Using CODE V to model adaptive optics

Using connected-element interferometer phase-delay data for Magellan navigation in Venus orbit

Using constraint programming to resolve the multi-source/multi-site data movement paradigm on the Grid

Using eclipse observations to search large-scale velocity field in the range 2-4Rsolar.

Using Euler buckling springs for vibration isolation

Using KD*P modulators to measure the Stokes vector on the Sun.

Using notch filter masks for high-contrast imaging of extra solar planets

Using raw star signals in the monitoring of GOES imager visible-channel responsivities

Using Science-Fiction to Teach General Education Astronomy

Using solar wind low-energy energetic ion enhancements to forecast large geomagnetic storms

Using the radial basis function neural network to predict ionospheric critical frequency of F2 layer over Wuhan

Using the shield for thermal energy storage in PULSAR

Using the VERITAS Experiment to Study the Performance of Imaging Atmospheric Cherenkov Telescope Experiments as Function of Design Parameters

Using today's Strategic Defense Initiative (SDI) technologies to accomplish tomorrow's low cost space missions

Utilizing Fractionated Space Mission Design and Small Satellites for a Next Generation Gamma Ray Burst Observatory

UV detectors aboard SOHO

UV Imaging Detectors: High-QE EBCMOS Enabling New Science Missions

UV Imaging of Extensive Air Showers at Tev Energies

UV photolysis of quinoline in interstellar ice analogs

UV Scanner DOAS Data Retrieved Using A Modelled Reference Spectrum