A mechanism for parallel electric field generation in the MHD limit: possible implications for the coronal heating problem in the two stage mechanism
arXiv:astro-ph/0606661 · doi:10.1051/0004-6361:20064816
Abstract
We solve numerically ideal, 2.5D, MHD equations in Cartesian coordinates, with a plasma beta of 0.0001 starting from the equilibrium that mimics a footpoint of a large curvature radius solar coronal loop or a polar region plume. On top of such an equilibrium, a purely Alfvénic, linearly polarised, plane wave is launched. In the context of the coronal heating problem a new two stage mechanism of plasma heating is presented by putting emphasis, first, on the generation of parallel electric fields within an ideal MHD description directly, rather than focusing on the enhanced dissipation mechanisms of the Alfvén waves and, second, dissipation of these parallel electric fields via {\it kinetic} effects. It is shown that a single Alfvén wave harmonic with frequency Hz and longitudinal wavelength Mm, for a putative Alfvén speed of 4328 km s, the generated parallel electric field could account for 10% of the necessary coronal heating requirement. We conjecture that wide spectrum (10 Hz) Alfvén waves, based on the observationally constrained spectrum, could provide the necessary coronal heating requirement. The exact amount of energy that could be deposited by such waves through our mechanism of parallel electric field generation can only be calculated once a more complete parametric study is done. Thus, the "theoretical spectrum" of the energy stored in parallel electric fields versus frequency needs to be obtained.
arXiv commentAstron. Astrophys. (accepted, in press) (2006) - FULL paper
References in corpus (11)
- On the Generation, Propagation, and Reflection of Alfven Waves from the Solar Photosphere to the Distant Heliosphere
- Wide-Spectrum Slow Magnetoacoustic Waves in Coronal Loops
- Particle-In-Cell simulations of circularly polarised Alfvén wave phase mixing: a new mechanism for electron acceleration in collisionless plasmas
- A Three Dimensional Magnetohydrodynamic Pulse in a Transversely Inhomogeneous Medium
- A Strongly Nonlinear Alfvenic Pulse in a Transversely Inhomogeneous Medium
- A Weakly Nonlinear Alfvenic Pulse in a Transversely Inhomogeneous Medium
- Phase mixing of a three dimensional magnetohydrodynamic pulse
- Phase mixing of shear Alfven waves as a new mechanism for electron acceleration in collisionless, kinetic plasmas
- Comment on "PIC simulations of circularly polarised Alfvén wave phase mixing: A new mechanism for electron acceleration in collisionless plasmas" by Tsiklauri et al
- A fresh look on the heating mechanisms of the Solar corona
- The Sun as a MHD generator: application of a new heating mechanism for the coronal loops and closed magnetic structures
Cited by in corpus (9)
- Impulsive phase flare energy transport by large-scale Alfven waves and the electron acceleration problem
- Enhanced phase mixing of Alfvén waves propagating in stratified and divergent coronal structures
- A minimal model of parallel electric field generation in a transversely inhomogeneous plasma
- Physics of collisionless phase mixing
- Astrophysics in 2006
- Particle acceleration and their escape into the heliosphere in solar flares with open magnetic field
- Heating of solar chromosphere by electromagnetic wave absorption in a plasma slab model
- Enhanced Phase Mixing of Torsional Alfvén Waves in Stratified and Divergent Solar Coronal Structures, Paper I: Linear Solutions
- On parallel electric field generation in transversely inhomogeneous plasmas