Analytical solution of steady reconnection outflows in a time-varying three-dimensional reconnection model with generalized spatiotemporal distributions Article Swipe
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· 2024
· Open Access
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· DOI: https://doi.org/10.3389/fphy.2024.1439949
Magnetic reconnection is a fundamental mechanism for energy conversion in the realms of space physics, astrophysics, and plasma physics. Over the past few decades, obtaining analytical solutions for three-dimensional (3D) magnetic reconnection has remained a challenging endeavor. Due to the complexity and nonlinearity of the equations, analytical solutions can only be obtained when specific spatiotemporal distributions of magnetic fields or plasma flows are provided. Particularly, the evolution of reconnection flows in time-dependent 3D reconnection has not been analytically discussed. Additionally, quasi-steady magnetic reconnection persisting for several hours can be observed in the turbulent solar wind, which raises an important question: can steady reconnection flows theoretically exist in a time-dependent 3D magnetic reconnection model? In this study, a generalized analytical model for time-dependent kinematic 3D magnetic reconnection has been constructed. In the framework of pure analytical approach, it is firstly demonstrated that steady reconnection outflows can theoretically exist within a time-varying magnetic field. We have also analytically discussed the possibility of the existence of quasi-steady reconnection flows in 3D magnetic reconnection for turbulent magnetic fields in the solar wind. These findings broaden our understanding of the stability and necessary conditions for time-dependent 3D magnetic reconnection, offering new insights into quasi-steady reconnection phenomena in real cosmic environments.
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- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3389/fphy.2024.1439949
- OA Status
- gold
- References
- 71
- Related Works
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- OpenAlex ID
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Raw OpenAlex JSON
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https://openalex.org/W4402463629Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3389/fphy.2024.1439949Digital Object Identifier
- Title
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Analytical solution of steady reconnection outflows in a time-varying three-dimensional reconnection model with generalized spatiotemporal distributionsWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2024Year of publication
- Publication date
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2024-09-11Full publication date if available
- Authors
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Yuxuan Chen, Yi Wang, Fangli Wei, Xueshang Feng, Zilu Zhou, B. Y. Wang, Pingbing Zuo, Chaowei Jiang, Yaxin Gu, L. D. Wang, Xiaojian Song, Xiaojun XuList of authors in order
- Landing page
-
https://doi.org/10.3389/fphy.2024.1439949Publisher landing page
- Open access
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YesWhether a free full text is available
- OA status
-
goldOpen access status per OpenAlex
- OA URL
-
https://doi.org/10.3389/fphy.2024.1439949Direct OA link when available
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Magnetic reconnection, Physics, Mechanics, Classical mechanics, Statistical physics, Plasma, Quantum mechanicsTop concepts (fields/topics) attached by OpenAlex
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0Total citation count in OpenAlex
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71Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.real | 202 |
| abstract_inverted_index.that | 140 |
| abstract_inverted_index.this | 114 |
| abstract_inverted_index.when | 52 |
| abstract_inverted_index.These | 178 |
| abstract_inverted_index.exist | 105, 146 |
| abstract_inverted_index.flows | 61, 69, 103, 165 |
| abstract_inverted_index.hours | 86 |
| abstract_inverted_index.model | 119 |
| abstract_inverted_index.solar | 93, 176 |
| abstract_inverted_index.space | 13 |
| abstract_inverted_index.which | 95 |
| abstract_inverted_index.wind, | 94 |
| abstract_inverted_index.wind. | 177 |
| abstract_inverted_index.cosmic | 203 |
| abstract_inverted_index.energy | 7 |
| abstract_inverted_index.field. | 151 |
| abstract_inverted_index.fields | 58, 173 |
| abstract_inverted_index.model? | 112 |
| abstract_inverted_index.plasma | 17, 60 |
| abstract_inverted_index.raises | 96 |
| abstract_inverted_index.realms | 11 |
| abstract_inverted_index.steady | 101, 141 |
| abstract_inverted_index.study, | 115 |
| abstract_inverted_index.within | 147 |
| abstract_inverted_index.broaden | 180 |
| abstract_inverted_index.firstly | 138 |
| abstract_inverted_index.several | 85 |
| abstract_inverted_index.Magnetic | 0 |
| abstract_inverted_index.decades, | 23 |
| abstract_inverted_index.findings | 179 |
| abstract_inverted_index.insights | 196 |
| abstract_inverted_index.magnetic | 30, 57, 81, 110, 124, 150, 168, 172, 192 |
| abstract_inverted_index.observed | 89 |
| abstract_inverted_index.obtained | 51 |
| abstract_inverted_index.offering | 194 |
| abstract_inverted_index.outflows | 143 |
| abstract_inverted_index.physics, | 14 |
| abstract_inverted_index.physics. | 18 |
| abstract_inverted_index.remained | 33 |
| abstract_inverted_index.specific | 53 |
| abstract_inverted_index.approach, | 135 |
| abstract_inverted_index.discussed | 156 |
| abstract_inverted_index.endeavor. | 36 |
| abstract_inverted_index.evolution | 66 |
| abstract_inverted_index.existence | 161 |
| abstract_inverted_index.framework | 131 |
| abstract_inverted_index.important | 98 |
| abstract_inverted_index.kinematic | 122 |
| abstract_inverted_index.mechanism | 5 |
| abstract_inverted_index.necessary | 187 |
| abstract_inverted_index.obtaining | 24 |
| abstract_inverted_index.phenomena | 200 |
| abstract_inverted_index.provided. | 63 |
| abstract_inverted_index.question: | 99 |
| abstract_inverted_index.solutions | 26, 47 |
| abstract_inverted_index.stability | 185 |
| abstract_inverted_index.turbulent | 92, 171 |
| abstract_inverted_index.analytical | 25, 46, 118, 134 |
| abstract_inverted_index.complexity | 40 |
| abstract_inverted_index.conditions | 188 |
| abstract_inverted_index.conversion | 8 |
| abstract_inverted_index.discussed. | 78 |
| abstract_inverted_index.equations, | 45 |
| abstract_inverted_index.persisting | 83 |
| abstract_inverted_index.challenging | 35 |
| abstract_inverted_index.fundamental | 4 |
| abstract_inverted_index.generalized | 117 |
| abstract_inverted_index.possibility | 158 |
| abstract_inverted_index.analytically | 77, 155 |
| abstract_inverted_index.constructed. | 128 |
| abstract_inverted_index.demonstrated | 139 |
| abstract_inverted_index.nonlinearity | 42 |
| abstract_inverted_index.quasi-steady | 80, 163, 198 |
| abstract_inverted_index.reconnection | 1, 31, 68, 73, 82, 102, 111, 125, 142, 164, 169, 199 |
| abstract_inverted_index.time-varying | 149 |
| abstract_inverted_index.Additionally, | 79 |
| abstract_inverted_index.Particularly, | 64 |
| abstract_inverted_index.astrophysics, | 15 |
| abstract_inverted_index.distributions | 55 |
| abstract_inverted_index.environments. | 204 |
| abstract_inverted_index.reconnection, | 193 |
| abstract_inverted_index.theoretically | 104, 145 |
| abstract_inverted_index.understanding | 182 |
| abstract_inverted_index.spatiotemporal | 54 |
| abstract_inverted_index.time-dependent | 71, 108, 121, 190 |
| abstract_inverted_index.three-dimensional | 28 |
| cited_by_percentile_year | |
| countries_distinct_count | 0 |
| institutions_distinct_count | 12 |
| citation_normalized_percentile.value | 0.14300124 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | False |