Tipo de publicación: Con árbitro

  • Publicación
    Resolving the Tachocline Using Inversion of Rotational Splitting Derived from Fitting Very Long and Long Time Series
    We use rotation splittings derived from very long and long time series, namely 25.2, 12.6, and 6.3 yr long, computed by S. G. Korzennik independent methodology...
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    Resolving the unresolved: Discovery and dynamical masses of the brown dwarf binary DE1756−45
    We present a method of resolving the geometric structure in unresolved CCD images of the two-component stellar objects with relative separations below the full...
  • Publicación
    Resonance scattering polarization in the magnetosphere of Mercury
    The conditions of the exosphere of Mercury constitute a prime example of a magnetosphere subject to space weather. We aim at improving the diagnostic of the...
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    Resonant Absorption in Complicated Plasma Configurations: Applications to Multistranded Coronal Loop Oscillations
    We study the excitation and damping of transverse oscillations in a multistranded model of a straight line-tied coronal loop. The transverse geometry of our...
  • Publicación
    Resonant absorption: Transformation of compressive motions into vortical motions
    This paper investigates the changes in spatial properties when magnetohydrodynamic (MHD) waves undergo resonant damping in the Alfvén continuum. The analysis is...
  • Publicación
    Resonant Structure in the Disks of Spiral Galaxies, Using Phase Reversals in Streaming Motions from Two-dimensional Hα Fabry-Perot Spectroscopy
    In this Letter, we introduce a technique for finding resonance radii in a disk galaxy. We use a two-dimensional velocity field in Hα emission obtained with...
  • Publicación
    Resonantly damped fast MHD kink modes in longitudinally stratified tubes with thick non-uniform transitional layers
    Resonantly damped fast kink quasi-modes are computed in fully resistive magnetohydrodynamics (MHD) for two-dimensional equilibrium models. The equilibrium model...
  • Publicación
    Resonantly Damped Surface and Body MHD Waves in a Solar Coronal Slab with Oblique Propagation
    The theory of magnetohydrodynamic (MHD) waves in solar coronal slabs in a zero- β configuration and for parallel propagation of waves does not allow the...
  • Publicación
    Response functions for the inversion of data from unresolved solar magnetic elements.
    By adopting the thin flux tube model as representative of spatially unresolved magnetic elements in the photosphere of the Sun, we identify an adequate set of...