activity
20082026
most citedThe multi-scale nature of the solar wind

424 citations · 2.6k across the 108 of their papers we have counts for

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32 papers · 1 filter

astro-ph.SR2026

Wave Emission and Absorption in a Near-Sun Proton-Cyclotron Wave Storm

Kristopher G Klein, Daniel Verscharen, Mihailo Martinovic +5

Quantification of energy transport and dissipation in weakly collisional heliospheric plasmas that are far from local thermodynamic equilibrium is an outstanding scientific problem…

astro-ph.SR2026

Decomposition of Solar Wind Velocity Distribution Functions with Orthogonal Polynomials

Byeongseon Park, Primoz Kajdic, Daniel Verscharen +7

We present a framework for decomposing solar-wind velocity distribution functions (VDFs) using orthogonal polynomial bases. We aim to establish a practical procedure for applying p…

astro-ph.SR2026

Collisionless stationary states of a stratified plasma in an expanding magnetic tube with stochastic heating

Luca Barbieri, Pascal Démoulin, Daniel Verscharen

We investigate the collisionless kinetic structure of the upper solar atmosphere in an expanding magnetic field. Building on established velocity-filtration models, we extend the s…

astro-ph.SR2026

Parker Solar Probe Observations of Preferential Heating of Protons over Alpha Particles near Turbulent Coherent Structures

Jiayang Xi, Tieyan Wang, Daniel Verscharen +15

Solar wind alpha particles exhibit preferential heating and acceleration relative to protons; however, their behavior in the vicinity of turbulent coherent structures remains less…

astro-ph.SR2026

The Damping and Instability of Ion-acoustic Waves in the Solar Wind: Solar Orbiter Observations

Hao Ran, Daniel Verscharen, Jesse Coburn +6

Observations of solar wind velocity distribution functions (VDFs) commonly reveal fine-scale structures. These features strongly influence kinetic processes such as wave damping an…

astro-ph.SR2026

A Non-Spherical Model for the Solar Coronal Magnetic Field

Ziqi Wu, Jiansen He, Chuanpeng Hou +7

The coronal magnetic field plays a fundamental role in governing coronal activities, driving space-weather events, and shaping the heliosphere. Due to a lack of direct observations…

astro-ph.SR2025

Alfvénic solar wind intervals observed by Solar Orbiter: Exploiting the capability of the SWA plasma suite and source region investigation

R. D'Amicis, J. M. Raines, S. Benella +32

Fast and slow solar wind have distinct properties linked to their solar sources.Alfvénic slow wind complicates the usual speed-based classification, especially at intermediate spee…

astro-ph.SR2025

How the Oblique Drift Instability Alters Solar Wind Heating and Constrains the Distribution of Solar Wind Observations

Mihailo M. Martinovic, Kristopher G. Klein, Leon Ofman +6

Ion-driven plasma instability thresholds, derived from linear theory, constrain the distribution of solar observations in parameter space, defining boundaries of stable plasma para…

astro-ph.SR2025

Double Power-law Electron Spectra in Solar Flares Due to Temperature Anisotropy Instabilities

Martín Astete, Mario Riquelme, Daniel Verscharen

Despite extensive observational and theoretical efforts, the physical processes responsible for shaping the diversity of accelerated electron spectra observed in solar flares remai…

astro-ph.SR2025

Observational Constraints on the Radial Evolution of O Temperature and Differential Flow in the Inner Heliosphere

Yeimy J. Rivera, Kristopher G. Klein, Joseph H. Wang +15

Over decades of solar wind observations, heavy ions have been observed to have a higher temperature and flow faster than protons in the solar corona and heliosphere. Remote observa…

astro-ph.SR2025★ 2 cited

Quasi-parallel anti-sunward propagating whistler waves associated to the electron-deficit in the near-Sun solar wind: Particle-in-Cell simulation

Alfredo Micera, Daniel Verscharen, Jesse T. Coburn +1

In-situ observations of the solar wind have shown that the electron velocity distribution function (VDF) consists of a quasi-Maxwellian core, comprising most of the electron popula…

astro-ph.SR2024

Impact of Two-Population -particle Distributions on Plasma Stability

Mihailo M. Martinović, Kristopher G. Klein, Rossana De Marco +3

The stability of weakly collisional plasmas is well represented by linear theory, and the generated waves play an essential role in the thermodynamics of these systems. The velocit…

astro-ph.SR2023

Solar Electron Beam -- Langmuir Wave Interactions and How They Modify Solar Electron Beam Spectra: Solar Orbiter Observations of a Match Made in the Heliosphere

