Showing 1–20 of 56 results
/ Date/ Name
Apr 15, 2022Variation in solar differential rotation and activity in the period 1964-2016 determined by the Kanzelhöhe data setDec 14, 2009The size distribution of magnetic bright points derived from Hinode/SOT observationsFeb 29, 2024Calculated brightness temperatures of solar structures compared with ALMA and Metsähovi measurementsFeb 20, 2019Mapping the magnetic field of flare coronal loopsJan 14, 2020The BRITE-SONG of Aldebaran -- Stellar Music in three voicesJul 11, 2002Determination of fractal dimensions of solar radio burstsJun 28, 2012The DWARF project: Eclipsing binaries - precise clocks to discover exoplanetsFeb 19, 2015SSALMON - The Solar Simulations for the Atacama Large Millimeter Observatory NetworkMay 8, 2012Time series of high resolution photospheric spectra in a quiet region of the Sun. II. Analysis of the variation of physical quantities of granular structuresApr 26, 2023Exploring magnetic field properties at the boundary of solar pores: A comparative study based on SDO-HMI observationsDec 19, 2012XUV exposed, non-hydrostatic hydrogen-rich upper atmospheres of terrestrial planets II: Hydrogen coronae and ion escapeOct 4, 2021Prominence instability and CMEs triggered by massive coronal rain in the solar atmosphereAug 1, 2016Indications of stellar prominence oscillations on fast rotating stars: the cases of HK Aqr and PZ TelAug 11, 2021Revealing the structure of the lensed quasar Q 0957+561: I. Accretion disk sizeJul 13, 2021Microlensing of the broad emission lines in 27 gravitationally lensed quasars. Broad line region structure and kinematicsAug 12, 2016Size of the accretion disk in the gravitationally lensed quasar SDSS J1004+4112 from the statistics of microlensing magnificationsOct 30, 2017$\texttt{PyTranSpot}$ - A tool for multiband light curve modeling of planetary transits and stellar spotsJul 6, 2023Revealing the structure of the lensed quasar Q 0957+561 III. Constraints on the size of the broad-line regionMar 21, 2022A prediction for the 25th solar cycle maximum amplitudeMar 14, 2013Observations and modeling of the emerging EUV loops in the quiet Sun as seen with the Solar Dynamics Observatory