Вісник астрономічної школи
- » Peculiarities of the Zeeman splitting in lines with small Lande factors in a sunspot...
- » The X-ray and radio structure of extragalactic jets
- » Searching of non-thermal X-ray emission from nearest galaxy clusters with large-scale...
- » Estimating the porosity of the upper soil layer for some details of the Moon
- » Geoinformation analysis of remote sensing data to forecast the possibility of forest fires
- » The research of optically transparent ferrites application possibility for portable...
- » On the influence of non-gravitational forces on cometary dynamics
- » Correlation of ultrahigh energy cosmic rays with nearest sources
- » Stochastic acceleration of cosmic rays in region of relativistic jet deceleration in...
- » X-ray emission of galaxies with emission lines
- » Features of morphology and geology of surface of Jupiter satellite Europe
- » Asymmetry of reflective properties of the hemispheres of Jupiter satellite Europa
- » Meteorites as a natural detectors of very heavy galactic cosmic ray nuclei: some...
- » The main belt 3628 Boznemcova asteroid as possible source of the LL6-chondrites
- » Photopolarimetric method of polarization radiation parameters determination
- » The modeled estimate of angular size for young meteor showers radiant area
- » Modeling of the origin of wide meteoroid shower produced by multi-stage parent comet...
- » Investigation of outburst activity of comets as a base for revealing interplanetary...
- » Chemical and mineral composition of particles of bright bolid EN171101 “Turyi Remety”...
- » About thermodynamic model of the Earth
- » Behavior of Na atoms in the lunar exosphere during activity of meteor showers
- » Pallasite meteorites: cosmic ray irradiation and shock-thermal history by the data of...
- » Catalog and Grotrian diagrams for the lines of multiplet iron FeI and FeII, observed in...
- » Analysis of the accuracy requirement for aerospace pictures and digital maps and...
- » The optical spectra of comets