Academic Journal
Recent advances in magnetic reconnection in Mars' space environment.
| Τίτλος: | Recent advances in magnetic reconnection in Mars' space environment. |
|---|---|
| Συγγραφείς: | Lin, Rentong1,2 (AUTHOR) rentonglin@ustc.edu.cn, Huang, Shiyong3 (AUTHOR), Jiang, Kui3 (AUTHOR), Xiong, Qiyang3 (AUTHOR), Wang, Yuming1,2 (AUTHOR) |
| Πηγή: | Discover Space. 8/20/2026, Vol. 130 Issue 1, p1-29. 29p. |
| Θεματικοί όροι: | *Magnetic reconnection, *Magnetosphere, *Plasma heating, *Solar wind, *Atmospheric ionization, *Auroras, *Magnetic anomalies, *Martian atmosphere |
| Περίληψη: | Magnetic reconnection has recently emerged as an important process in the Martian space environment. In contrast to Earth, Mars lacks a global intrinsic dipole field and possesses an induced magnetosphere shaped by solar-wind interaction with the ionosphere, localized crustal magnetic anomalies, and abundant planetary heavy ions. Recent measurements from Mars Global Surveyor, Mars Express, MAVEN, and Tianwen-1 have revealed reconnection signatures in several distinct regions, including the dayside induced magnetosphere, the induced magnetotail, the crustal-field mini-magnetospheres, and the upper ionosphere. These reconnection signatures include Hall-like magnetic perturbations, multi-species ion outflows, magnetic flux ropes, reconnection fronts, and electron pitch-angle changes indicative of magnetic topology reconfiguration. This review synthesizes recent observational and theoretical progress on Martian magnetic reconnection and discusses its implications for magnetospheric structure, plasma energization, auroral activity, and atmospheric ion escape. Particular attention is given to the effects of interplanetary magnetic field variability, heavy-ion composition, and ionospheric collisionality, which distinguish reconnection at Mars from more familiar terrestrial cases. Although existing observations show that reconnection is a recurrent and potentially important component of Mars–solar-wind coupling, its global occurrence rate, spatial extent, and long-term atmospheric impact remain poorly constrained. Future coordinated multi-spacecraft measurements and multi-scale simulations will be critical for linking local reconnection physics to global plasma transport and atmospheric evolution. [ABSTRACT FROM AUTHOR] |
| Βάση Δεδομένων: | Academic Search Index |
| FullText | Text: Availability: 0 CustomLinks: – Url: https://dx.doi.org/doi:10.1007/s11038-026-09597-z Name: EDS - Springer Nature Journals (s7799221) Category: fullText Text: View record at Springer – Url: https://resolver.ebsco.com/c/fiv2js/result?sid=EBSCO:asx&genre=article&issn=29482941&ISBN=&volume=130&issue=1&date=20260820&spage=1&pages=1-29&title=Discover Space&atitle=Recent%20advances%20in%20magnetic%20reconnection%20in%20Mars%27%20space%20environment.&aulast=Lin%2C%20Rentong&id=DOI:10.1007/s11038-026-09597-z Name: Full Text Finder (for New FTF UI) (ns324271) Category: fullText Text: Full Text Finder MouseOverText: Full Text Finder |
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| Header | DbId: asx DbLabel: Academic Search Index An: 196364885 RelevancyScore: 1452 AccessLevel: 6 PubType: Academic Journal PubTypeId: academicJournal PreciseRelevancyScore: 1452.42517089844 |
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| Items | – Name: Title Label: Title Group: Ti Data: Recent advances in magnetic reconnection in Mars' space environment. – Name: Author Label: Authors Group: Au Data: <searchLink fieldCode="AR" term="%22Lin%2C+Rentong%22">Lin, Rentong</searchLink><relatesTo>1,2</relatesTo> (AUTHOR)<i> rentonglin@ustc.edu.cn</i><br /><searchLink fieldCode="AR" term="%22Huang%2C+Shiyong%22">Huang, Shiyong</searchLink><relatesTo>3</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Jiang%2C+Kui%22">Jiang, Kui</searchLink><relatesTo>3</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Xiong%2C+Qiyang%22">Xiong, Qiyang</searchLink><relatesTo>3</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Wang%2C+Yuming%22">Wang, Yuming</searchLink><relatesTo>1,2</relatesTo> (AUTHOR) – Name: TitleSource Label: Source Group: Src Data: <searchLink fieldCode="JN" term="%22Discover+Space%22">Discover Space</searchLink>. 