On the Backscatter Instability of Solar Wind Alfvn Waves

نویسندگان

  • RONALD H. COHEN
  • ROBERT L. DEWAR
چکیده

A coherent Alfv6n wave propagating along the equilibrium magnetic field is unstable against decay into an Alfv6n wave traveling in the opposite direction and a sound wave [Sagdeer and Galeev, 1969]. The stability of incoherent Alfv6n waves against his mode decay is considered, assuming that the sound waves are damped. The criterion for stabilizing waves with power spectral density In o• k -N is N > 1. The results indicate that solar wind Alfv6n waves are stable in the wavelength range considered in Mariner 5 observations, although a mild instability is predicted for longer wavelengths.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Observations of polar patches generated by solar wind Alfve n wave coupling to the dayside magnetosphere

A long series of polar patches was observed by ionosondes and an all-sky imager during a disturbed period (Kp ˆ 7and IMF Bz < 0). The ionosondes measured electron densities of up to 9 ́ 10 m in the patch center, an increase above the density minimum between patches by a factor of 4.5. Bands of F-region irregularities generated at the equatorward edge of the patches were tracked by HF radars. Th...

متن کامل

MHD waves and instabilities in flowing solar flux-tube plasmas in the framework of Hall magnetohydrodynamics

It is well established now that the solar atmosphere, from photosphere to the corona and the solar wind is a highly structured medium. Satellite observations have confirmed the presence of steady flows. Here, we investigate the parallel propagation of magnetohydrodynamic (MHD) surface waves travelling along an ideal incompressible flowing plasma slab surrounded by flowing plasma environment in ...

متن کامل

Ionospheric cusp flows pulsed by solar wind Alfvén waves

Pulsed ionospheric flows (PIFs) in the cusp footprint have been observed by the SuperDARN radars with periods between a few minutes and several tens of minutes. PIFs are believed to be a consequence of the interplanetary magnetic field (IMF) reconnection with the magnetospheric magnetic field on the dayside magnetopause, ionospheric signatures of flux transfer events (FTEs). The quasiperiodic P...

متن کامل

Modified temperature-anisotropy instability thresholds in the solar wind.

The proton and electron temperature anisotropies in the solar wind are constrained by the instability thresholds for temperature-anisotropy-driven kinetic plasma instabilities. The modifications to the marginal instability conditions from accounting for the influence of damping connected with the collisional effects in the solar wind plasma are calculated for right- and left-handed polarized pa...

متن کامل

Observations of radar backscatter at Ku and C bands in the presence of large waves during the Surface Wave Dynamics Experiment

Abshact — Ocean radar backscatter in the presence of large waves is investigated using data acquired with the Jet Propulsion Laboratory NUSCAT radar at K. band for horizontal and vertical polarizations and the University of Massachusetts C-SCAT radar at C band for vertical polarization during the Surface Wave Dynamics Experiment. Backscatter 2 data of ocean surfaces was obtained in the presence...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 1974