge current density

  16. Diffusion in Plasma Fluid • because diffusion fluxes of ions and electrons Ambipolar diffusion flux

  17. Diffusion in Plasma Fluid • The diffusion of ions and electrons has decomposed into 2 kinds of fluxes, one associated with charge current density, and the other called ambipolar diffusion • No ambipolar diffusion will occur in fully ionized plasma

  18. Diffusion in Plasma Fluid • Remember diffusion in classical fluid , we have 2 assumptions • Recall Aj in plasma fluid is from Boltzmann’s eq.

  19. Ohm’s Law • Consider absence of ambipolar difusion • Calculate by using the above two methods Assume external force is not important and ,and T=constant

  20. Ohm’s Law • is often negligible • Assume can be ignored • Define scalar electrical conductivity This is called Ohm’s Law

  21. PS: Ohm’s Law • Consider simple application • Define electrical conductivity tensor

  22. Ohm’s Law • The electrical conductivity tensor is also equal to • Hall charge current density Pederson conductivity where Hall conductivity

  23. Ohm’s Law • For Hall conductivity: When is very high . It is unimportant When , it’s also negligible It becomes important when , it would cause the media being anisotropy • When is very low ,Hall term 0 ,Pederson term  then σ will reduce to isotropic electrical conductivity

  24. Ohm’s Law • When B is very high  is very high the charge current density lies in the direction of , and only the projection of along the direction of is effective in producing it  the σ becomes highly anisotropic

  25. Ohm’s Law • If choosing OX-axis = the direction of B field and it also can reproduce the above properties of the electrical conductivity tensor

  26. Ambipolar Diffusion • Consider a weakly ionized medium with nn >>ne • Calculate the Ai and Ae individually (a) (b)

  27. Ambipolar Diffusion • Consider B field=0  ambipolar diffusion in the absence of magnetic field • Assume j=0 , E=0 ,and solve (a) (b) but Di is not equal to De  the problem should appear in the hypothesis

  28. Ambipolar Diffusion • We must consider the electric field being generated  binding electric field is allowed to existence take The ambipolar diffusion coefficient is twice the ion diffusion coefficient , but lower than De

  29. Ambipolar Diffusion • The binding electric field In the absence of B field , ambipolar diffusion is isotropic

  30. Summary • a • a • Ohm’s Law • Ambipolar Diffusion

  31. Thank You

  32. Introduction to Plasma Theory , Nicholson

  33. E x B Drift

  34. g x B Drift

  35. Alfven Wave

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