PSP Bibliography





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Found 6 entries in the Bibliography.


Showing entries from 1 through 6


2022

In Situ Signature of Cyclotron Resonant Heating in the Solar Wind

Bowen, Trevor; Chandran, Benjamin; Squire, Jonathan; Bale, Stuart; Duan, Die; Klein, Kristopher; Larson, Davin; Mallet, Alfred; McManus, Michael; Meyrand, Romain; Verniero, Jaye; Woodham, Lloyd;

Published by: \prl      Published on: oct

YEAR: 2022     DOI: 10.1103/PhysRevLett.129.165101

Parker Data Used

Cross-scale Correlations in Imbalanced Solar Wind Turbulence: Parker Solar Probe Observations

Zhao, G.~Q.; Meyrand, R.; Feng, H.~Q.; Wu, D.~J.; Kasper, J.~C.;

Published by: \apj      Published on: oct

YEAR: 2022     DOI: 10.3847/1538-4357/ac9380

Parker Data Used; Solar wind; interplanetary turbulence; Solar coronal heating; Space plasmas; Plasma physics; 1534; 830; 1989; 1544; 2089

On the properties of Alfv\ enic switchbacks in the expanding solar wind: Three-dimensional numerical simulations

Switchbacks-abrupt reversals of the magnetic field within the solar wind-have been ubiquitously observed by Parker Solar Probe (PSP). Their origin, whether from processes near the solar surface or within the solar wind itself, remains under debate and likely has key implications for solar wind heating and acceleration. Here, using three-dimensional expanding box simulations, we examine the properties of switchbacks arising from the evolution of outwards-propagating Alfv\ en waves in the expanding solar wind in detail. Our go ...

Johnston, Zade; Squire, Jonathan; Mallet, Alfred; Meyrand, Romain;

Published by: Physics of Plasmas      Published on: jul

YEAR: 2022     DOI: 10.1063/5.0097983

Parker Data Used; Astrophysics - Solar and Stellar Astrophysics; Physics - Plasma Physics

Erratum: On the properties of Alfv\ enic switchbacks in the expanding solar wind: Three-dimensional numerical simulations [Phys. Plasmas 29, 072902 (2022)]

Switchbacks — abrupt reversals of the magnetic field within the solar wind — have been ubiquitously observed by Parker Solar Probe (PSP). Their origin, whether from processes near the solar surface or within the solar wind itself, remains under debate, and likely has key implications for solar wind heating and acceleration. Here, using three-dimensional expanding box simulations, we examine the properties of switchbacks arising from the evolution of outwards-propagating Alfv\ en waves in the expanding solar wind ...

Johnston, Zade; Squire, Jonathan; Mallet, Alfred; Meyrand, Romain;

Published by: Physics of Plasmas      Published on: dec

YEAR: 2022     DOI: 10.1063/5.0133296

Parker Data Used; Astrophysics - Solar and Stellar Astrophysics; Physics - Plasma Physics

2021

On the violation of the zeroth law of turbulence in space plasmas

The zeroth law of turbulence states that, for fixed energy input into large-scale motions, the statistical steady state of a turbulent system is independent of microphysical dissipation properties. This behaviour, which is fundamental to nearly all fluid-like systems from industrial processes to galaxies, occurs because nonlinear processes generate smaller and smaller scales in the flow, until the dissipation - no matter how small - can thermalise the energy input. Using direct numerical simulations and theoretical arguments ...

Meyrand, R.; Squire, J.; Schekochihin, A.; Dorland, W.;

Published by: Journal of Plasma Physics      Published on: 05/2021

YEAR: 2021     DOI: 10.1017/S0022377821000489

space plasma physics; astrophysical plasmas; plasma nonlinear phenomena; Physics - Space Physics; Astrophysics - Solar and Stellar Astrophysics; Nonlinear Sciences - Chaotic Dynamics; Physics - Plasma Physics; Parker Data Used

2020

In-situ Switchback Formation in the Expanding Solar Wind

Recent near-Sun solar-wind observations from Parker Solar Probe have found a highly dynamic magnetic environment, permeated by abrupt radial-field reversals, or "switchbacks." We show that many features of the observed turbulence are reproduced by a spectrum of Alfv\ enic fluctuations advected by a radially expanding flow. Starting from simple superpositions of low-amplitude outward-propagating waves, our expanding-box compressible magnetohydrodynamic simulations naturally develop switchbacks because (i) the normalized am ...

Squire, J.; Chandran, B.; Meyrand, R.;

Published by: The Astrophysical Journal      Published on: 03/2020

YEAR: 2020     DOI: 10.3847/2041-8213/ab74e1

Astrophysics - Solar and Stellar Astrophysics; Parker Data Used; parker solar probe; Physics - Plasma Physics; Physics - Space Physics; Solar Probe Plus



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