Resonant Instability of Kink Oscillations in Magnetic Flux Tubes with Siphon Flow

Solar Physics. 2021. Vol. 296. Article 106.

Ruderman M., Petrukhin N.

We study kink oscillations of a straight magnetic tube in the presence of siphon flows. The
tube consists of a core and a transitional or boundary layer. The flow velocity is parallel to
the tube axis, has constant magnitude, and confined in the tube core. The plasma density
is constant in the tube core and it monotonically decreases in the transitional layer to its
value in the surrounding plasma. We use the expression for the decrement/increment previously obtained by Ruderman and Petrukhin (Astron. Astrophys. 631, A31, 2019) to study
the damping and resonant instability of kink oscillations. We show that, depending on the
magnitude of siphon-velocity, resonant absorption can cause either the damping of kink oscillations or their enhancement. There are two threshold velocities: When the flow velocity
is below the first threshold velocity, kink oscillations damp. When the flow velocity is above
the second threshold velocity, the kink oscillation amplitudes grow. Finally, when the flow
velocity is between the two threshold velocities, the oscillation amplitudes do not change.
We apply the theoretical result to kink oscillations of prominence threads. We show that, for
particular values of thread parameters, resonant instability can excite these kink oscillations
 

Keywords: волны, устойчивость, Sun, Солнце, плазма, waves, plasma, Колебания, Stability, Sun: oscillations, magnetohydrodynamics, Магнитогидродинамика