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Near-Earth space is filled with energetic ions and electrons of multi-MeV energy, which can damage sensitive satellite components and harm humans in space. The energy comes from the Sun’s outbursts of plasmas, the dynamic solar wind, but it is focused and amplified in Earth’s magnetized space environment, the magnetosphere. The tug of war between the solar wind and our magnetized planet drives the dynamic auroras, Earth’s radiation belts, and affects our atmosphere. Space weather is a major field of study for space agencies around the world. Modeling and predicting radiation particle fluxes is still in its infancy. We have recently learned that like their close-kin, substorms, the large space storms are powered by magnetotail reconnection outflows. These are localized (1-2 Earth radii East-West and 1000km North-South) and thus highly elusive. They are initiated by reconnection but deposit their energy very close to Earth, near the geosynchronous region. Multi-satellite investigations are required to make progress on how these convert the tail magnetic energy to heat and how they drive field aligned currents to heat the upper atmosphere. Like our atmosphere, whose study was revolutionized by the advent of telegraphy, permitting near-real time observations of atmospheric pressure fronts, space environment is equally dynamic requiring dozens to hundreds of space buoys to first understand and then monitor space plasma interactions across multiple scales. Today this appears feasible thanks to a new generation of technologies maturing through CubeSat programs around the world. This represents a new way of conducting high-quality space science, while advancing new space technologies. It also represents a new educational model in space science and engineering, emphasizing critical thinking, responsibility and teamwork, preparing well our future explorers.