activity
20182025
collaborators

6 papers

physics.plasm-ph2025

CIEMAT-QI4X: a reactor-relevant quasi-isodynamic stellarator configuration compatible with an island divertor

E. Sánchez, J. L. Velasco, I. Calvo +3

A four-field-period quasi-isodynamic stellarator configuration is presented that exhibits small neoclassical and electrostatic turbulent transport, good fast-ion confinement over a…

physics.plasm-ph2025

Modification of ion-temperature-gradient turbulence by impurities in stellarator plasmas

Ivan Calvo, Felix I. Parra, Hanne Thienpondt +1

Recent nonlinear gyrokinetic simulations have shown that impurities can strongly modify the turbulent heat flux in stellarator plasmas. Here, the ion-temperature-gradient (ITG) dis…

physics.plasm-ph2023

Electrostatic microturbulence in W7-X: comparison of local gyrokinetic simulations with Doppler reflectometry measurements

A. González-Jerez, J. M. García-Regaña, I. Calvo +5

The first experimental campaigns of Wendelstein 7-X (W7-X) have shown that turbulence plays a decisive role in the performance of neoclassically optimized stellarators. This stress…

physics.plasm-ph2021

Electrostatic gyrokinetic simulations in Wendelstein 7-X geometry: benchmark between the codes stella and GENE

A. González-Jerez, P. Xanthopoulos, J. M. García-Regaña +6

The first experimental campaigns have proven that, due to the optimization of the magnetic configuration with respect to neoclassical transport, the contribution of turbulence is e…

physics.plasm-ph2019

KNOSOS: a fast orbit-averaging neoclassical code for stellarator geometry

J. L. Velasco, I. Calvo, F. I. Parra +1

KNOSOS (KiNetic Orbit-averaging SOlver for Stellarators) is a freely available, open-source code (\href{https://github.com/joseluisvelasco/KNOSOS}{https://github.com/joseluisvelasc…

physics.plasm-ph2018

Electrostatic potential variations on stellarator magnetic surfaces in low collisionality regimes

Ivan Calvo, J. L. Velasco, Felix I. Parra +2

The component of the neoclassical electrostatic potential that is non-constant on the magnetic surface, that we denote by , can affect radial transport of highly charged i…