59th Annual Meeting of the APS Division of Plasma Physics 
Volume 62, Number 12
Monday–Friday, October 23–27, 2017;
Milwaukee, Wisconsin
Session YI2: SOL and Divertor
9:30 AM–12:30 PM, 
Friday, October 27, 2017
Room: 102ABC
Chair: John Canik, Oak Ridge National Laboratory
Abstract ID: BAPS.2017.DPP.YI2.4
Abstract: YI2.00004 : Density profiles in the Scrape-Off Layer interpreted through filament dynamics
11:00 AM–11:30 AM
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Author:
Fulvio Militello
(Culham Centre for Fusion Energy)
We developed a new theoretical framework to clarify the relation between 
radial Scrape-Off Layer density profiles and the fluctuations that generate 
them. The framework provides an interpretation of the experimental features 
of the profiles and of the turbulence statistics on the basis of simple 
properties of the filaments, such as their radial motion and their draining 
towards the divertor. L-mode and inter-ELM filaments are described as a 
Poisson process in which each event is independent and modelled with a wave 
function of amplitude and width statistically distributed according to 
experimental observations and evolving according to fluid equations. We will 
rigorously show that radially accelerating filaments, less efficient 
parallel exhaust and also a statistical distribution of their radial 
velocity can contribute to induce flatter profiles in the far SOL and 
therefore enhance plasma-wall interactions. A quite general result of our 
analysis is the resiliency of this non-exponential nature of the profiles 
and the increase of the relative fluctuation amplitude towards the wall, as 
experimentally observed. According to the framework, profile broadening at 
high fueling rates can be caused by interactions with neutrals (e.g. charge 
exchange) in the divertor or by a significant radial acceleration of the 
filaments. The framework assumptions were tested with 3D numerical 
simulations of seeded SOL filaments based on a two fluid model. In 
particular, filaments interact through the electrostatic field they generate 
only when they are in close proximity (separation comparable to their width 
in the drift plane), thus justifying our independence hypothesis. In 
addition, we will discuss how isolated filament motion responds to 
variations in the plasma conditions, and specifically divertor conditions. 
Finally, using the theoretical framework we will reproduce and interpret 
experimental results obtained on JET, MAST and HL-2A.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2017.DPP.YI2.4