Portable Field Emission Spectrometer (PFES) data were acquired on July 15 and 17, 1989. A total of 31 measurements were collected for GRSFE. Of these measurements, 13 were calibrations and 18 were of representative surfaces. The data were collected primarily to support the calibration of the TIMS data and to assist in interpreting spectral mixing in the mid-infrared. Sites were selected for calibration that covered a range of emissivities. On July 15, PFES data were collected at Kelso Dunes and the Cima Volcanic Field as part of the Calibration Team effort. Daedalus and SIRIS data were collected over the same sites. For the PFES data, the Kelso Dunes Bright Target site represented the silica-rich endmember and the Cima basalt tephra Dark Target site represented the more silica-poor endmember. On July 17, PFES data were collected at two of the modelling sites at Lunar Lake (the playa and the cobble sites). Several spectra were also collected at the playa surface next to the Lunar Lake thermistor site.

Published colors of Trans-Neptunian objects through December 2001

This data set contains Raw data taken by the New Horizons Linear Etalon Imaging Spectral Array instrument during the post-launch checkout mission phase.

The Ames Mars General Circulation Model is a three dimensional model based on the primitive equations of meteorology. It includes the radiative effects of dust and carbon dioxide as well as other features such as large-scale topography (see [POLLACKETAL1990]

TBD

The High Rate Detector (HRD) from the University of Chicago is an independent part of the CDA instrument on the Cassini Orbiter that measures the dust flux and particle mass distribution of dust particles hitting the HRD detectors. This data set includes all data from the HRD through December 31, 2014. Please refer to Srama et al. (2004) for a detailed HRD description.

This volume contains the CRISM Map-projected Targeted Reduced Data Record (MTRDR) archive, a collection of multiband image cubes derived from targeted (gimbaled) observations of Mars' surface acquired by the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) instrument on the Mars Reconnaissance Orbiter (MRO) spacecraft. Post-processing attempts to represent the spectrum the instrument would have measured looking at the surface of Mars at a standard illumination geometry, in the absence of atmospheric gases, with aerosol scattering normalized to that at the geometry within the observation that is closest to nadir, in the absence of instrument artifacts. A series of value added products represent spatial variability in signatures of minerals of interest. The data are map projected using terrain models of the Martian surface. A companion Targeted Empirical Record (TER) archive contains mostly the same data in the sensor space of the IR detector to support map projection using future more accurate terrain models.

This collection of asteroid masses and densities was compiled from the published literature by Jim Baer, Steve Chesley, and Dan Britt. This is the version of the compilation as of January 7, 2009.

This data set contains CODMAC level 3 calibration, and instrument checkout data acquired by the Rosetta Orbiter ALICE UV Spectrometer during the second commissioning phase of the Rosetta mission

This data set contains raw calibration and test images acquired by the Deep Impact Impactor Targeting Sensor Visible CCD during the cruise phase of the mission. These observations were used for optical and autonomous navigation (NAV) of the impactor spacecraft. These data were collected from 7 April to 30 April 2005. The comet was not imaged during cruise.