


Vol 63, No 3 (2025)
Articles
Generation and dynamics of the Hall magnetic field during sub-Alfven plasma expansion in the kinetic regime
Abstract
The paper presents a complex study of the Hall effect during the expansion of a spherical plasma cloud into a medium with a uniform external magnetic field. The results were obtained in a laboratory experiment on the KI-1 plasma facility and three-dimensional numerical modeling using the “particle-in-cell” method. The data obtained are in good qualitative and quantitative agreement and demonstrate that when the plasma cloud expands in a regime where the Larmor radius of ions RL is comparable to the scale of the diamagnetic cavity Rb, a large-scale antisymmetric magnetic fields structure is formed, caused by Hall effects. In this case, both internal and external Hall magnetic structures are observed. The work demonstrates the coherence between Hall effects and the diamagnetic cavity collapse, which occurs as the transfer of a magnetic field by Hall electrons currents at an anomalously high speed.



Radiation-protective properties of polymer composite material in the ISS cabin according to thermoluminescent and solid-state track detectors
Abstract



The Beginning of the 25th Cycle of Solar Activity in Variations of Oxygen Ion Density in the Orbit of the Meteor Spacecraft
Abstract
Based on the archive of measurement data in the upper atmosphere by radio frequency mass spectrometers on the Meteor spacecraft at the end of the 24th and at the beginning of the 25th cycle of solar activity, estimates of the parameters of the statistical model of the concentration of oxygen ion (O+) over the polar caps and the equatorial belt of the Earth are given. The signs of a change in the “11-year” cycle of solar activity according to O+ measurements are given, as well as variations that can be used to monitor the gas composition of the upper atmosphere.



The influence of jump conditions in conjugate variables on the multiorbit spacecraft transfers with switching the low thrust off in the earth's shadow
Abstract
Transfers in the central Newtonian field to the geostationary orbit are considered under the assumption that low thrust becomes zero when spacecraft with solar panels enters the Earth’s shadow. Using the maximum principle, the two-point boundary value problem is formed. It includes the conditions for optimal intersection of the shadow boundaries, the so called jump conditions in conjugate variables. Then the influence of jump conditions on the two-point boundary value problem solutions is investigated. Calculations for the flights of spacecraft with initial mass 5550 kg and thrust 0.55 N (initial acceleration 0.1 mm/s2) from the initial orbit with inclination 13° and the height of perigee 9.2 Mm and of apogee 76.8 Mm were done. They showed that if the argument of pericenter is equal to 0° and the longitude of the ascending node Ω0 = 180°, the difference in the propellant cost for two trajectories – with or without taking into account the jump conditions – does not exceed 0.15 % (in comparison with “nominal” trajectories, i.e., transfers without zeroing the thrust), and may be less than 0.01 % for some values of initial time. For other values of Ω0, the difference may be greater than 30 %. It was discovered also that the two-point boundary value problem may have several solutions. They differ from each other by the set of orbits crossing the Earth’s shadow.



VIRTUAL GRAVITY ASSISTS MANEUVERS IN INTERPLANETARY BALLISTIC MISSION DESIGN
Abstract



A simple control scheme for the problem of spacecraft transfer into a target orbit with releasing the separable part of its launch vehicle into the earth's atmosphere
Abstract



Gravispheric Effect for Flights Between the Earth and High Lunar Orbit
Abstract



Endogenous factors influencing the ice conditions of navigation along the northern sea route
Abstract



Tomographic methods for studying the upper atmosphere and near-Earth space: current state and development prospects
Abstract


