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

Multiple properties of the solar wind that affect the earth are summarized in this overview. 13
specific solar-wind parameters that influence geomagnetic activity, the plasma sheet, the …

Abstract Using Magnetospheric Multiscale (MMS) data, we find, classify, and analyze
transient dynamic pressure enhancements in the magnetosheath (jets) from May 2015 to …

We present multipoint Time History of Events and Macroscale Interactions during Substorms
(THEMIS) observations of transient dynamic pressure pulses in the magnetosheath 3–10 …

Introduction: For the last several decades, continuous monitoring of the solar wind has been
carried out by spacecraft at the first Earth-Sun Lagrange point (L1). Due to computational …

We have developed neural network models that predict Kp from upstream solar wind data.
We study the importance of various input parameters, starting with the magnetic component …

To assess the effect of uncertainties in solar wind driving on the predictions from the
operational configuration of the Space Weather Modeling Framework, we have developed a …

Mode coupling is an important mechanism to excite Alfvén waves and has been extensively
investigated based on numerical simulations. However, no direct observational evidence …

The OMNI database is formed by propagating the solar wind measured at around Lagrange
point L1, whose result may differ from the actual solar wind in the vicinity of the bow shock …

We investigate the lagged correlation between a selection of geomagnetic indices and solar
wind parameters for a complete solar cycle, from 2000 to 2011. We first discuss the …