Use of satellite observations for the study of mesoscale systems in polar regions

Use of satellite soundings in monitoring mesoscale precipitation systems

Use of satellite, surface, and aerological information for the calculation of thermal radiation fluxes

Use of the backscatter method for studying ionization inhomogeneities and their motions in the ionospheric D region

Using complex independent component analysis to extract weak returns in MARSIS radar data and their possible relation to a subsurface reflector on Mars

Using energetic electrons to probe the topology of the October 18-20, 1995 magnetic cloud

Using fluctuations of Entropy as a starting point for obtaining behavior of scalar fields permitting collapse of thin wall approximation

Using lunar sounder imagery to distinguish surface from subsurface reflectors in lunar highlands areas

Using Mimicry to Learn about Mental Representations

Using SHARAD radar soundings to evaluate the origin of martian gullies and pingos

Using Solar Ultraviolet Irradiance Modeling Techniques to Understand and Correct for Ultraviolet Instrument Degradation

Using speed of sound measurements to constrain the Huygens probe descent profile

Using TEM for sounding conductive and deep groundwater in Mars analog environments: Comparing two field studies

Using the International Monitoring System infrasound network to study gravity waves

Using the Transient Electromagnetic (TEM) Method for Mapping Deep Groundwater Tables in Mars Analog Environments: a Baseline Field Study.

Using the Very Large Array (VLA) and other radio telescopes to perform a parasitic search for extraterrestrial intelligence (SETI)

Using the Very Long Baseline Array

Using X-ray Occultation Sounding (XOS) to Detect Atmospheric Features in the Upper Mesosphere and Lower Thermosphere: A comparison to NRLMSISE-00 and SABER measurements.

Using X-ray Occultation Sounding (XOS) to Detect Atmospheric Features in the Upper Mesosphere and Lower Thermosphere: A comparison to NRLMSISE-00 and SABER measurements.

Using X-ray Occultation Sounding to Detect Dynamic Atmospheric Features in the Upper Mesosphere and Lower Thermosphere