4.4 Article

Scattering by the broadband electrostatic turbulence in the space plasma

Journal

PHYSICS OF PLASMAS
Volume 25, Issue 7, Pages -

Publisher

AIP Publishing
DOI: 10.1063/1.5039687

Keywords

-

Funding

  1. JHU/APL [922613]
  2. NASA [80NSSC18K0155]
  3. Russian Science Foundation [15-32-21078]
  4. CNES
  5. Russian Science Foundation [17-12-00084] Funding Source: Russian Science Foundation

Ask authors/readers for more resources

The broadband electrostatic turbulence that is produced by electrostatic solitary waves and associated with strong parallel currents is widely observed in the space plasma. In this paper, we develop a basis for quantifying particle scattering by the broadband electrostatic turbulence. We show that the pitch angle and energy scattering rates can be computed using the classical quasi-linear theory in spite of the fact that the turbulence is produced by nonlinear solitary waves. The developed formalism is applied to estimate the particle scattering rates by the broadband turbulence observed in the Earth's inner magnetosphere. We show that the scattering rates of ions are negligible, while the pitch-angle scattering of electrons is sufficiently fast to drive valuable electron losses to the atmosphere. The anomalous dissipation of a parallel current and anomalous electron heating by the broadband turbulence are evaluated. Published by AIP Publishing.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.4
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

Article Astronomy & Astrophysics

Kinetic-scale Current Sheets in the Solar Wind at 1 au: Scale-dependent Properties and Critical Current Density

I. Y. Vasko, K. Alimov, T. Phan, S. D. Bale, F. S. Mozer, A. Artemyev

Summary: In this study, we analyzed proton kinetic-scale current sheets in the solar wind and found that smaller-scale current sheets have higher current density, but do not exceed the drift between ions and electrons of local Alven speed. This observation holds in normalized units.

ASTROPHYSICAL JOURNAL LETTERS (2022)

Article Physics, Fluids & Plasmas

Electron magnetosonic waves and sub-ion magnetic holes in the magnetotail plasma

P. I. Shustov, A. V. Artemyev, A. S. Volokitin, I. Y. Vasko, X. -J. Zhang, A. A. Petrukovich

Summary: Recent observations in Earth's magnetotail and magnetosheath have shown the presence of nonlinear sub-ion scale magnetic holes, which are localized dips in magnetic field intensity. These structures, resembling magnetosonic solitary waves, are balanced by hot electron pressure rather than significant density perturbations. Investigating linear modes of hot plasma with two electron components (hot and cold) reveals an electromagnetic mode with nearly cross field propagation and absence of density perturbations, resembling an electron magnetosonic mode.

PHYSICS OF PLASMAS (2022)

Article Astronomy & Astrophysics

Electron Resonant Interaction With Whistler Waves Around Foreshock Transients and the Bow Shock Behind the Terminator

A. V. Artemyev, X. Shi, T. Z. Liu, X. -J. Zhang, I. Vasko, V. Angelopoulos

Summary: Investigation of electron energization at (and around) the Earth's bow shock is critical to our understanding of space weather and astrophysical phenomena. In this study, using THEMIS and ARTEMIS wave measurements, we quantified the nonlinear effects of resonant interactions between >= 100 eV electrons and intense coherent whistler waves, and found that trapped electrons can gain energy up to several hundreds of eV.

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS (2022)

Article Astronomy & Astrophysics

Langmuir-Slow Extraordinary Mode Magnetic Signature Observations with Parker Solar Probe

A. Larosa, T. Dudok de Wit, V. Krasnoselskikh, S. D. Bale, O. Agapitov, J. Bonnell, C. Froment, K. Goetz, P. Harvey, J. Halekas, M. Kretzschmar, R. MacDowall, David M. Malaspina, M. Moncuquet, J. Niehof, M. Pulupa, C. Revillet

Summary: The study reports on the direct measurement of the magnetic signature of electromagnetic emissions in the solar wind using the Parker Solar Probe/FIELDS instrument. It reveals the presence of magnetic components in the slow extraordinary modes in an inhomogeneous plasma, which is influenced by density inhomogeneities.

