自由才谨慎
发表于 2025-3-21 18:30:57
书目名称MHD Structures, Waves and Turbulence in the Solar Wind影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0620156<br><br> <br><br>书目名称MHD Structures, Waves and Turbulence in the Solar Wind影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0620156<br><br> <br><br>书目名称MHD Structures, Waves and Turbulence in the Solar Wind网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0620156<br><br> <br><br>书目名称MHD Structures, Waves and Turbulence in the Solar Wind网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0620156<br><br> <br><br>书目名称MHD Structures, Waves and Turbulence in the Solar Wind被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0620156<br><br> <br><br>书目名称MHD Structures, Waves and Turbulence in the Solar Wind被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0620156<br><br> <br><br>书目名称MHD Structures, Waves and Turbulence in the Solar Wind年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0620156<br><br> <br><br>书目名称MHD Structures, Waves and Turbulence in the Solar Wind年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0620156<br><br> <br><br>书目名称MHD Structures, Waves and Turbulence in the Solar Wind读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0620156<br><br> <br><br>书目名称MHD Structures, Waves and Turbulence in the Solar Wind读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0620156<br><br> <br><br>
tolerance
发表于 2025-3-21 23:15:36
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Tincture
发表于 2025-3-22 01:40:13
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否认
发表于 2025-3-22 07:10:05
ons and magnetohydrodynamic waves and turbulence,preference being given to phenomena in the inner heliosphere. Emphasisis placed on the progress made in the past decade in the understandingof the nature and origin of especially small-scale, compressible andincompressible fluctuations. Turbulence mod
不规则的跳动
发表于 2025-3-22 10:04:50
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Merited
发表于 2025-3-22 13:30:49
The Heating and Acceleration Effects on the Solar Wind,c moment ../., which should be conserved in a collisionless double-adiabatic plasma. However, it is found observationally that ../. increases with increasing heliocentric distance. These results are interpreted as evidence that solar wind protons in high-speed streams are heated between 0.3 and 1 AU. Yet, the heat source remains to be determined.
buoyant
发表于 2025-3-22 20:25:08
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粗鄙的人
发表于 2025-3-22 22:43:52
Introduction,so connected with basic MHD turbulence theory. The solar wind can be considered as a natural laboratory for the investigation of MHD turbulence in supersonic flow. So, studying the properties of interplanetary fluctuations has always been among the major research topics in solar wind physics from th
Soliloquy
发表于 2025-3-23 02:35:26
Data Analysis and Basic Observational Results,rgodic random function of time. At least it can be meaningfully viewed as a’weakly’ stationary random function (i.e., the stationarity of the average and the two-pointtime correlation function is ensured). The time averages of the products of turbulent fields at fixed points in space are equivalent
Overthrow
发表于 2025-3-23 09:14:27
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