Search Publications

Energetic particle distributions in space physics represented by the Pearson differential equation for the kappa distribution
DOI: 10.1007/s10509-021-03956-0 Bibcode: 2021Ap&SS.366...50S

Shizgal, Bernie D.

The kappa distribution has been used for decades as a numerical fitting function to represent the energetic particle distributions measured with satellite instruments. The distributions are generally either a three dimensional distribution in the particle velocity or the one dimensional distribution in a velocity component in a particular directio…

2021 Astrophysics and Space Science
Cluster 2
Dipolar and Kelvin-Stuart's cat's eyes vortices in magnetoplasmas with non-Maxwellian electron distribution
DOI: 10.1007/s10509-020-03759-9 Bibcode: 2020Ap&SS.365...52N

Masood, W.; Naeem, Ismat; Mirza, Arshad M.

Linear and nonlinear propagation characteristics of drift ion acoustic waves are analyzed in an inhomogeneous plasma comprising of warm ions having shear flow parallel to the magnetic field and electrons that are followed by a distribution which is dictated by spectral indices, r

2020 Astrophysics and Space Science
Cluster 6
Spectrum of imbalanced Alfvénic turbulence at ion-kinetic scales in the solar wind
DOI: 10.1007/s10509-020-03865-8 Bibcode: 2020Ap&SS.365..149G

Voitenko, Y. M.; Gogoberidze, G.

Using a semi-phenomenological model of the imbalanced Alfvénic turbulence, we study the turbulence transition from magnetohydrodynamic to sub-ion kinetic scales in the conditions typical for the fast solar wind. We show that the transition takes place in a wide wave number interval where the energy spectrum does not follow any power law. For large…

2020 Astrophysics and Space Science
Cluster 1
Implication of kinetic Alfvén waves to magnetic field turbulence spectra: Earth's magnetosheath
DOI: 10.1007/s10509-019-3592-2 Bibcode: 2019Ap&SS.364..101D

Khodachenko, M. L.; Kumar, S.; Echim, M. +5 more

In the present paper, we investigate the power-law behaviour of the magnetic field spectra in the Earth's magnetosheath region using Cluster spacecraft data under solar minimum condition. The power spectral density of the magnetic field data and spectral slopes at various frequencies are analysed. Propagation angle,

2019 Astrophysics and Space Science
Cluster 9
Nonlinear model to study filamentation instability of circularly polarized dispersive Alfvén waves in solar wind plasmas
DOI: 10.1007/s10509-018-3382-2 Bibcode: 2018Ap&SS.363..164S

Sharma, R. P.; Sharma, Swati; Mishra, M. K.

This paper examines the small-scale solar wind turbulence driven in view of the Alfvén waves subjected to ponderomotive nonlinearity. Filamentation instability is known to take place for the case of dispersive Alfvén wave (DAW) propagating parallel to the ambient magnetic field. The ponderomotive force associated with DAW is responsible for wave l…

2018 Astrophysics and Space Science
Cluster 0
A two-fluid modeling of kinetic Alfvén wave turbulence
DOI: 10.1007/s10509-018-3427-6 Bibcode: 2018Ap&SS.363..204K

Moon, Y. -J.; Sharma, R. P.; Dwivedi, Navin Kumar +1 more

We present an analytical model to explore the magnetic field turbulent spectrum by coupled high-frequency kinetic Alfvén wave (KAW) and slow mode of Alfvén wave (AW). The spectrum is computed as a realization of energy cascades from larger to smaller scales for a specific case of solar wind plasma at 1 AU. A two-fluid technique is implemented for …

2018 Astrophysics and Space Science
Cluster 0
Electron acceleration in the near-Earth magnetotail: test particle calculations in electromagnetic fields from two-dimensional hybrid simulations
DOI: 10.1007/s10509-017-3093-0 Bibcode: 2017Ap&SS.362..119G

Wu, Mingyu; Du, Aimin; Guo, Zhifang

Electron acceleration in the near-Earth magnetotail during the substorm period is still an unresolved question. In this paper, by tracing electron trajectories in the dynamically evolving electromagnetic fields obtained from a two-dimensional (2D) global hybrid simulation, we investigate electron acceleration in the near-Earth magnetotail during d…

2017 Astrophysics and Space Science
Cluster 4
Double-cusp simulation during northward IMF using 3D PIC global code
DOI: 10.1007/s10509-017-3098-8 Bibcode: 2017Ap&SS.362..125E

Esmaeili, Amin; Kalaee, Mohammad Javad

The cusp has important effects on the transportation of particles and their energy from the solar wind to the magnetosphere, and ionosphere, and high-altitude atmosphere. The cusp can be considered to be a part of the magnetospheric boundary layer with weaker magnetic fields. It has been studied since 1971 by different satellite observations. Desp…

2017 Astrophysics and Space Science
Cluster 3
Nonlinear evolution of oblique whistler waves in radiation belts
DOI: 10.1007/s10509-016-3003-x Bibcode: 2017Ap&SS.362...32S

Sharma, R. P.; Sharma, Swati; Nandal, P. +1 more

Magnetic power spectrum and formation of coherent structures have been investigated in the present work applicable to Van Allen radiation belt. The nonlinear interaction of high frequency oblique whistler wave and low frequency magnetosonic wave has been investigated. Simulation was performed of the coupled equation of these two waves. The nonline…

2017 Astrophysics and Space Science
Cluster 0
Energy budget during an isolated substorm using measurements of multi satellites and geomagnetic indices
DOI: 10.1007/s10509-017-3072-5 Bibcode: 2017Ap&SS.362..101M

Dunlop, M. W.; Ma, Yuduan; Yang, Jian +1 more

Measurements of multi satellites and geomagnetic indices are used to investigate the energy budget during an isolated substorm. The calculation of the energy transfer from the solar wind to the magnetosphere (parameter ɛ), the energy increase of the ring current (

2017 Astrophysics and Space Science
Cluster 0