plasma structure造句

• Their control is imperfect, but they learn to control it enough to build an elaborate plasma structure inside their encampment.
• The mission will investigate its plasma and magnetic structure, including transient plasma structures, magnetic field structure, magnetic activity and correlation with solar wind drivers.
• This model works well for the description of a number of plasma structures observed in the solar corona : e . g . coronal loops, prominence fibrils, plumes, various filaments.
• The theoretical foundation of coronal seismology is the dispersion relation of MHD modes of a plasma cylinder : a plasma structure which is nonuniform in the transverse direction and extended along the magnetic field.
• *Sausage modes, which are also oblique fast magnetoacoustic waves guided by the plasma structure; the mode causes expansions and contractions of the plasma structure, but does not displace its axis.
• *Sausage modes, which are also oblique fast magnetoacoustic waves guided by the plasma structure; the mode causes expansions and contractions of the plasma structure, but does not displace its axis.
• Note that, unlike most plasma structures, the Lorentz force and the Magnus force, \ rho \ vec { \ nabla } \ times \ vec { v }, play equivalent roles . \ rho is the mass density.
• The plasma turbulence phenomena that are studied include different types on nonlinear wave interactions, in which different waves in the plasma couple and interact with the transmitted radio wave, formation and self organization of filamentary plasma structures, as well as electron acceleration.
• Each satellite carries a scientific payload of 11 instruments designed to study the small-scale plasma structures in space and time in the key plasma regions : solar wind, bow shock, magnetopause, polar cusps, magnetotail, plasmapause boundary layer and over the polar caps and the auroral zones.
• "' Transition Region and Coronal Explorer "'( "'TRACE "') was a NASA heliophysics and solar observatory designed to investigate the connections between fine-scale magnetic fields and the associated plasma structures on the Sun by providing high resolution images and observation of the solar photosphere, the transition region, and the corona.