Member Since 1999
Katariina Nykyri
AGU Research
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On the Importance of the Kelvin‐Helmholtz Instability on Magnetospheric and Solar Wind Dynamics During High Magnetic Shear
GEOPHYSICAL RESEARCH LETTERS
14 april 2024
Katariina Nykyri
The secondary processes driven by the velocity shear driven Kelvin‐Helmholtz Instability (KHI) in the magnetized plasmas have been shown to b...
Density and Magnetic Field Asymmetric Kelvin‐Helmholtz Instability
JOURNAL OF GEOPHYSICAL RESEARCH: SPACE PHYSICS
13 march 2024
Xuanye Ma, Peter A. Delamere, Katariina Nykyri, An...
The Kelvin‐Helmholtz (KH) instability can transport mass, momentum, magnetic flux, and energy between the magnetosheath and magnetosphere, wh...
Defining the Middle Corona
FUNDAMENTAL PHYSICS OF THE SOLAR CORONA AND INNER HELIOSPHERE IV POSTER
spa-solar and heliospheric physics | 15 december 2023
Matthew J. West, Daniel B. Seaton, David Wexler, J...
The middle corona, the region roughly spanning heliocentric distances from 1.5 to 6 solar radii, encompasses almost all of the influential physical tr...
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Statistical Study of Solar Wind Current Sheet Properties as Identified by Seven Sisters Instrumentation
TURBULENCE, MAGNETIC RECONNECTION, PARTICLE ENERGIZATION, AND FUNDAMENTAL PLASMA PROCESSES IN SPACE PLASMA I POSTER
spa-solar and heliospheric physics | 14 december 2023
Yu-Lun Liou, Katariina Nykyri
The Seven Sisters mission is a multi-spacecraft solar wind mission concept dedicated for the study of the fundamental physical processes and solar win...
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Impact of Solar Wind and IMF Fluctuations on Magnetosphere Dynamics
TURBULENCE, MAGNETIC RECONNECTION, PARTICLE ENERGIZATION, AND FUNDAMENTAL PLASMA PROCESSES IN SPACE PLASMA I POSTER
spa-solar and heliospheric physics | 14 december 2023
Shiva Kavosi, Katariina Nykyri, Yu-Lun Liou, Xuany...
Solar wind (SW) is a highly structured, predominantly supermagnetosonic plasma that includes large-scale transients, meso-scale density structures, as...
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Investigation of Solar Wind Propagation Using Information Theory
TURBULENCE, MAGNETIC RECONNECTION, PARTICLE ENERGIZATION, AND FUNDAMENTAL PLASMA PROCESSES IN SPACE PLASMA I POSTER
spa-solar and heliospheric physics | 14 december 2023
Xuanye Ma, Katariina Nykyri, Simon Wing, Katherine...
Solar wind (SW) comprises various structures, including coronal mass ejections (CMEs), stream interaction regions (SIRs), and interplanetary shocks, a...
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MHD inertial range power anisotropy in the young solar wind
ENERGY TRANSFER AND DISSIPATION IN SPACE PLASMAS: KINETIC TO GLOBAL SCALES III ORAL
spa-solar and heliospheric physics | 13 december 2023
Laxman Adhikari, Gary P. Zank, Bofeng Tang, Bingbi...
Anisotropy, an important property of solar wind fluctuations, indicates that turbulence properties vary depending on the direction relative to the bac...
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Investigation of causal relationships of the cross-scale wave coupling through information theoretical approach
DAYSIDE MAGNETOSPHERE INTERACTIONS IV POSTER
spa-magnetospheric physics | 13 december 2023
Elmer Alberto Ccopa Rivera, Jay Johnson, Simon Win...
On 10-02-2015, MMS spacecraft observed an electron micro-injection event near the southern hemispheric high-altitude cusp, coinciding with intense wav...
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