9–13 Sept 2024
Turin, Italy
Europe/Rome timezone

Modeling of wave dissipation around X-points

Not scheduled
1h
Turin, Italy

Turin, Italy

Centro Congressi Unione Industriali Torino Via Vela, 17 - 10128 Torino
Poster Fundamental mechanisms of solar plasmas: magnetic reconnection, waves, radiation and particle acceleration Coffee break and poster session 1

Description

Oscillations around the X-points play an important role in corona plasma heating. In this paper we investigate resonance absorption around X points. We have found analytical solutions for the Alfven continuum mode in the presence of a guide field. We also drive a jump conditions in the flux coordinates. Using these conditions, we obtain the dispersion relation and solve it numerically to find the frequencies and damping rates. The results show that resonance absorption can be an effective mechanism for damping the waves around the X points.

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