Local Well-Posedness of the Plasma-Vacuum Interface Problem for the Ideal Incompressible Mhd
SSRN, ISSN: 1556-5068
2023
- 129Usage
Metric Options: Counts1 Year3 YearSelecting the 1-year or 3-year option will change the metrics count to percentiles, illustrating how an article or review compares to other articles or reviews within the selected time period in the same journal. Selecting the 1-year option compares the metrics against other articles/reviews that were also published in the same calendar year. Selecting the 3-year option compares the metrics against other articles/reviews that were also published in the same calendar year plus the two years prior.
Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Article Description
In this article, we consider the plasma-vacuum interface problem for the incompressible ideal MHD. The plasma magnetic field is tangential to the interface while the vacuum magnetic field vanishes. We shall prove the stability of the interface under the Taylor sign condition. By deriving the evolution equation of the interface in the Eulerian coordinates, we are able to identify different stability mechanisms which correspond to the hyperboliticity of this evolution equation. Once the optimal regularity of the interface is obtained, all the other quantities can be estimated in the Eulerian coordinates. Therefore, we do not need the change of coordinates or the use of the Alinhac’s good unknowns.
Bibliographic Details
Elsevier BV
Provide Feedback
Have ideas for a new metric? Would you like to see something else here?Let us know