activity
20182022
most citedMagnetic connectivity of the ecliptic plane within 0.5 AU : PFSS modeling of the first PSP encounter

161 citations · 492 across the 11 of their papers we have counts for

collaborators
Showing physics.space-phShow all

7 papers · 1 filter

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-ph2019

The rotation angle distribution underlying magnetic field fluctuations in the 1/f range of solar wind turbulent spectra

L. Matteini, D. Stansby, T. S. Horbury +1

We discuss properties of large amplitude magnetic field fluctuations during fast Alfvenic solar wind streams, focussing on the statistics of the rotation angle between consecutive…

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-ph201873 cited

On the 1/f spectrum in the solar wind and its connection with magnetic compressibility

Lorenzo Matteini, David Stansby, Timothy Horbury +1

We discuss properties of Alfvénic fluctuations with large amplitude in plasmas characterised by low magnetic field compression. We note that in such systems power laws can not deve…

physics.space-ph2018

Alpha particle thermodynamics in the inner heliosphere fast solar wind

D. Stansby, D. Perrone, L. Matteini +2

Plasma processes occurring in the corona and solar wind can be probed by studying the thermodynamic properties of different ion species. However, most in-situ observations of posit…

physics.space-ph2018

Radial evolution of the solar wind in pure high-speed streams: HELIOS revised observations

D. Perrone, D. Stansby, T. Horbury +1

Spacecraft observations have shown that the proton temperature in the solar wind falls off with radial distance more slowly than expected for an adiabatic prediction. Usually, prev…