Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
Scientific paper
2011-08-30
Astronomy and Astrophysics
Astrophysics
Galaxy Astrophysics
To appear in "Physics of the Heliosphere: a 10-year Retrospective", Jacob Heerikhuisen, Gang Li, and Gary P. Zank, Eds
Scientific paper
Recent observations indicate that kinetic and magnetic energies are not in equipartition in the solar wind turbulence. Rather, magnetic fluctuations are more energetic and have somewhat steeper energy spectrum compared to the velocity fluctuations. This leads to the presence of the so-called residual energy E_r=E_v-E_b in the inertial interval of turbulence. This puzzling effect is addressed in the present paper in the framework of weak turbulence theory. Using a simple model of weakly colliding Alfv\'en waves, we demonstrate that the kinetic-magnetic equipartition indeed gets broken as a result of nonlinear interaction of Alfv\'en waves. We establish that magnetic energy is indeed generated more efficiently as a result of these interactions, which proposes an explanation for the solar wind observations.
Boldyrev Stanislav
Perez Jean Carlos
Zhdankin Vladimir
No associations
LandOfFree
Residual energy in magnetohydrodynamic turbulence and in the solar wind does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Residual energy in magnetohydrodynamic turbulence and in the solar wind, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Residual energy in magnetohydrodynamic turbulence and in the solar wind will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-624624