Laboratory measurements of scattering matrix elements of randomly oriented Mars analog palagonite particles.
Laboratory measurements of the Ka-band (7.5 mm to 9.2 mm) opacity of phosphine (PH3) and ammonia (NH3) under simulated conditions for the Cassini-Saturn encounter
Laboratory measurements of the microwave opacity and vapor pressure of sulfuric acid vapor under simulated conditions for the middle atmosphere of Venus
Laboratory measurements of the microwave properties of H2S under simulated Jovian conditions with an application to Neptune
Laboratory measurements of the solar reemission factor G1.0 of the NO-gamma band at 2147 A for the determination of the density of nitric oxide in the D-region of the ionosphere
Laboratory Measurements of the Sound Generated by Breaking Waves.
Laboratory Measurements of Tortuosity and Permeability in Mars Analog Soils
Laboratory Measurements on Charging of Individual Micron-Size Apollo-11 Dust Grains by Secondary Electron Emission
Laboratory measurements on molecules of astrophysical interest
Laboratory modeling of pulsed regimes of electron cyclotron instabilities in a mirror confined plasma produced by ECR discharge
Laboratory modeling of the interaction of the solar wind with the moon
Laboratory Observation of Mass-Independent Oxygen Isotopic Composition in Solid Silicates Through Gas Phase Reaction: Cosmochemical Implications
Laboratory polarimeter for measuring the Stokes vector of light scattered from surfaces
Laboratory reflection spectra for the determination of chemical composition of ice bodies
Laboratory Research
Laboratory Results in High Contrast Imaging with the Shaped Pupil Coronagraph
Laboratory Shock Emplacement of Nitrogen and Noble Gases Into Basalt
Laboratory shock emplacement of noble gases, nitrogen, and carbon dioxide into basalt, and implications for trapped gases in shergottite EETA 79001
Laboratory simulation experiments on the solid-state greenhouse effect in planetary ices
Laboratory simulation improvements for hypervelocity micrometeorite impacts with a new dust particle source