Publication type: Non-refereed

  • Publication
    Flux emergence and interaction with a coronal field: 3D MHD simulations
    The dynamic process of magnetic flux emergence from the solar interior to the outer atmosphere may well be related with eruptive phenomena and intense events of...
  • Publication
    Flux Emergence at the Photosphere
    To model the emergence of magnetic fields at the photosphere, we carried out 3D magneto-hydrodynamics (MHD) simulations using the MURaM code. Our simulations...
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    Flux Emergence from the Solar Interior Into a Uniformly Magnetized Corona
    Not Available
  • Publication
    Flux Emergence from the Solar Interior to the Atmosphere: the Passage through the Photosphere
    The atmosphere of the Sun is being stirred and reshaped continuously through the emergence of magnetized plasma from the convection zone. Magnetic elements...
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    Flux Emergence In The Solar Photosphere - Diagnostics Based On 3-D Rradiation-MHD Simulations
    We investigate flux tube emergence in the solar photosphere using a diagnostic procedure based on analyzing Stokes signals from different spectral lines...
  • Publication
    Follow up observationes of extremely metal-poor stars identified from SDSS and LAMOST
    The most metal-poor stars in the Milky Way witnessed the early phases of formation of the Galaxy, and have chemical compositions close to the pristine mixture...
  • Publication
    Follow-up observations of GLIMPSE selected Post-AGB candidates
    We propose to use the last Spitzer observing cycle to increase the sample of hidden post-AGB stars with mid-infrared spectroscopy. We selected predominantly...
  • Publication
    Follow-Up of Comet-Asteroid Transition Object 107P Wilson-Harrington During Its 2009 Return to Perihelium
    We have been monitoring 107P comet-asteroid transition object during its 2009 return to perihelium. We have been unable of identifying any trace of cometary...
  • Publication
    Footprints of the early Universe in the SFHs of dwarf galaxies
    We present the star formation histories (SFHs) as a function of galactocentric radius of four isolated dwarf galaxies, Cetus, Tucana, LGS-3, and Phoenix. Our...