Dayside transients, such as hot flow anomalies, foreshock bubbles, magnetosheath jets, flux
transfer events, and surface waves, are frequently observed upstream from the bow shock …

Abstract The Mars Atmosphere and Volatile Evolution mission has obtained comprehensive
particle and magnetic field measurements. The Solar Wind Electron Analyzer provides …

A parallel adaptive mesh refinement (AMR) finite‐volume scheme for predicting ideal MHD
flows is used to simulate the initiation, structure, and evolution of a coronal mass ejection …

A magnetosphere is a" sphere" of influence around a planet in which the forces associated
with the magnetic field of the planet prevail over all other forces. The magnetic field of the …

We illustrate some fundamental alterations of the solar wind‐magnetosphere interaction that
occur during low Mach number solar wind. We first show that low Mach number solar wind …

The purpose of this chapter is to present a tutorial and recent advances on the Earth's inner
magnetosphere, which includes the plasmasphere, warm plasma, ring current, and radiation …

The magnetopause is the key region in space for the transfer of solar wind mass,
momentum, and energy into the magnetosphere. During the last decade, our understanding …

An understanding of the transport of solar wind plasma into and throughout the terrestrial
magnetosphere is crucial to space science and space weather. For non-active periods, there …

The global BATS‐R‐US MHD code is used to simulate the interaction of a moderately strong
interplanetary shock with the Earth's magnetosphere. The model predicts the propagation of …

Relativistic electron precipitation (REP) into the Earth's atmosphere is one of the
fundamental mechanisms causing radiation belt electron flux dropout. It is important to know …