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Question
Help! Can you give advice on solving this?

Show that: m(dv_z/ dt) = -mu (@B/@z)

where @ are partials, and mu is a constant of the motion
Let there be a slowly-convergiing magnetic field: B(r, z, phi)= B_rr^ + B_zz^

where the field is axi-symmetric and assume: B_r^2 << B_z^2

and B_r = r/2[ dB_z/ dz]

Answer
Hello,

You certainly have a lot of plasma physics problems these days, don't you?

The key point to note in the solution is that the field is axisymmetric so that

B_phi = 0 and @/ @phi = 0

(Note – the field designation is also more accurately B(r, phi, z))

To proceed with your working you will need the force-motion eqn.

F = q(v X B)

And be aware that you have to resolve v, B into components as per the vector cross product function.

This means, you need to find: F_r,   F_phi, and F_z

To remind you, the basics of the cross-product in matrix form are given here:

http://www.physics.uoguelph.ca/tutorials/torque/Q.torque.cross.html


Now, you should be able to obtain for your case:

F_r = q(v_phiB_z – v_zB_phi)

F_phi = q(-v_rB_z + v_zB_r)

F_z = q( v_rB_phi – v_phi B_r)

Since we know B_phi = 0, the above reduces to:


F_r = q(v_phiB_z)

F_phi = q(-v_rB_z + v_zB_r)

F_z = -q( v_phi B_r)

Now, for the motion with which you’re concerned – the terms for the usual Larmor gyration are not needed, so the terms in B_z are omitted. Same with the “v_zB_r” term since it vanishes on the z-axis.

Thus, you are left with:

F_z = -q v_phi B_r

From one of your assumptions you have:  B_r = r/2[dB_z/ dz]

So:

F_z = - q v_phi (r/2)[dB_z/ dz] =  -(q v_phi r)/ 2  [dB_z/ dz]

From here you should be able to complete the solution fairly quickly.

Tips:

Take an average over one gyration period. Let the guiding center lie on the z-axis, so then:

v_phi = const.

(during a gyration)

If then, r = r_c (guiding center radius) the average force can be found

Further hint: Go back to the previous problem you asked about, concerning gyration periods, times, gyro-frequency etc!

With the correct substitutions you should have your result!  

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Philip A. Stahl

Expertise

I specialize in stellar and solar astrophysics. Can answer any questions pertaining to these areas, the spectroscopic analysis of stars – as well as the magneto-hydrodynamics of sunspots and solar flares. Sorry – No homework problems done or research projects! I will provide hints on solutions.

Experience

Have published papers on the relationship between sunspot morphology and solar flares; discovery of SID flares related to this, constructed computerized stellar models; MHD research.

Organizations
American Astronomical Society (Solar physics and Dynamical astronomy divisions), American Geophysical Union, American Mathematical Society, Intertel.

Publications
Solar Physics, Journal of the Royal Astronomical Society of Canada, Journal of the Barbados Astronomical Society, Meudon Solar Flare Proceedings (Meudon, France). Books: 'Selected Analyses in Solar Flare Plasma Dynamics', 'Physics Notes for Advanced Level'.

Education/Credentials
B.A. degree in Astronomy; M.Phil. degree in Physics - specializing in solar physics.

Awards and Honors
Postgraduate research award- Barbados government; Studentship Award in Solar Physics - American Astronomical Society

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