(1) A hydrogen plasma has a number density of 5 atoms/cm, and there is a magnetic field
G. What is the Alfvén speed in this plasma?
(2) An Alfvén wave is propagating in the plasma described in problem # 1. It has an amplitude of
(as defined in lecture) and a wavelength of
km. What is the maximum acceleration of the plasma due to the presence of this wave?
(3) If the Alfvén wave described in Problem # 2 were propagating in a single direction, what would the associated energy flux be? Hint: The energy flux is given by where is the energy density and is the speed at which the energy is transported.
(4) We see the solar corona mainly because photospheric light is Thomson scattered out of its original direction of propagation and into our line of sight. An empirical estimate of the electron density in the solar corona is
(1) |
(5) Consider an imaginary spherical surface of radius in a moving, constant density fluid. Measurements show that the fluid velocity on the surface of the sphere is given by
(2) |
(6) Assume that a velocity field is given as the gradient of a scalar potential,
(3) |
(7) Problem 11.11
(8) Problem 11.12