Intermittency of electron density in interstellar kinetic Alfvén wave turbulence

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

2

Magnetohydrodynamics And Plasmas, Pulsars, Magnetohydrodynamic Waves

Scientific paper

The statistics of electron density fluctuations in kinetic Alfvén wave (KAW) turbulence is investigated in connection with the inferred Lévy statistics of pulsar signal broadening. Using analytic theory and computation, decaying KAW turbulence is shown to form coherent, intermittent current filaments in regions where local current intensity exceeds the rms value by a critical factor of a few. Nonlinear mixing is suppressed because the filament magnetic field has sufficient shear to refract away turbulent waves. While the magnetic field and density associated with the filament are as coherent as the current, they are not localized and isolated. Ampere's law dictates that the magnetic field decays as r-1 outside the current, and KAW equipartition dictates that density has the same envelope. This structure gives the density gradient a Lévy distribution, consistent with pulsar scintillation.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Intermittency of electron density in interstellar kinetic Alfvén wave turbulence 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 Intermittency of electron density in interstellar kinetic Alfvén wave turbulence, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Intermittency of electron density in interstellar kinetic Alfvén wave turbulence will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1077087

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.