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Laboratory Data
The Geosciences Node archives
laboratory-based data sets that have relevance to
planetary studies.
The
Apollo Soil Reflectance Data Set consists
of bidirectional reflectance distribution function
measurements of Apollo samples at several wavelengths,
acquired by the Bloomsburg University Goniometer (BUG)
(Michael Shepard, Bloomsburg University).
The
Mars Analog Soil BUG observations
are bidirectional reflectance distribution
function (BRDF) measurements of Mars soil
analogs acquired by the Bloomsburg
University Goniometer (BUG) (Michael
Shepard, Bloomsburg University).
The
Mars Analog
Handlens-Scale Image Data Base
is a collection of images and measurements
of potential martian analog features and
materials taken at 10 micrometers per pixel,
approximately the scale of a geologist's
handlens (Aileen Yingst, Planetary Science
Institute).
The
Laboratory Shocked Feldspars bundle
consists of data acquired from thin sections
created from a suite of experimentally
shocked plagioclase feldspars, and a basalt
and basaltic andesite (Jeff Johnson, JHU
Applied Physics Laboratory).
The
Complex
Refractive Indices of Carbonates bundle
consists of estimates of the visible to
mid-infrared (VMIR, ~0.3-6 micrometer)
complex refractive indices of the carbonates
calcite, dolomite, and magnesite (Ted Roush,
NASA Ames Research Center).
The
Astromaterials Database bundle
is a compendium of published geochemical
data on astromaterials analyzed in
terrestrial laboratories (Kerstin Lehnert,
Columbia University).
The
Ronald Greeley 35mm Slide Collection
consists of slides digitized to preserve the
research materials of Dr. Ronald Greeley,
who played a critical role in the planetary
missions to the planets of the inner and
outer Solar System (David Williams, Arizona
State University).
The
Lunar Simulants JSC-1A and LMS-1
Far-ultraviolet Reflectance Bundle
contains all of the data presented in the
paper "Far-Ultraviolet Photometric
Characteristics of JSC-1A and LMS-1 Lunar
Regolith Simulants: Comparative
Investigations With Apollo 10084," as
published in Volume 127, Issue 11, of the
Journal of Geophysical Research: Planets,
doi:10.1029/2022JE007508 (Caleb Gimar,
University of Texas at San Antonio).
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