Conditions for the Kelvin‐Helmholtz Instability in the Polar Ionosphere

Abstract The Kelvin‐Helmholtz instability can be excited by a velocity shear in a fluid. Inhomogeneous flows are frequently observed in regions with polar cap patches, reversed flow events and auroral arcs, that is, regions with irregularities that disturb navigation satellite signals. Understanding...

Бүрэн тодорхойлолт

Номзүйн дэлгэрэнгүй

Үндсэн зохиолчид:	Andreas Kvammen, Andres Spicher, Matthew Zettergren, Devin Huyghebaert, Theresa Rexer, Björn Gustavsson, Juha Vierinen
Формат:	Artigo
Хэл сонгох:	Inglês
Хэвлэсэн:	Wiley 2025-03-01
Цуврал:	Geophysical Research Letters
Нөхцлүүд:	Kelvin‐Helmholtz instability plasma fluid simulation ionospheric flow shear ionospheric turbulence irregularity formation non‐linear instability evolution
Онлайн хандалт:	https://doi.org/10.1029/2025GL114621
Шошгууд:	Шошго нэмэх Шошго байхгүй, Энэхүү баримтыг шошголох эхний хүн болох!