TITLE:
A study of Kelvin-Helmholtz instability in solar partially ionised magnetised jets

AUTHOR:
S. Lomineishvili, AI SAS

ABSTRACT:
Kelvin-Helmholtz Instability (KHI) in solar, partially ionised, magnetised jets is studied. The jets are
modelled as two magnetic slabs in a relative motion at an arbitrary angle. Using MHD equations of par-
tially ionised plasmas, an analytical dispersion relation is obtained, which further is solved analytically
and numerically for various settings pertaining to the solar chromospheric jets and prominences. The rela-
tive importance of partial ionisation and perpendicular magnetic field component on the onset and growth
rate of KHI is quantified and discussed.