English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

In this work linear stability analysis of a magnetized dusty plasma with ananisotropic dust component having transversal motions much stronger thanmotions parallel to the external magnetic field, and isotropic light plasmacomponents is described. Such a situation presumably establishes in a shockcompressed space dusty plasma downstream the shock front. Oblique low-frequencymagneto-hydrodynamic waves ($\omega\ll \omega_{cd}$, $\omega_{cd}$ being thedust cyclotron frequency) are shown to be undergone to the mirror instability.Consequences for nonthermal dust destruction behind shock fronts in theinterstellar medium are discussed.

Mirror instability in a plasma with cold gyrating dust particles