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

Deep surveys with the SKA1-MID array offer for the first time the opportunityto systematically explore the polarization properties of the microJy sourcepopulation. Our knowledge of the polarized sky approaching these levels isstill very limited. In total intensity the population will be dominated bystar-forming and normal galaxies to intermediate redshifts ($z \sim1-2$), andlow-luminosity AGN to high redshift. The polarized emission from these objectsis a powerful probe of their intrinsic magnetic fields and of their magneticenvironments. For redshift of order 1 and above the broad bandwidth of themid-bands span the Faraday thick and thin regimes allowing study of theintrinsic polarization properties of these objects as well as depolarizationfrom embedded and foreground plasmas. The deep field polarization images willprovide Rotation Measures data with very high solid angle density allowing asensitive statistical analysis of the angular variation of RM on criticalarc-minute scales from a magnetic component of Large Scale Structure of theUniverse.

SKA Deep Polarization and Cosmic Magnetism