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 Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We analyze the Sun's shadow observed with the Tibet-III air shower array andfind that the shadow's center deviates northward (southward) from the opticalsolar disc center in the "Away" ("Toward") IMF sector. By comparing withnumerical simulations based on the solar magnetic field model, we find that theaverage IMF strength in the "Away" ("Toward") sector is $1.54 \pm 0.21_{\rmstat} \pm 0.20_{\rm syst}$ ($1.62 \pm 0.15_{\rm stat} \pm 0.22_{\rm syst}$)times larger than the model prediction. These demonstrate that the observedSun's shadow is a useful tool for the quantitative evaluation of the averagesolar magnetic field.

Evaluation of the Interplanetary Magnetic Field Strength Using the Cosmic-Ray Shadow of the Sun