Camille Y. Lorfing, Hamish A. S. Reid, Raul Gomez-Herrero +7

Solar Orbiter's four in-situ instruments have recorded numerous energetic electron events at heliocentric distances between 0.5 and 1au. We analyse energetic electron fluxes, spect…

astro-ph.SR2023

The Effects of Non-Equilibrium Velocity Distributions on Alfvén Ion-Cyclotron Waves in the Solar Wind

Jada Walters, Kristopher G. Klein, Emily Lichko +3

In this work, we investigate how the complex structure found in solar wind proton velocity distribution functions (VDFs), rather than the commonly assumed two-component bi-Maxwelli…

astro-ph.SR2023★ 7 cited

The effect of variations in magnetic field direction from turbulence on kinetic-scale instabilities

Simon Opie, Daniel Verscharen, Christopher H. K. Chen +2

At kinetic scales in the solar wind, instabilities transfer energy from particles to fluctuations in the electromagnetic fields while restoring plasma conditions towards thermodyna…

astro-ph.SR2023★ 3 cited

Does Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves?

Daniele Telloni, Gary P. Zank, Laxman Adhikari +32

Evidence for the presence of ion cyclotron waves, driven by turbulence, at the boundaries of the current sheet is reported in this paper. By exploiting the full potential of the jo…

astro-ph.SR2022★ 14 cited

Thermal energy budget of electrons in the inner heliosphere: Parker Solar Probe Observations

Joel B. Abraham, Daniel Verscharen, Robert T. Wicks +4

We present an observational analysis of the electron thermal energy budget using data from Parker Solar Probe. We use the macroscopic moments, obtained from our fits to the measure…

astro-ph.SR2022

Radial evolution of thermal and suprathermal electron populations in the slow solar wind from 0.13 to 0.5 au : Parker Solar Probe Observations

Joel B. Abraham, Christopher J Owen, Daniel Verscharen +8

We develop and apply a bespoke fitting routine to a large volume of solar wind electron distribution data measured by Parker Solar Probe (PSP) over its first five orbits, covering…

astro-ph.SR2022★ 13 cited

The Stability of the Electron Strahl against the Oblique Fast-magnetosonic/Whistler Instability in the Inner Heliosphere

Seong-Yeop Jeong, Joel B. Abraham, Daniel Verscharen +8

We analyze the micro-kinetic stability of the electron strahl in the solar wind depending on heliocentric distance. The oblique fast-magnetosonic/whistler (FM/W) instability has em…

astro-ph.SR2022

Test Problems for Potential Field Source Surface Extrapolations of Solar and Stellar Magnetic Fields

David Stansby, Daniel Verscharen

The potential field source surface (PFSS) equations are commonly used to model the coronal magnetic field of the Sun and other stars. As with any computational model, solving equat…

astro-ph.SR2021★ 32 cited

Exploring the Solar Wind from its Source on the Corona into the Inner Heliosphere during the First Solar Orbiter - Parker Solar Probe Quadrature

Daniele Telloni, Vincenzo Andretta, Ester Antonucci +68

This Letter addresses the first Solar Orbiter (SO) -- Parker Solar Probe (PSP) quadrature, occurring on January 18, 2021, to investigate the evolution of solar wind from the extend…

astro-ph.SR2021★ 58 cited

Strong perpendicular velocity-space in proton beams observed by Parker Solar Probe

J. L. Verniero, B. D. G. Chandran, D. E. Larson +16

The SWEAP instrument suite on Parker Solar Probe (PSP) has detected numerous proton beams associated with coherent, circularly polarized, ion-scale waves observed by PSP's FIELDS i…

astro-ph.SR2021★ 7 cited

Growth of Outward Propagating Fast-Magnetosonic/Whistler Waves in the Inner Heliosphere Observed by Parker Solar Probe

Jiansen He, Ying Wang, Xingyu Zhu +3

The solar wind in the inner heliosphere has been observed by Parker Solar Probe (PSP) to exhibit abundant wave activities. The cyclotron wave modes in the sense of ions or electron…

astro-ph.SR2021★ 13 cited

Deriving the bulk properties of solar wind electrons observed by Solar Orbiter: A preliminary study of electron plasma thermodynamics

Georgios Nicolaou, Robert T. Wicks, Christopher J. Owen +8

We demonstrate the calculation of solar wind electron bulk parameters from recent observations by Solar Wind Analyser Electron Analyser System on board Solar Orbiter. We use our me…