Publication type: Refereed

  • Publication
    Method for determining dust particle density above the ecliptic plane
    A method for determining the variation in the density of dust particles is described. Here, the altitude above the symmetry plane of interplanetary dust is...
  • Publication
    Method for the determination of density and phase functions of interplanetary dust
    A method for the determination of the intensity of the solar light scattered by a unit volume of interplanetary space and thus the density and phase functions...
  • Publication
    Methodology for Predicting the Probability Distribution of the Amplitude of Solar Cycle 25
    A number of precursor-type methods for solar-cycle prediction are based on the use of regression models and confidence-level estimates. A drawback of these...
  • Publication
    Mg and TiO spectral features at the near-IR: spectrophotometric index definitions and empirical calibrations
    Using the near-infrared spectral stellar library of Cenarro et al., the behaviour of the MgI line at 8807 Å and nearby TiO bands is analyzed in terms of the...
  • Publication
    MG II observed in the local interstellar medium - The local cloud
    Observations of interstellar absorptions superposed on the chromospheric Mg II emissions of nearby cool stars have been used to explore the structure of the...
  • Publication
    MHD seismology of coronal loops using the period and damping of quasi-mode kink oscillations
    Aims:We combine the magnetohydrodynamic (MHD) theory of resonantly damped quasi-mode kink oscillations with observational estimates of the period and damping of...
  • Publication
    MHDSTS: a new explicit numerical scheme for simulations of partially ionised solar plasma
    The interaction of plasma with magnetic field in the partially ionised solar atmosphere is frequently modelled via a single-fluid approximation, which is valid...
  • Publication
    MHS-Equilibrium of Twisted Magnetic Tubes
    Not Available
  • Publication
    Micro-structured magnetic atmospheres
    Asymmetrical Stokes profiles are produced if the photospheric magnetic and velocity fields are structured on scales smaller than the mean-free-path of the...