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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Showing 2022Show all

12 papers · 1 filter

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…

physics.space-ph2022

The essential role of multi-point measurements in investigations of turbulence, three-dimensional structure, and dynamics: the solar wind beyond single scale and the Taylor Hypothesis

W. H. Matthaeus, S. Adhikari, R. Bandyopadhyay +49

Space plasmas are three-dimensional dynamic entities. Except under very special circumstances, their structure in space and their behavior in time are not related in any simple way…

physics.space-ph2022★ 15 cited

Conditions for proton temperature anisotropy to drive instabilities in the solar wind

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

Using high-resolution data from Solar Orbiter, we investigate the plasma conditions necessary for the proton temperature anisotropy driven mirror-mode and oblique firehose instabil…

physics.plasm-ph2022★ 10 cited

Energy transport during 3D small-scale reconnection driven by anisotropic plasma turbulence

Jeffersson A. Agudelo Rueda, Daniel Verscharen, Robert T. Wicks +6

Energy dissipation in collisionless plasmas is a longstanding fundamental physics problem. Although it is well known that magnetic reconnection and turbulence are coupled and trans…

physics.plasm-ph2022★ 19 cited

Whistler Waves As a Signature of Converging Magnetic Holes in Space Plasmas

Wence Jiang, Daniel Verscharen, Hui Li +2

Magnetic holes are plasma structures that trap a large number of particles in a magnetic field that is weaker than the field in its surroundings. The unprecedented high time-resolu…

physics.space-ph2022

Electron-driven instabilities in the solar wind

Daniel Verscharen, Benjamin D. G. Chandran, Elisabetta Boella +9

The electrons are an essential particle species in the solar wind. They often exhibit non-equilibrium features in their velocity distribution function. These include temperature an…