Each Focused Science Team Research abstract can be found here under NNH211ZDA001N, "Understanding the Large-Scale Evolution of the Solar Wind".
This FST primarily addresses two Key Science Goals of the 2013 Decadal Survey: #1 “Determine the origins of the Sun’s activity and predict the variations in the space environment,” and #3 “Determine the interaction of the Sun with the solar system and the interstellar medium.” In addition, it supports several LWS Strategic Science Areas including SSA-I (Origins and Variability of Global Solar Processes), SSA-II (Solar Eruptive and Transient Heliospheric Phenomena), and SSA-III (Acceleration and Transport of Solar Energetic Particles.
The main goals of this FST are to understand (1) the physical processes driving the formation and propagation of solar-wind structures throughout the heliosphere and their variability with the solar cycle and (2) how the solar magnetic field and coronal structure determine the plasma and magnetic-field conditions in the inner heliosphere throughout the solar cycle.
There are a large number of physical processes acting under a variety of conditions, with varying drivers and their associated large time lags. Consequently, a more holistic approach will be necessary to gain an understanding of the heliosphere as a system. Types of investigations include but are not limited to:
In order to improve the usefulness of the results from this FST, all investigations in this FST must consider data and model uncertainty and how sources of error impact the results.