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|a 10.1029/2021GL093029
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|a eng
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|a Chen, Li-Jen
|e verfasserin
|4 aut
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|a Magnetopause Reconnection and Indents Induced by Foreshock Turbulence
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|c 2021
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|a Text
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|a ƒaComputermedien
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|a ƒa Online-Ressource
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|a Date Revised 02.04.2024
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|a published: Print-Electronic
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|a Citation Status PubMed-not-MEDLINE
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|a © 2021. The Authors. Geophysical Research Letters published by Wiley Periodicals LLC on behalf of American Geophysical Union.
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|a Based on global hybrid simulation results, we predict that foreshock turbulence can reach the magnetopause and lead to reconnection as well as Earth-sized indents. Both the interplanetary magnetic field (IMF) and solar wind are constant in our simulation, and hence, all dynamics are generated by foreshock instabilities. The IMF in the simulation is mostly Sun-Earth aligned with a weak northward and zero dawn-dusk component, such that subsolar magnetopause reconnection is not expected without foreshock turbulence modifying the magnetosheath fields. We show a reconnection example to illustrate that the turbulence can create large magnetic shear angles across the magnetopause to induce local bursty reconnection. Magnetopause reconnection and indents developed from the impact of foreshock turbulence can potentially contribute to dayside loss of planetary plasmas
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|a Journal Article
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|a collisionless shocks
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| 650 |
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|a foreshock turbulence
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| 650 |
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4 |
|a ion escape
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| 650 |
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|a magnetopause reconnection
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| 650 |
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|a magnetosheath
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| 650 |
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|a planetary magnetospheres
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| 700 |
1 |
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|a Ng, Jonathan
|e verfasserin
|4 aut
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| 700 |
1 |
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|a Omelchenko, Yuri
|e verfasserin
|4 aut
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| 700 |
1 |
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|a Wang, Shan
|e verfasserin
|4 aut
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| 773 |
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|i Enthalten in
|t Geophysical research letters
|d 1984
|g 48(2021), 11 vom: 16. Juni, Seite e2021GL093029
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|x 0094-8276
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| 773 |
1 |
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|g volume:48
|g year:2021
|g number:11
|g day:16
|g month:06
|g pages:e2021GL093029
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|u http://dx.doi.org/10.1029/2021GL093029
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