@inproceedings{5de232875b91482fb5f54f657c412ce7,
title = "Flux concentrations in turbulent convection",
abstract = "We present preliminary results from high resolution magneto-convection simulations where we find the formation of flux concentrations from an initially uniform magnetic field. The structures appear in roughly ten convective turnover times and live close to a turbulent diffusion time. The time scales are compatible with the negative effective magnetic pressure instability (NEMPI), although structure formation is not restricted to regions where the effective magnetic pressure is negative.",
keywords = "MHD, Sun: magnetic fields, turbulence",
author = "K{\"a}pyl{\"a}, {Petri J.} and Axel Brandenburg and Nathan Kleeorin and Mantere, {Maarit J.} and Igor Rogachevskii",
year = "2012",
month = aug,
day = "1",
doi = "10.1017/S1743921313002640",
language = "American English",
isbn = "9781107033832",
series = "Proceedings of the International Astronomical Union",
number = "S294",
pages = "283--288",
editor = "Kosovichev, {Alexander G.} and {de Gouveia Dal Pino}, Elisabete and Yihua Yan",
booktitle = "Solar and Astrophysical Dynamos and Magnetic Activity",
edition = "S294",
}