期刊
SPACE SCIENCE REVIEWS
卷 214, 期 1, 页码 -出版社
SPRINGER
DOI: 10.1007/s11214-017-0435-8
关键词
Solar wind; Turbulence; Intermittency; Coherent structures
资金
- NASA Heliophysics Grand Challenges TMS program [NNX14AI63G]
- LWS program [NNX15AB88G]
- Solar Probe Plus ISOIS project [D99031L]
- NSF SHINE and Solar Terrestrial programs
- Agenzia Spaziale Italiana [ASI-INAF 2015-039-R.O]
- NASA [681607, NNX14AI63G] Funding Source: Federal RePORTER
The method called PVI (Partial Variance of Increments) has been increasingly used in analysis of spacecraft and numerical simulation data since its inception in 2008. The purpose of the method is to study the kinematics and formation of coherent structures in space plasmas, a topic that has gained considerable attention, leading the development of identification methods, observations, and associated theoretical research based on numerical simulations. This review paper will summarize key features of the method and provide a synopsis of the main results obtained by various groups using the method. This will enable new users or those considering methods of this type to find details and background collected in one place.
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