Energy cascades in large-scale solar flare reconnection
Astrophysics and Space Science Proceedings, ISSN: 1570-6605, Vol: 33, Page: 43-48
2012
- 3Citations
- 2Captures
Metric Options: CountsSelecting 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.
Conference Paper Description
Very fast energy release is sometimes observed in large-scale current layers formed in astrophysical plasmas. Solar flares represent a clear example. The dissipation and changes of the magnetic field topology in the almost collisionless plasmas are inherently related to plasma-kinetic processes in very thin current sheets (CSs). Question arises, how the originally thick current layer is efficiently fragmented into these small-scale dissipative CSs. We investigated this question by means of high-resolution MHD simulations. In addition to the earlier considered chain plasmoid instability we identified other elementary process for energy transport from large to small scales – fragmenting coalescence of plasmoids. This result changes so far basically 1D picture of energy cascade in a large scale magnetic reconnection and reveals multi-dimensional nature of the fragmentation process. At the same moment it shows that plasmoid coalescence contributes – quite surprisingly – to the direct energy cascade.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=84922370964&origin=inward; http://dx.doi.org/10.1007/978-3-642-30442-2_5; http://link.springer.com/10.1007/978-3-642-30442-2_5; http://link.springer.com/content/pdf/10.1007/978-3-642-30442-2_5; https://doi.org/10.1007%2F978-3-642-30442-2_5; https://dx.doi.org/10.1007/978-3-642-30442-2_5; https://link.springer.com/chapter/10.1007/978-3-642-30442-2_5
Springer Science and Business Media LLC
Provide Feedback
Have ideas for a new metric? Would you like to see something else here?Let us know