ASTROPHYSICAL JOURNAL (2022)

Article Astronomy & Astrophysics

Kinetic-scale Current Sheets in Near-Sun Solar Wind: Properties, Scale-dependent Features and Reconnection Onset

A. B. Lotekar, I. Y. Vasko, T. Phan, S. D. Bale, T. A. Bowen, J. Halekas, A. Artemyev, Yu Khotyaintsev, F. S. Mozer

Summary: This study presents statistical analysis of proton kinetic-scale current sheets observed by the Parker Solar Probe. The analysis reveals the range and typical values for the thickness and current density of these current sheets, as well as their asymmetry and relationship with scale and magnetic shear angles. The findings suggest that these proton kinetic-scale current sheets are produced by turbulence cascade and are not suppressed by the diamagnetic mechanism.

ASTROPHYSICAL JOURNAL (2022)

Article Astronomy & Astrophysics

Core Electron Heating by Triggered Ion Acoustic Waves in the Solar Wind

F. S. Mozer, S. D. Bale, C. A. Cattell, J. Halekas, I. Y. Vasko, J. L. Verniero, P. J. Kellogg

Summary: Research on the orbits of Parker Solar Probe has shown that solar wind core electrons emerge from 15 solar radii with a temperature of 55 +/- 5 eV, regardless of solar wind speed. The core electron temperature then varies with radial distance due to cooling caused by adiabatic expansion. Triggered ion acoustic waves can heat the core electrons up to twice the minimum temperature observed.

ASTROPHYSICAL JOURNAL LETTERS (2022)

Article Geosciences, Multidisciplinary

Ion-Acoustic Waves in a Quasi-Perpendicular Earth's Bow Shock

I. Y. Vasko, F. S. Mozer, S. D. Bale, A. Artemyev

Summary: This study presents an analysis of electrostatic waves observed near the quasi-perpendicular Earth's bow shock by the Magnetospheric Multiscale spacecraft. The analysis reveals that these electrostatic waves have large amplitudes and can propagate almost perpendicular to the local magnetic field. The results suggest that these waves may strongly affect the dynamics of electrons in collisionless shocks.

GEOPHYSICAL RESEARCH LETTERS (2022)

Article Astronomy & Astrophysics

First Results From the SCM Search-Coil Magnetometer on Parker Solar Probe

T. Dudok de Wit, V. V. Krasnoselskikh, O. Agapitov, C. Froment, A. Larosa, S. D. Bale, T. Bowen, K. Goetz, P. Harvey, G. Jannet, M. Kretzschmar, R. J. MacDowall, D. Malaspina, P. Martin, B. Page, M. Pulupa, C. Revillet

Summary: Parker Solar Probe, the first mission to directly probe the innermost heliosphere, has made significant discoveries in the dynamic and structured outer solar corona through measuring fluctuating magnetic fields. These discoveries include the observation of various solar wind wave phenomena and their interaction with energetic electrons.

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS (2022)

Article Astronomy & Astrophysics

Structured type III radio bursts observed in interplanetary space

I. C. Jebaraj, J. Magdalenic, V Krasnoselskikh, V Krupar, S. Poedts

Summary: This study reports the existence of numerous structured type III radio bursts observed during the STEREO era. The aim is to classify and describe the characteristics of these bursts and to understand the physical mechanism behind their generation. Data from STEREO and Wind spacecraft were used, along with spectral analysis of the fine structures. The results indicate similarities in the fine structures of type III bursts at metric-decameter and interplanetary wavelengths, suggesting a common physical process responsible for their generation.

ASTRONOMY & ASTROPHYSICS (2023)

Article Astronomy & Astrophysics

ICARUS: in-situ studies of the solar corona beyond Parker Solar Probe and Solar Orbiter

Vladimir Krasnoselskikh, Bruce T. Tsurutani, Thierry Dudok de Wit, Simon Walker, Michael Balikhin, Marianne Balat-Pichelin, Marco Velli, Stuart D. Bale, Milan Maksimovic, Oleksiy Agapitov, Wolfgang Baumjohann, Matthieu Berthomier, Roberto Bruno, Steven R. Cranmer, Bart de Pontieu, Domingos de Sousa Meneses, Jonathan Eastwood, Robertus Erdelyi, Robert Ergun, Viktor Fedun, Natalia Ganushkina, Antonella Greco, Louise Harra, Pierre Henri, Timothy Horbury, Hugh Hudson, Justin Kasper, Yuri Khotyaintsev, Matthieu Kretzschmar, Sam Krucker, Harald Kucharek, Yves Langevin, Benoit Lavraud, Jean-Pierre Lebreton, Susan Lepri, Michael Liemohn, Philippe Louarn, Eberhard Moebius, Forrest Mozer, Zdenek Nemecek, Olga Panasenco, Alessandro Retino, Jana Safrankova, Jack Scudder, Sergio Servidio, Luca Sorriso-Valvo, Jan Soucek, Adam Szabo, Andris Vaivads, Grigory Vekstein, Zoltan Voeroes, Teimuraz Zaqarashvili, Gaetano Zimbardo, Andrei Fedorov

Summary: The ICARUS mission aims to understand the magnetic field and plasma dynamics in the outer solar atmosphere and their effects on the corona, solar wind, and heliosphere. This research is important for the fields of space plasma physics and astrophysics.

