3-D VPIC simulation of an vortex-induced reconnection event observed by MMS
- Nakamura, Takuma | Oak Ridge National Laboratory
- Daughton, William | Oak Ridge National Laboratory
Overview
Description
The data set consists of a 3-D fully kinetic (VPIC) simulation of an in-situ observation event at the Earth's magnetopause by the NASA MMS spacecraft on September 8, 2015. The results show a turbulent development of magnetic reconnection induced by the Kelvin-Helmohltz vortex, and resulting significantly efficient plasma mixing across the magnetopause. The vortex-induced reconnection signatures are well consistent with the MMS observations. These results are published in some scientific journals such as Nature Communications. Fortran unformatted files with 1024x1536x512 cells, which have been compressed from original ones with 2048x3072x1024 cells, are archived for selected time slices of field and moment data shown in these papers.
Funding resources
DOE contract number
DE-AC05-00OR22725Originating research organization
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States);Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States);Austrian Academy of SciencesSponsoring organization
Office of Science (SC)Details
DOI
10.13139/OLCF/1395321Release date
September 28, 2017Dataset
Dataset type
AS Animations/SimulationsOther contract number(s)
NASA grant - NNH13AV26IAcknowledgements
Users should acknowledge the OLCF in all publications and presentations that speak to work performed on OLCF resources:
This research used resources of the Oak Ridge Leadership Computing Facility at the Oak Ridge National Laboratory, which is supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC05-00OR22725.
Category
- 58 GEOSCIENCES,
- 79 ASTRONOMY AND ASTROPHYSICS
Keywords
- Magnetosphere,
- Magnetic reconnection,
- Kelvin-Helmholtz instability,
- mixing,
- kinetic simulaiton,
- VPIC code