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 …

The magnetosheath flow may take the form of large amplitude, yet spatially localized,
transient increases in dynamic pressure, known as “magnetosheath jets” or “plasmoids” …

Abstract The Time History of Events and Macroscale Interactions during Substorms
(THEMIS) mission is the fifth NASA Medium-class Explorer (MIDEX), launched on February …

We present a new method for determining the shape of the magnetopause as a bivariate
function of the hourly averaged solar wind dynamic pressure (p) and the north‐south …

Three‐component dynamic spectrograms (0–80 mHz) of AMPTE/CCE magnetic field data
from August 24, 1984, through December 7, 1985, have been used to survey ULF pulsation …

Brief, impulsive, large‐amplitude (δp/p∼ 1) solar wind dynamic pressure pulses, recurring
on time scales of 5 to 15 min, are common just upstream of the Earth's bow shock. When …

We present a comprehensive observational study of the magnetospheric response to an
interplanetary magnetic field (IMF) tangential discontinuity, which first struck the postnoon …

Magnetic field enhancements and depressions on the time scales of minutes were
frequently observed simultaneously by the AMPTE CCE, GOES 5, and GOES 6 spacecraft in …

The downstream region of a collisionless quasiparallel shock is structured containing bulk
flows with high kinetic energy density from a previously unidentified source. We present …

On 3 July 2001, the four Cluster satellites traversed along the dawnside magnetospheric
flank and observed large variations in all plasma parameters. The estimated magnetopause …