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20182022
most citedScattering of Strahl Electrons in the Solar Wind between 0.3 and 1 au: Helios Observations

85 citations · 236 across the 7 of their papers we have counts for

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physics.space-ph202211 cited

The Kinetic Expansion of Solar-Wind Electrons: Transport Theory and Predictions for the very Inner Heliosphere

Seong-Yeop Jeong, Daniel Verscharen, Christian Vocks +9

We propose a transport theory for the kinetic evolution of solar-wind electrons in the heliosphere. We derive a gyro-averaged kinetic transport equation that accounts for the spher…

physics.space-ph2021

Whistler wave occurrence and the interaction with strahl electrons during the first encounter of Parker Solar Probe

V. K. Jagarlamudi, T. Dudok de Wit, C. Froment +16

We studied the properties and occurrence of narrow band whistler waves and their interaction with strahl electrons observed between 0.17 and 0.26 au during the first encounter of P…

physics.space-ph202030 cited

Whistler Waves and Electron Properties in the Inner Heliosphere: Helios Observations

Vamsee Krishna Jagarlamudi, Olga Alexandrova, Laura Bercic +4

We present the analysis of narrowband whistler wave signatures observed in the inner heliosphere (0.3-1 au). These signatures are bumps in the spectral density in the 10-200 Hz fre…

physics.space-ph2020

Resonant whistler-electron interactions: MMS observations vs. test-particle simulation

Etienne Behar, Fouad Sahraoui, Laura Bercic

Simultaneous observation of characteristic 3-dimensional (3D) signatures in the electron velocity distribution function (VDF) and intense quasi-monochromatic waves by the Magnetosp…

physics.space-ph2019

The origin of slow Alfvénic solar wind at solar minimum

D. Stansby, L. Matteini, T. S. Horbury +3

Although the origins of slow solar wind are unclear, there is increasing evidence that at least some of it is released in a steady state on over-expanded coronal hole magnetic fiel…

physics.space-ph201985 cited

Scattering of Strahl Electrons in the Solar Wind between 0.3 and 1 au: Helios Observations

L. Bercic, M. Maksimovic, S. Landi +1

Electron velocity distribution functions in the solar wind according to standard models consist of 4 components, of which 3 are symmetric - the core, the halo, and the superhalo, a…