M. L. Kaiser

TL;DR: The twin STEREO spacecraft were launched on October 26, 2006, at 00:52 UT from Kennedy Space Center aboard a Delta 7925 launch vehicle to understand the causes and mechanisms of coronal mass ejection (CME) initiation and follow the propagation of CMEs through the inner heliosphere to Earth as mentioned in this paper.

TL;DR: The WAVES investigation on the WIND spacecraft will provide comprehensive measurements of the radio and plasma wave phenomena which occur in Geospace as mentioned in this paper, in coordination with the other onboard plasma, energetic particles, and field measurements will help us understand the kinetic processes that are important in the solar wind and in key boundary regions of the Geospace.

TL;DR: The Cassini radio and plasma wave investigation is designed to study radio emissions, plasma waves, thermal plasma, and dust in the vicinity of Saturn as mentioned in this paper, which is the only spacecraft that can perform radio and plasmas measurements.

TL;DR: In this article, an empirical model was proposed to predict the arrival of CMEs at 1 AU, based on the relation between the acceleration and initial speed of the CME.

TL;DR: The STEREO/WAVES instrument as discussed by the authors was designed to measure the three components of the fluctuating electric field from a fraction of a hertz up to 16 MHz, plus a single frequency channel near 30 MHz.