EXPERIMENTAL ASTRONOMY (2022)

Article Astronomy & Astrophysics

Whistler waves generated inside magnetic dips in the young solar wind: Observations of the search-coil magnetometer on board Parker Solar Probe

C. Froment, O. V. Agapitov, V. Krasnoselskikh, S. Karbashewski, T. Dudok de Wit, A. Larosa, L. Colomban, D. Malaspina, M. Kretzschmar, V. K. Jagarlamudi, S. D. Bale, J. W. Bonnell, F. S. Mozer, M. Pulupa

Summary: The study aims to investigate the parameters of whistler waves in the young solar wind using the Parker Solar Probe (PSP). The results show that most of the detected wave packets in the cross-spectra are quasi-parallel to the background magnetic field, but a significant portion of the waves have oblique wave normal angles. It is concluded that magnetic dips provide favorable conditions for the generation of whistler waves.

ASTRONOMY & ASTROPHYSICS (2023)

Article Astronomy & Astrophysics

Energy Repartition and Entropy Generation across the Earth's Bow Shock: MMS Observations

O. V. Agapitov, V. Krasnoselskikh, M. Balikhin, J. W. Bonnell, F. S. Mozer, L. Avanov

Summary: The evolution of plasma entropy and the redistribution of plasma energy at the collisionless plasma shock front were evaluated using high temporal resolution data from four Magnetospheric Multiscale spacecraft. Different populations of ions were observed near the shock front, and their moments were determined separately. It was found that the solar wind core population velocity slows down mainly in the ramp region, and the proton temperature peak in the foot region is an effect of relative motion of different ion populations. The ion entropy showed a significant increase across the shock, while the entropy of electrons did not show a significant change. Rating: 8/10.

ASTROPHYSICAL JOURNAL (2023)

Article Astronomy & Astrophysics

Fundamental-Harmonic Pairs of Interplanetary Type III Radio Bursts

Immanuel Christopher Jebaraj, Vladimir Krasnoselskikh, Marc Pulupa, Jasmina Magdalenic, Stuart D. Bale

Summary: This research report presents the first detailed observations of type III fundamental-harmonic pairs in hectokilometric wavelengths, observed by the Parker Solar Probe. The report provides a statistical analysis of the spectral characteristics, polarization measurements, and other characteristics of the fundamental-harmonic pairs, drawing conclusions based on the observations.

ASTROPHYSICAL JOURNAL LETTERS (2023)

Article Astronomy & Astrophysics

Reconstruction of Polarization Properties of Whistler Waves From Two Magnetic and Two Electric Field Components: Application to Parker Solar Probe Measurements

L. Colomban, O. V. Agapitov, V. Krasnoselskikh, M. Kretzschmar, T. Dudok de Wit, S. Karbashewski, F. S. Mozer, J. W. Bonnell, S. Bale, D. Malaspina, N. E. Raouafi

Summary: This article discusses the technical issues and limitations of the search-coil magnetometer aboard Parker Solar Probe (PSP) and proposes a method to reconstruct missing components using the electric field instrument. The method has been validated and successfully applied to determine the polarization of a whistler event.

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS (2023)

Article Astronomy & Astrophysics

Ion Kinetics of Plasma Interchange Reconnection in the Lower Solar Corona

Vladimir Krasnoselskikh, Arnaud Zaslavsky, Anton Artemyev, Clara Froment, Thierry Dudok de Wit, Nour E. Raouafi, Oleksiy V. Agapitov, Stuart D. Bale, Jaye L. Verniero

Summary: The exploration of the inner heliosphere by the Parker Solar Probe has revealed the presence of switchbacks in the highly structured solar wind, which may be generated by interchange reconnection (IR). Although IR does not significantly contribute to the heating and acceleration of the solar wind, it affects the way the solar wind is connected to its sources and can lead to a new energy balance.

ASTROPHYSICAL JOURNAL (2023)

No Data Available