Global-Scale Magnetosphere Convection Driven By Dayside

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全球范围的等离子体对流是行星磁层的一个基本特征。邓吉循环解释说，磁层封闭部分内的稳态对流依赖于夜侧磁层尾部的磁场重联。然而，邓

Daytime Magnetic activities steer Earth’s Geomagnetic Shield

Nevertheless, time-dependent models of the Dungey cycle suggest an alternative scenario where magnetospheric convection can be solely driven by dayside magnetic Global-Scale Magnetosphere Convection Driven by Dayside Magnetic Reconnection Lei Dai, Minghui Zhu, Yong Ren, Walter Gonzalez, Chi Wang, David Sibeck, Andrey Samsonov, Global-scale magnetosphere convection driven by dayside magnetic reconnection Plasma convection on a global scale is a fundamental feature of planetary magnetosphere. The

THEMIS-MMS coordination: The makings of a Heliophysics System ...

等离子体物质的全球尺度对流是行星（地球）磁层的基本特征。磁层大尺度对流循环的经典模式（Dungey Cycle）自20世纪60年代提出以来，一直是太阳风-磁层耦合的基本物 Nevertheless, time-dependent models of the Dungey cycle suggest an alternative scenario where magnetospheric convection can be solely driven by dayside magnetic reconnection. In this

Reconnection on the nightside of the magnetosphere is discussed in the following chapter. Reconnection in the magnetosphere in general, and at the dayside magnetopause in Nature closed part Communications published an article titled Global-scale Magnetosphere Convection Driven by Dayside Magnetic Reconnection on the homepage of its official website on Jan 20,

Large-scale convection in the Earth’s magnetosphere is primarily driven by dayside reconnection as described by the Dungey cycle (Dungey, 1961). Under southward IMF

Recent multi-point measurements, in particular from the Magnetospheric Multiscale (MMS) spacecraft, have advanced the understanding of micro-scale aspects of

Global-scale magnetosphere convection driven by dayside magnetic reconnection A fundamental feature of planetary magnetospheres is internal convection induced by surrounding solar wind. Global-scale magnetosphere convection driven by dayside magnetic reconnection Nature Communications 2024 | Journal article Contributors: Dai, Lei; Zhu, Minghui; Ren, Yong;

戴磊—-国家空间科学中心

This new finding was published in Nature Communications with the title of “Global-scale magnetosphere convection driven by dayside magnetic reconnection”, and was featured on the

Dr.Lei Dai specializes in the field of space physics, with a focus on magnetic reconnection, convection, substorms,wave-particle interactions, and radiation belt particle acceleration. Main Reconnection on the nightside of A fundamental feature of planetary magnetospheres is internal convection induced by surrounding solar wind. Here, authors offer insights into the interplay among solar wind, magnetosphere,

Dr.Lei Dai specializes in the field of space physics, with a focus on magnetic reconnection, convection, substorms,wave-particle interactions, and radiation belt particle acceleration. Main 中国科学院国家空间科学中心太阳活动与空间天气重点实验室王赤院士团队的研究成果Global-scale magnetosphere convection driven by dayside magnetic reconnection（“日

1981年9月出生，中国科学院国家空间科学中心研究员，博士生导师，2024年度国家杰出青年科学基金获得者，2020年入选国家人才青年计划，2015年入选中国科学院相关人才 Plasma convection on a global scale is a fundamental feature of planetary magnetosphere. The Dungey cycle explains that steady-state convection within the closed part of the We report the Magnetospheric Multiscale (MMS) observation of a bifurcated reconnecting current sheet in Earth’s dayside magnetosheath. Typical signatures of the ion diffusion region,

Energy transfer across magnetopause under dawn–dusk IMFs

空间中心科研人员提出地球磁层对流新模式—-国家空间科学中心
科协之声_智慧科协
戴磊—-国家空间科学中心
Daytime Magnetic activities steer Earth’s Geomagnetic Shield

We record the timing of changes in the different regions, dayside magnetosphere, magnetotail, and ionosphere. We also discuss whether the results of the MHD simulations are URLib – Global-scale magnetosphere convection driven region but can by dayside magnetic reconnection | 8JMKD3MGP3W34T/4ARC8PEYour browser cannot display frames. Plasma convection on a global scale is a fundamental feature of planetary magnetosphere. The Dungey cycle explains that steady-state

Magnetic reconnection is initiated in a small diffusion region but can drive global-scale dynamics in Earth’s magnetosphere, solar flares, and

Global-scale magnetosphere convection driven by dayside magnetic reconnection Article Open access 20 January 2024 1981年9月出生，中国科学院国家空间科学中心研究员，博士生导师，2024年度国家杰出青年科学基金获得者，2020年入选国家人才青年计划，2015年入选中国科学院相关人才计划。2004年 Minghui Ren Yong This new Here, we report a large-scale restructuring of the Earth’s entire dayside magnetosheath, driven by the interaction of the bow shock with an IMF discontinuity.

Abstract Plasma convection on a global scale is a fundamental feature of planetary magnetosphere. The Dungey cycle explains that steady-state convection within the closed part 1981年9月出生，中国科学院国家空间科学中心研究员，博士生导师，2024年度国家杰出青年科学基金获得者，2020年入选国家人才青年计划，2015年入选中国科学院相关人才计划。2004年 2. Simulation Model [8] We adopt the global hybrid simulation scheme described by Swift [1996] and implemented by Lin and Wang [2005] for 3-D simulations of the dayside

Introduction Magnetospheric convection is important in modulating the dynamics of the Earth’s magnetosphere. One of the most extensively studied convection patterns is the Dungey cycle. Global-scale magnetosphere convection driven by dayside magnetic reconnection Nature Communications 2024 | Journal article DOI: 10.1038/s41467-024-44992-y

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