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Ultraviolet spectropolarimetric diagnostics of hot star magnetospheres
Several space missions and instruments for UV spectropolarimetry are in preparation, such as the proposed NASA MIDEX Polstar project, the proposed...
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Chiral anomalous processes in magnetospheres of pulsars and black holes
We propose that chirally asymmetric plasma can be produced in the gap regions of the magnetospheres of pulsars and black holes. We show that, in the...
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Resonant Interaction of Energetic Electrons with Radio Emission in the Magnetospheres of Exoplanets
We analyze the resonant interaction of energetic electrons with radio emission in the magnetospheres of exoplanets using the planet Tau Bootis b as...
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X-ray emission spectrum for axion–photon conversion in magnetospheres of strongly magnetized neutron stars
Detecting axionic dark matter (DM) could be possible in an X-ray spectrum from strongly magnetized neutron stars (NSs). We examine the possibility of...
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Current Sheets with Multicomponent Plasma in Magnetospheres of Planets of the Solar System
AbstractA self-consistent hybrid model of a thin current sheet (TCS) with a thickness of the order of several ion gyroradii is proposed that takes...
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Internal and External Jovian Magnetic Fields: Community Code to Serve the Magnetospheres of the Outer Planets Community
We report on a new international community coding project to provide shared scientific computer code that performs common calculations to aid in...
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Ultraviolet spectropolarimetry with Polstar: using Polstar to test magnetospheric mass-loss quenching
Polstar is a proposed NASA MIDEX space telescope that will provide high-resolution, simultaneous full-Stokes spectropolarimetry in the far...
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Radiative Effects in the Modelling of Accretion onto Stellar Magnetospheres
Accretion onto neutron stars and black holes is the main energy supply in galactic X-ray sources. The angular momentum captured by the X-ray star... -
Magnetic Reconnection at Planetary Bodies and Astrospheres
Magnetic reconnection is a fundamental mechanism for the transport of mass and energy in planetary magnetospheres and astrospheres. While the process...
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Magnetic reconnection in the magnetodisk of centrifugally dominated giant planets
Magnetic reconnection is crucial in understanding magnetospheric dynamics and aurorae processes at planets. In planetary magnetospheres, magnetic...
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On Possible Types of Magnetospheres of Hot Jupiters
As a rule, the orbits of “hot Jupiter” exoplanets are located close to the Alfven point of the stellar wind of the host star. Many hot Jupiters could...
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Phase Velocity Anisotropy of MHD Waves in Plasma with Thermal Imbalance
AbstractThe anisotropic behavior of the phase velocity of magnetogasdynamic (MHD) waves in plasma with thermal imbalance is studied. Examples of such...
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The Metron Project—I. The Metron Project Science Program
AbstractIn this paper, the first in a series of four articles, the scientific goals of the Metron project are highlighted, and the characteristics of...
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A unified framework for global auroral morphologies of different planets
Planetary magnetic fields control energetic particles in their space environments and guide particles to polar atmospheres, where they produce...
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Synchrotron emission from the depths of pulsar magnetospheres
In this paper we study the generation of high energy emission from normal pulsars. For this purpose we consider the particles accelerated in the...
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UV exploration of the solar system
The study of the Solar System is fundamental to answer key questions from space agencies, as outlined in their strategic plans, about the content,...
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Formation of Hydrogen Emission Lines in the Magnetospheres of Young Stars
The formation of hydrogen emission lines in the magnetospheres of young stars is considered. The magnetosphere is assumed to be formed by a dipolar...
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Ultraviolet spectropolarimetry: investigating stellar magnetic field diagnostics
Magnetic fields are important for stellar photospheres and magnetospheres, influencing photospheric physics and sculpting stellar winds. Observations...
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Models of Magnetospheric Accretion onto Young Stars in the Absence of Ionization Equilibrium
AbstractThe formation of hydrogen emission lines in the magnetospheres of young stars is considered. The magnetosphere is assumed to be formed by a...
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The characteristics of ion-acoustic solitary waves in relativistic rotating astrophysical plasmas
We investigate the character of ion-acoustic (IA) solitary waves in plasma structures that experience rotational motions. The plasma properties...