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Relational-geometric justification of magnetic fields in astrophysical objects the framework of the relational-geometric concept is given.

On Explanations of Magnetic Fields of Astrophysical Objects in the Geometric and Relational ApproachesThe geometric and relational approach to the unified description of gravity and electromagnetism

The Sutherland–Einstein Hypothesis on the Origin of Magnetic Fields of Astropysical Objects of the magnetic fields of the Earth and other astrophysical objects, put forward in the early twentieth century

Supermassive hot Jupiters provide more favourable conditions for the generation of radio emission via the cyclotron maser instability - a case study based on Tau Bootis b Tau Bootis b-like planets (a supermassive hot Jupiter with 5.84 Jupiter masses and 1.06 Jupiter radii

Making the software package for analysis the statistical models of space observations
space observations. In particular, the potential fields of the planets, the topography and gravitational

Crystal-field approach to rare-earth higher borides: Dimerization, thermal, and magnetic properties of R B50 (R=Tb,Dy,Ho,Er,Tm) CRYSTAL-FIELD APPROACH to RARE-EARTH HIGHER . B. Z. MALKIN, S. L. BUD'KO, and V. V. NOVIKOV and the indirect exchange fields generated by magnetic interactions along the ladder legs. The crystal-field

Вселенная как конструкт: эпистемологические верования и когерентность обоснования в современной космологии with empirical reality, but in the coherence of epistemic justification which relates to belief-like commitments

Effect of stellar wind induced magnetic fields on planetary obstacles of non-magnetized hot Jupiters of the induced magnetic field, the planetary obstacle can move up to ≈0.5–1 planetary radii closer to the planet

Magnetic fields of astrophysical objects in three physical paradigms the Earth's magnetic field and other astrophysical objects. The dynamo mechanism, the Sutherland

Transit Lyman-α signatures of terrestrial planets in the habitable zones of M dwarfs-sized planet orbiting in the habitable zone (HZ) of the M dwarf GJ 436. We estimated the transit depth

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