On the Importance of the Kelvin-Helmholtz Instability on Magnetospheric and Solar Wind Dynamics During High Magnetic Shear

Katariina Nykyri

doi:10.1029/2024GL108605

On the Importance of the Kelvin-Helmholtz Instability on Magnetospheric and Solar Wind Dynamics During High Magnetic Shear

NASA Goddard Space Flight Center

Research output: Contribution to journal › Comment/debate › peer-review

Original language	English
Article number	e2024GL108605
Journal	Geophysical Research Letters
Volume	51
Issue number	8
DOIs	https://doi.org/10.1029/2024GL108605
State	Published - Apr 28 2024
Externally published	Yes

ASJC Scopus Subject Areas

Geophysics
General Earth and Planetary Sciences

Keywords

Kelvin-Helmholtz instability
magnetic reconnection
plasma entry and loss

Access to Document

10.1029/2024GL108605

Cite this

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title = "On the Importance of the Kelvin-Helmholtz Instability on Magnetospheric and Solar Wind Dynamics During High Magnetic Shear",

keywords = "Kelvin-Helmholtz instability, magnetic reconnection, plasma entry and loss",

author = "Katariina Nykyri",

note = "Publisher Copyright: Published 2024. This article is a U.S. Government work and is in the public domain in the USA.",

year = "2024",

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doi = "10.1029/2024GL108605",

language = "English",

volume = "51",

journal = "Geophysical Research Letters",

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AU - Nykyri, Katariina

N1 - Publisher Copyright: Published 2024. This article is a U.S. Government work and is in the public domain in the USA.

PY - 2024/4/28

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KW - Kelvin-Helmholtz instability

KW - magnetic reconnection

KW - plasma entry and loss

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DO - 10.1029/2024GL108605

M3 - Comment/debate

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JO - Geophysical Research Letters

JF - Geophysical Research Letters

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On the Importance of the Kelvin-Helmholtz Instability on Magnetospheric and Solar Wind Dynamics During High Magnetic Shear

ASJC Scopus Subject Areas

Keywords

Access to Document

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