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Colorado Student Space Weather Experiment : ウィキペディア英語版 | Colorado Student Space Weather Experiment
Colorado Student Space Weather Experiment (CSSWE) was the sixth National Science Foundation sponsored CubeSat mission.〔(NSF Award Details )〕〔(University of Colorado Press Release )〕 It was built by students at the University of Colorado at Boulder with advising from professionals at the Laboratory for Atmospheric and Space Physics. The CSSWE mission was a joint effort by the University of Colorado's Department of Aerospace Engineering Sciences and Laboratory for Atmospheric and Space Physics. The mission principal investigator was Profs. Xinlin Li, and the Co-PIs are Prof. Scott Palo and Dr. Shri Kanekal. The project manager for the project was Dr. Lauren Blum, the system engineer was Dr. David Gerhardt, and the instrument scientist was Dr. Quintin Schiller. 〔http://www.colorado.edu/news/releases/2012/08/01/tiny-cu-boulder-satellite-may-launch-early-aug-14〕 CSSWE launched on September 13, 2012, on an Atlas V rocket by the United Launch Alliance on ELaNa-VI as part of the NASA's CubeSat Launch Initiative (CSLI).〔(ULA NROL-36 Launch Highlights )〕 The CSSWE team released its science products to the public for download on NASA's Coordinated Data Analysis Web Site (CDAWeb). As of December 22, 2014, CSSWE showed severe battery degradation, likely due to pushing the battery thousands of cycles beyond the battery's design specs. As a result, CSSWE cannot retain enough power to receive or transmit data. ==Mission Objective==
CSSWE's mission objective is to study space weather from a near-Earth orbit (480 km x 780 km).〔Li, X., S. Palo, R. Kohnert, L. Blum, D. Gerhardt, Q. Schiller, and S. Califf (2013), Small mission accomplished by students - big impact on space weather research, ''Space Weather'', Accepted, DOI: 10.1002/swe.20025〕 Specifically, CSSWE works in conjunction with concurrent missions (such as the Van Allen Probes, BARREL, and SAMPEX) to address the following questions: 1) How does solar flare location, magnitude, and frequency elate to the timing, duration, and energy spectrum of solar energetic particles (SEPs) reaching Earth and 2) How the spectrum and dynamics of Earth's radiation belt electrons evolve.〔Li, X., S. Palo, and R. Kohnert (2011), Small Space Weather Research Mission Designed Fully by Students, ''Space Weather'', 9, S04006, doi:10.1029/2011SW000668〕
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