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Whistler-mode waves in Mercury’s magnetosphere observed by BepiColombo/Mio
Whistler-mode chorus waves are natural electromagnetic emissions known to play a key role in electron acceleration and loss mechanisms via...
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Flexible filaments buckle into helicoidal shapes in strong compressional flows
The occurrence of coiled or helical morphologies is common in nature, from plant roots to DNA packaging into viral capsids, as well as in...
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Coronal Quasi-periodic Fast-mode Propagating Wave Trains
Quasi-periodic, fast-mode propagating (QFP) wave trains in the corona have been studied intensively over the last decade, thanks to the full-disk,...
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Numerical Study of S0 Lamb Mode Resonator based on c-BN/AlN for 5G Operating Acoustic Devices
AbstractThe present work aims the numerical study of acoustic Lamb wave resonator LWR based on Aluminium Nitride (AlN) deposited on cubic Boron...
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Effects of galactic cosmic rays and finite electrical resistivity on the Jeans instability in magnetized viscoelastic fluid
In this paper, we have investigated the effects of galactic cosmic rays (CRs) and finite electrical resistivity on the linear gravitational...
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X-ray Emissions from the Jovian System
The Jovian system is a treasure trove of X-ray sources: diverse and dynamic atmospheric and auroral emissions, diffuse radiation belt and Io Plasma...
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Transmission of foreshock waves through Earth’s bow shock
The Earth’s magnetosphere and its bow shock, which is formed by the interaction of the supersonic solar wind with the terrestrial magnetic field,...
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Longitudinal Plasma Motions Generated by Shear Alfvén Waves in Plasma with Thermal Misbalance
Compressional plasma perturbations may cause thermal misbalance between plasma-heating and -cooling processes. This misbalance significantly affects...
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Transport from electron-scale turbulence in toroidal magnetic confinement devices
Plasma transport driven by turbulence ultimately determines the energy confinement performance of controlled fusion devices regardless of their...
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Collective Effects in Dusty Plasmas
Dusty plasmas, i.e. plasmas containing particles of nanometer to micrometer size, allow the observation of kinetic and collective effects on a...
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Single-component superconductivity in UTe2 at ambient pressure
The microscopic mechanism of Cooper pairing in a superconductor leaves its fingerprint on the symmetry of the order parameter. UTe 2 has previously...
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Kinetic Alfvén waves in the magnetotail during substorms
Kinetic Alfvén waves (KAWs) are low-frequency dispersive Alfvén waves with a small perpendicular wavelength and long parallel wavelength to the...
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X-Ray Emissions from the Jovian System
The Jovian system is a treasure trove of X-ray sources: diverse and dynamic atmospheric and auroral emissions, diffuse radiation belt and Io Plasma...
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Study of the Shear Alfvén Waves via Parametric Degeneration of Lower Hybrid Pump Wave in Dusty Plasma
The phenomena of excitation of shear Alfvén waves via parametric degeneration of lower hybrid wave are explored in complex plasma. In this...
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Merging mechanical bound states in the continuum in high-aspect-ratio phononic crystal gratings
Mechanical bound states in the continuum (BICs) present an alternative avenue for develo** high-frequency, high- Q mechanical resonators, distinct...
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Jeans instability in strongly coupled clumpy molecular cloud with dissipative effects
Gravitational instability in a strongly coupled self-gravitating viscoelastic clumpy molecular cloud in the presence of dissipative effects is...
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Elastic orbital angular momentum transfer from an elastic pipe to a fluid
Research into the orbital angular momentum carried by helical wave-fronts has been dominated by the fields of electromagnetism and acoustics, owing...
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Investigation of mechanical, optical, phonon frequencies, and sound velocity of nano-structured Gallium Phosphide (GaP) material under the effect of pressure
We present an investigation of the electronic, optical, and mechanical characteristics of the nano-structured Gallium Phosphide (GaP) semiconductor....
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Intermittent plasma turbulence in the Martian plasma environment
Due to the absence of a global intrinsic magnetic field, Mars presents an induced magnetosphere, which is formed by the interaction between the solar...
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Physics of “Hot” Plasmas
The physics of hot plasmas, i.e. nearly collisionless plasmas with finite pressure as they occur in astrophysical or fusion applications, is...