Multipoint Observations of Sharp Boundaries of Solar Wind Density Structures

G. N. Zastenker; M. O. Riazantseva; P. E. Eiges

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Multipoint Observations of Sharp Boundaries of Solar Wind Density Structures

机译：太阳风密度结构尖锐边界的多点观测

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The results of comparison of the characteristics of sharp boundaries of small-scale and medium-scale solar wind structures in the case of their simultaneous observation on widely spaced spacecraft are described. It is shown that even very sharp boundaries, with duration of several seconds or fractions of a second, retain their amplitude and remain very sharp during solar wind propagation to distances of up to a million kilometers.

机译：描述了在大空间航天器上同时观测的情况下，小规模和中型太阳风结构的尖锐边界特征的比较结果。结果表明，即使是非常尖锐的边界（持续时间为几秒或几分之一秒），也可以保持其振幅，并在太阳风传播至一百万公里的距离时保持非常尖锐的状态。

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来源
《Cosmic research》 |2006年第6期|p.493-499|共7页
作者
G. N. Zastenker; M. O. Riazantseva; P. E. Eiges;
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作者单位

Space Research Institute, Russian Academy of Sciences, Profsoyuznaya ul. 84/32, Moscow, 117997 Russia;

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原文格式 PDF
正文语种 eng
中图分类航天（宇宙航行）;
关键词
solar wind plasma; waves and discontinuities;

机译：太阳风等离子体;波和不连续性;

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专利

1. Multipoint observations of the dynamics of the sharp solar wind structure boundaries [J] . G. Zastenker, M. Riazantseva Planetary and space science . 2007,第15期

机译：尖锐的太阳风结构边界动力学的多点观测
2. Similarity and difference of the durations of the small-scale solar wind structure boundaries by multipoint observations [J] . Zastenker G, Riazantseva M Journal of atmospheric and solar-terrestrial physics . 2008,第2a4期

机译：多点观测的小尺度太阳风结构边界持续时间的异同
3. Solar Wind Structure Dynamics by Multipoint Observations [J] . G. N. Zastenker, P. A. Dalin, A. A. Petrukovich, Physics and chemistry of the earth, Part C. Solar-terrestrial and planetary science . 2000,第1a2期

机译：多点观测的太阳风结构动力学
4. Three-Dimensional Solar Wind Structures Obtained with MHD Simulation Model Using Observation-Based Time-Varying Inner Boundary Map [C] . Keiji Hayashi, Munetoshi Tokumaru, Kenichi Fujiki, International Conference on Numerical Modeling of Space Plasma Flows . 2011

机译：使用基于观察的时变内边界映射，用MHD仿真模型获得的三维太阳风结构
5. Response of the geosynchronous magnetic field to sudden, large increases in solar wind density during perods of strongly southward IMF: MHD simulations and comparison to geosynchronous observations. [D] . Hernandez, John C. 2005

机译：在强烈向南的IMF期间，地球同步磁场对太阳风密度突然大幅度增加的响应：MHD模拟以及与地球同步观测的比较。
6. Ion‐driven instabilities in the solar wind: Wind observations of 19 March 2005 [O] . S. Peter Gary, Lan K. Jian, Thomas W. Broiles, -1

机译：太阳风中离子驱动的不稳定性：2005年3月19日的风观测
7. Reconstructing Solar Wind Inhomogeneous Structures From Stereoscopic Observations in White Light: Solar Wind Transients in 3‐D [O] . Xiaolei Li, Yuming Wang, Rui Liu, 2020

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8. Lunar Exospheric Column Densities and Solar Wind Access Beyond the Terminator from ROSAT Soft X-Ray Observations of Solar Wind Charge Exchange. [R] . Collier, M. R., Snowden, S. L., Holmstrom, M., 2014

机译：太阳风电荷交换的ROsaT软X射线观测中的月球外层柱密度和超越终结者的太阳风接入。

Multipoint Observations of Sharp Boundaries of Solar Wind Density Structures

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