Abstract
The Space Plasma Environment Research Facility (SPERF) for ground simulation of the space plasma environment is a key component of the Space Environment Simulation Research Infrastructure (SESRI), a major national science and technology infrastructure for fundamental research. It is designed to investigate outstanding issues in the space plasma environment, such as energetic particle acceleration, transport, and interaction with electromagnetic waves, as well as magnetic reconnection processes, in magnetospheric plasmas. The Tail-Research EXperiment (TREX) is part of the SPERF for laboratory studies of space physics relevant to magnetic reconnection, dipolarization and hydromagnetic wave excitation in the magnetotail. SPERF-TREX is designed to carry out three types of experiments: the tail plasmoid for magnetic reconnection, dipolarization front formation, and magnetohydrodynamic waves excited by high-speed plasma jets. In this paper, the scientific goals and three scenarios of SPERF-TREX for typical processes in space plasmas are presented, and experimental plans for SPERF-TREX are also reviewed, together with the plasma sources applied to generate the plasma with the desired parameters and various magnetic configurations.
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