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SoWHat

Solar Wind Heating and Turbulence

Total Cost €

EC-Contrib. €

Partnership

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Outcomes and
results

SoWHat project word cloud

Explore the words cloud of the SoWHat project. It provides you a very rough idea of what is the project "SoWHat" about.

scaling particles mechanisms acceleration plasma numerical emphasized theories astrophysical cascade observations usually simulations dissipated solar sw model particle kinetic frequently situ magnetic magnetohydrodynamic energy plasmas turbulence scales mhd dissipation answering combines missions multispacecraft heating kolmogorov wind behavior minus terminates debated fundamental question innovative nonlinear interactions spectra hotly smaller multiple data thought

Project "SoWHat" data sheet

The following table provides information about the project.

Coordinator	ECOLE POLYTECHNIQUE Organization address address: ROUTE DE SACLAY city: PALAISEAU CEDEX postcode: 91128 website: http://www.polytechnique.fr contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.
Coordinator Country	France [FR]
Project website	https://www.lpp.polytechnique.fr/-Romain-Meyrand-567-
Total cost	264˙668 €
EC max contribution	264˙668 € (100%)
Programme	1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
Code Call	H2020-MSCA-IF-2014
Funding Scheme	MSCA-IF-GF
Starting year	2015
Duration (year-month-day)	from 2015-11-01 to 2018-10-31

Partnership

Take a look of project's partnership.

#	participants	country	role	EC contrib. [€]
1	ECOLE POLYTECHNIQUE ECOLE POLYTECHNIQUE Organization address address: ROUTE DE SACLAY city: PALAISEAU CEDEX postcode: 91128 website: http://www.polytechnique.fr contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.	FR (PALAISEAU CEDEX)	coordinator	264˙668.00
2	THE REGENTS OF THE UNIVERSITY OF CALIFORNIA THE REGENTS OF THE UNIVERSITY OF CALIFORNIA Organization address address: FRANKLIN STREET 1111, 12 FLOOR city: OAKLAND CA postcode: 94607 website: n.a. contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.	US (OAKLAND CA)	partner	0.00

Map

Project objective

Observations of solar wind (SW) turbulence have usually emphasized magnetohydrodynamic (MHD) scales where the Kolmogorov scaling f −5/3 of the magnetic spectra is frequently observed. These spectra are thought to result from strongly nonlinear interactions. However, the question as to how turbulence of the MHD scales terminates its cascade at smaller (kinetic) scales is still hotly debated. Answering this question is indeed fundamental to understanding the processes of particle acceleration and plasma heating in the SW and in other astrophysical plasmas. This project aims at studying the mechanisms of energy dissipation in solar wind. We will use a innovative multiple approach that combines in-situ fields and particles data available from the multispacecraft missions, numerical simulations and theories to model the complex behavior of turbulence cascade at kinetic scales where it is dissipated.

Publications

List of publications.
year	authors and title	journal	last update
2019	Romain Meyrand, Anjor Kanekar, William Dorland, Alexander A. Schekochihin Fluidization of collisionless plasma turbulence published pages: , ISSN: 0027-8424, DOI:	Proceedings of the National Academy of Sciences	2019-09-02
2018	Romain Meyrand, Khurom H. Kiyani, Ã–zgur D. GÃ¼rcan, SÃ©bastien Galtier Coexistence of Weak and Strong Wave Turbulence in Incompressible Hall Magnetohydrodynamics published pages: 31066, ISSN: 2160-3308, DOI: 10.1103/physrevx.8.031066	Physical Review X 8/3	2019-09-02
2016	Romain Meyrand, SÃ©bastien Galtier, Khurom H. Kiyani Direct Evidence of the Transition from Weak to Strong Magnetohydrodynamic Turbulence published pages: , ISSN: 0031-9007, DOI: 10.1103/physrevlett.116.105002	Physical Review Letters 116/10	2019-09-02

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