Spontaneous thermal waves in a magnetized plasma.
نویسندگان
چکیده
Coherent temperature oscillations corresponding to thermal (diffusion) waves are observed to be spontaneously excited in a narrow temperature filament embedded in a large, but colder, magnetized plasma. The parallel and transverse propagation properties of the waves satisfy the predictions of the classical transport theory based on Coulomb collisions. The frequency of the oscillations meets the conditions for a quarter-wave thermal resonator. This is the plasma version of thermal resonators used in the study of other states of matter.
منابع مشابه
Investigation of Dust-Ion Acoustic Waves in a Magnetized Collisional Dusty Plasma with Kappa Distribution Function for Electrons
The propagation of arbitrary amplitude dust ion acoustic waves (DIAWs) in a magnetized collisional dusty plasma including hot electrons, with kappa velocity distribution for electrons, warm ions and dust particles has been studied. In the presence of immobile massive dust particulates, DIAWs have been investigated through the Sagdeev pseudo-potential method. It is demonstrated that the amplitud...
متن کاملSome properties of magnetized pair plasmas
Three aspects of the physics of pair plasmas are discussed. The main emphasis is on the properties of waves in cold, magnetized pair plasmas, where it is shown that the inclusion of an admixture of positrons introduces an additional ‘cyclotron mode’ into the magneto-ionic theory. Thermal effects on these waves are described. The quadratic nonlinear response and the fluid description of a pair p...
متن کاملLocal thermodynamics of a magnetized, anisotropic plasma
Related Articles Transport properties of multicomponent thermal plasmas: Grad method versus Chapman-Enskog method Phys. Plasmas 20, 023504 (2013) Equation of state of dense plasmas by ab initio simulations: Bridging the gap between quantum molecular dynamics and orbital-free molecular dynamics at high temperature Phys. Plasmas 19, 122712 (2012) Reactive and internal contributions to the thermal...
متن کاملMhd Tidal Waves on a Spinning Magnetic Compact Star
In an X-ray binary system, the companion star feeds the compact neutron star with plasma materials via accretions. The spinning neutron star is likely covered with a thin “magnetized ocean” and may support magnetohydrodynamic (MHD) tidal waves. While modulating the thermal properties of the ocean, MHD tidal waves periodically shake the base of the stellar magnetosphere that traps energetic part...
متن کاملAtmospheres of Magnetized Neutron Stars: Vacuum Polarization and Partially Ionized Models
We construct hydrogen atmosphere models for magnetized neutron stars in radiative equilibrium with surface fields B = 10−5×10 G and effective temperatures Teff ∼ a few×10 5 −10 K by solving the full radiative transfer equations for both polarization modes in the magnetized hydrogen plasma. The atmospheres directly determine the characteristics of thermal emission from isolated neutron stars. We...
متن کاملذخیره 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 ناماگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید
ورودعنوان ژورنال:
- Physical review letters
دوره 101 3 شماره
صفحات -
تاریخ انتشار 2008