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  1. ; ; ; ; (, ACM)
    Free, publicly-accessible full text available June 29, 2027
  2. ; ; ; ; ; ; ; ; (, Advances in Neural Information Processing Systems (NeurIPS 2025))
    Free, publicly-accessible full text available December 2, 2026
  3. ; ; ; ; ; ; ; (, ACS applied materials interfaces)
    Free, publicly-accessible full text available October 29, 2026
  4. ; ; ; ; ; ; (, IEEE)
    Accepted Manuscript Full Text Available
  5. ; ; ; ; ; ; ; ; ; ; et al (, PIER)
    We present our latest development and experimental validation of carrier cooperative recovery for enhancing the resilience of optical packet transport networks. Experimental results prove that in case of resource crunch caused by, e.g., traffic congestion, failures, man-made/natural disasters, etc., swift and low-cost recovery can be achieved by exploiting the interconnection capability among carriers, which demonstrates a novel use case of multi-carrier interconnection technology. 
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    Free, publicly-accessible full text available November 5, 2026
  6. ; ; ; ; ; ; ; ; (, Conference on Language Modeling (COLM))
    Accepted Manuscript Full Text Available
  7. ; ; ; ; ; (, COLING)
    Accepted Manuscript Full Text Available
  8. ; ; ; ; ; ; ; (, Conference on Neural Information Processing Systems (NeurIPS))
    Accepted Manuscript Full Text Available
  9. ; ; ; (, IEEE International Conference on Computer Vision Workshops)
    Accepted Manuscript Full Text Available
  10. ; ; ; ; (, Geophysical Research Letters)
    Abstract The collisionless nature of planetary magnetospheres means that electromagnetic forces are fundamental in controlling the flow of energy and momentum through these systems. We use Pioneer Venus Orbiter (PVO) observations to demonstrate that the magnetic pumping process can be active at Venus, in analogy to its recent discovery at Mars. The presented case study demonstrates the framework for how the process can work at Venus, and the results of a statistical analysis show that the ambient plasma conditions support the process being active. Magnetic pumping enables low frequency magnetosonic waves to heat ambient ionospheric electrons and provides a mechanism that couples the solar wind to the Venusian ionosphere. This is the first time the magnetic pumping process has been discussed at Venus. 
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    Full Text Available