8/20/2026, Vol. 130 Issue 1, p1-29. 29p. – Name: Subject Label: Subject Terms Group: Su Data: *<searchLink fieldCode="DE" term="%22Magnetic+reconnection%22">Magnetic reconnection</searchLink><br />*<searchLink fieldCode="DE" term="%22Magnetosphere%22">Magnetosphere</searchLink><br />*<searchLink fieldCode="DE" term="%22Plasma+heating%22">Plasma heating</searchLink><br />*<searchLink fieldCode="DE" term="%22Solar+wind%22">Solar wind</searchLink><br />*<searchLink fieldCode="DE" term="%22Atmospheric+ionization%22">Atmospheric ionization</searchLink><br />*<searchLink fieldCode="DE" term="%22Auroras%22">Auroras</searchLink><br />*<searchLink fieldCode="DE" term="%22Magnetic+anomalies%22">Magnetic anomalies</searchLink><br />*<searchLink fieldCode="DE" term="%22Martian+atmosphere%22">Martian atmosphere</searchLink> – Name: Abstract Label: Abstract Group: Ab Data: Magnetic reconnection has recently emerged as an important process in the Martian space environment. In contrast to Earth, Mars lacks a global intrinsic dipole field and possesses an induced magnetosphere shaped by solar-wind interaction with the ionosphere, localized crustal magnetic anomalies, and abundant planetary heavy ions. Recent measurements from Mars Global Surveyor, Mars Express, MAVEN, and Tianwen-1 have revealed reconnection signatures in several distinct regions, including the dayside induced magnetosphere, the induced magnetotail, the crustal-field mini-magnetospheres, and the upper ionosphere. These reconnection signatures include Hall-like magnetic perturbations, multi-species ion outflows, magnetic flux ropes, reconnection fronts, and electron pitch-angle changes indicative of magnetic topology reconfiguration. This review synthesizes recent observational and theoretical progress on Martian magnetic reconnection and discusses its implications for magnetospheric structure, plasma energization, auroral activity, and atmospheric ion escape. Particular attention is given to the effects of interplanetary magnetic field variability, heavy-ion composition, and ionospheric collisionality, which distinguish reconnection at Mars from more familiar terrestrial cases. Although existing observations show that reconnection is a recurrent and potentially important component of Mars–solar-wind coupling, its global occurrence rate, spatial extent, and long-term atmospheric impact remain poorly constrained. Future coordinated multi-spacecraft measurements and multi-scale simulations will be critical for linking local reconnection physics to global plasma transport and atmospheric evolution. [ABSTRACT FROM AUTHOR] |
| PLink | https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&db=asx&AN=196364885 |
| RecordInfo | BibRecord: BibEntity: Identifiers: – Type: doi Value: 10.1007/s11038-026-09597-z Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 29 StartPage: 1 Subjects: – SubjectFull: Magnetic reconnection Type: general – SubjectFull: Magnetosphere Type: general – SubjectFull: Plasma heating Type: general – SubjectFull: Solar wind Type: general – SubjectFull: Atmospheric ionization Type: general – SubjectFull: Auroras Type: general – SubjectFull: Magnetic anomalies Type: general – SubjectFull: Martian atmosphere Type: general Titles: – TitleFull: Recent advances in magnetic reconnection in Mars' space environment. Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: Lin, Rentong – PersonEntity: Name: NameFull: Huang, Shiyong – PersonEntity: Name: NameFull: Jiang, Kui – PersonEntity: Name: NameFull: Xiong, Qiyang – PersonEntity: Name: NameFull: Wang, Yuming IsPartOfRelationships: – BibEntity: Dates: – D: 20 M: 08 Text: 8/20/2026 Type: published Y: 2026 Identifiers: – Type: issn-print Value: 29482941 Numbering: – Type: volume Value: 130 – Type: issue Value: 1 Titles: – TitleFull: Discover Space Type: main |
| ResultId | 1 |