The solar-wind magnetosphere interaction primarily occurs at altitudes where the dipole
component of Earth's magnetic field is dominating. The disturbances that are created in this …

An important question that is being increasingly studied across subdisciplines of
Heliophysics is “how do mesoscale phenomena contribute to the global response of the …

The Wind spacecraft, launched on November 1, 1994, is a critical element in NASA's
Heliophysics System Observatory (HSO)—a fleet of spacecraft created to understand the …

This paper addresses the question of the contribution of azimuthally localized flow channels
and magnetic field dipolarizations embedded in them in the global dipolarization of the inner …

Jupiter's bright persistent polar aurora and Earth's dark polar region indicate that the planets'
magnetospheric topologies are very different. High-resolution global simulations show that …

A high‐resolution global magnetohydrodynamic simulation is conducted with the Lyon‐
Fedder‐Mobarry (LFM) model for idealized solar wind conditions. Within the simulation …

We present an angle-resolved photoemission study of the electronic structure of the three-
dimensional pyrochlore iridate Nd 2 Ir 2 O 7 through its magnetic metal-insulator transition …

The Earth's magnetosphere is the outermost layer of the geospace system deflecting
energetic charged particles from the Sun and solar wind. The solar wind has major impacts …

Abstract Using 3‐D particle‐in‐cell simulations, we study magnetic reconnection with the X‐
line being spatially confined in the current direction. We include thick current layers to …

It is well‐known that solar eclipses can significantly impact the ionosphere and
thermosphere, but how an eclipse influences the magnetosphere‐ionosphere system is still …