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

Many phenomena seen in solar atmosphere are connected with underphotosphericprocesses. MHD oscillation and other dynamical processes observed in quit sunobjects are, for example, these phenomena. In our research we use Stereo BehindEUV(171\AA and 304\AA ) observations to study dynamical processes in quiet Sunregions. We found an eruption event in a coronal bright point on the border ofa small coronal hole close to the center of the Solar disk. Several oscillatingloops became visible inside of the hole after the eruption. We suppose thatthese loops oscillation were induced by the eruption process in coronal brightpoint. The nature of interaction transfer agent is unclear because anypropagating disturbance was not detected. For data processing we used Pixelizewavelet filtration (PWF method) and Time-distance plots. We measured thesupposed interaction transfer speed and found it about 2-3 km/s. We tried tofind out the nature of the interaction transfer agent.

Induced MHD oscillations of fine loop structures located in coronal hole