Issue |
A&A
Volume 452, Number 1, June II 2006
|
|
---|---|---|
Page(s) | 321 - 330 | |
Section | The Sun | |
DOI | https://doi.org/10.1051/0004-6361:20054285 | |
Published online | 17 May 2006 |
Tearing and Kelvin-Helmholtz instabilities in the heliospheric plasma
1
Department of Astronomy and Space Science, Univ. of Firenze, 50125 Firenze, Italy e-mail: betta@arcetri.astro.it
2
Department of Physics, Univ. of Pisa, 56127 Pisa, Italy
3
Jet Propulsion Laboratory, California Institute of Technology, 91109 Pasadena, CA, USA
Received:
30
September
2005
Accepted:
9
January
2006
We used 2.5D simulations to analyze the magnetohydrodynamic instabilities arising from an initial equilibrium configuration consisting of a plasma jet or wake in the presence of a magnetic field with strong transverse gradients, such as those arising in the solar wind. Our analysis extends previous results by considering both a force-free equilibrium and a pressure-balance condition for a jet in a plasma sheet, along with arbitrary angles between the magnetic field and velocity field. In the force-free case, the jet/wake does not contain a neutral sheet but the field rotates through the flow to invert its polarity. The presence of a magnetic field component aligned with the jet/wake destroys the symmetric nature of the fastest growing modes, leading to asymmetrical wake acceleration (or, equivalently, jet deceleration). In the case of a jet, the instability properties depend both on the magnetic field and flow gradients, as well as on the length of the jet. The results are applied to the post-termination shock jet recently found in 3D global heliospheric simulations, where our analysis confirms and explains the stability properties found in such simulations.
Key words: instabilities / magnetohydrodynamics (MHD) / plasmas / methods: numerical / Sun: solar wind
© ESO, 2006
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.