Stochastic modeling of blob-like plasma filaments in the scrape-off layer: Time-dependent velocities and pulse stagnation

TL;DR

This paper presents a stochastic model for plasma filaments in the scrape-off layer, incorporating time-dependent velocities and pulse stagnation, revealing how these factors influence radial profiles and plasma-surface interactions.

Contribution

It introduces a novel stochastic model with time-dependent velocities and pulse damping, aligning with experimental observations of plasma filament behavior.

Findings

Pulse stagnation causes increased waiting times radially outward.

Mean process decreases exponentially with radial distance when velocity is proportional to amplitude.

Higher average pulse velocities flatten radial profiles and increase fluctuation levels.

Abstract

A stochastic model for a super-position of uncorrelated pulses with a random distribution of and correlations between amplitudes and velocities is analyzed. The pulses are assumed to move radially with fixed shape and amplitudes decreasing exponentially in time due to linear damping. The pulse velocities are taken to be time-dependent with a power law dependence on the instantaneous amplitudes, as suggested by blob velocity scaling theories. In accordance with experimental measurements, the pulse function is assumed to be exponential and the amplitudes are taken to be exponentially distributed. As a consequence of linear damping and time-dependent velocities, it is demonstrated that the pulses stagnate during their radial motion. This makes the average pulse waiting time increase radially outwards in the scrape-off layer of magnetically confined plasmas. In the case that pulse velocities are proportional to their amplitudes, the mean value of the process decreases exponentially with radial coordinate, similar to the case when all pulses have the same, time-independent velocity. The profile e-folding length is then given by the product of the average pulse velocity and the parallel transit time. Moreover, both the average pulse amplitude and the average velocity are the same at all radial positions due to stagnation of slow and small-amplitude pulses. In general, an increasing average pulse velocity results in a flattened radial profile of the mean value of the process as well as a higher relative fluctuation level, strongly enhancing plasma-surface interactions.