This contract task will mature several NASA descent and landing sensors and conduct flight tests in a relevant environment. Blue Origin, along with its NASA and JPL partners, proposes to mature critical technologies that enable precision and soft landing on the Moon. We will mature several current NASA sensors and conduct flight tests in a relevant environment. Testing will be performed at approximately 100 km altitude on-board our flight proven New Shepard vertical takeoff vertical landing (VTVL) suborbital vehicle. This proposal will allow the country to eventually meet ambitious lunar objectives, enable economic development, and support U.S. strategic leadership in space.

This dataset contains the list of all publicly published NASA projects from within the NASA technology portfolio. In-depth portfolio information, including details for each of the NASA projects found here, can be found and searched at TechPort.NASA.gov.

A test dataset for Socrata help ticket

A test dataset for Socrata help ticket

A test dataset for Socrata help ticket

These data were used to create Fig. 1 of “Monte Carlo Evaluation of the Europa Clipper TID Margin based on the Variability of the Jovian Radiation Environment with Application for Mission Design” by Allen Andersen, Wousik Kim, Steven McClure, and Insoo Jun of the Jet Propulsion Laboratory, California Institute of Technology.

This data set contains Galileo Energetic Particle Detector (EPD) average counts per second measurements of 3.2-10.1 MeV protons (B0), 1.5-10.5 MeV electrons (B1), and >11 MeV electrons (DC3) between 8-10 Jovian Radii (Rj) only. Each entry has a corresponding time stamp and orbit name. Further details regarding these data can be found in

Jun, I., Garrett, H. B., Swimm, R., Evans, R. W., and Clough, G. (2005), Statistics of the variations of the high-energy electron population between 7 and 28 jovian radii as measured by the Galileo spacecraft, Icarus, 178(2), 386-394. https://doi.org/10.1016/j.icarus.2005.01.022

The research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.

X-ray micro-tomography (micro-CT) is a non-destructive imaging technique that provides resolution of material microstructures in three dimensions at scales from hundreds of nanometers to centimeters. The technique is used at NASA Ames Research Center to investigate a variety of advanced materials, including lightweight composite heatshields for atmospheric entry, woven materials, parachute textiles and meteoroids. Data are collected using both synchrotron and laboratory-based X-ray sources. Synchrotron micro-CT is performed in collaboration with the beamline 8.3.2 at the Advanced Light Source at Lawrence Berkeley National Laboratory. High-fidelity digital representations of microstructures obtained from micro-CT are used as framework to perform predictive simulations of effective material properties and material response using high performance computing.

This entry does not contain data itself, it is for the website, the NASA Disasters Mapping Portal: https://maps.disasters.nasa.gov

The Disasters Mapping Portal contains numerous datasets that can be streamed from the Portal into GIS software.

The Disasters Applications area promotes the use of Earth observations to improve prediction of, preparation for, response to, and recovery from natural and technological disasters. Disaster applications and applied research on natural hazards support emergency mitigation approaches, such as early warning systems, and providing information and maps to disaster response and recovery teams.

NOTE: Removed "2017 - Present" from "Temporal Applicability" since it's not valid
NOTE: Removed "Event-Specific and Near-Real Time Products" from "Update Frequency" since it's not valid

Companies that visited the NASA boot at the SxSW 2016 conference.

The Global Landslide Catalog (GLC) was developed with the goal of identifying rainfall-triggered landslide events around the world, regardless of size, impacts or location. The GLC considers all types of mass movements triggered by rainfall, which have been reported in the media, disaster databases, scientific reports, or other sources. The GLC has been compiled since 2007 at NASA Goddard Space Flight Center. This is a unique data set with the ID tag “GLC” in the landslide editor.

This dataset on data.nasa.gov was a one-time export from the Global Landslide Catalog maintained separately. It is current as of March 7, 2016. The original catalog is available here: http://www.arcgis.com/home/webmap/viewer.html?url=https%3A%2F%2Fmaps.nccs.nasa.gov%2Fserver%2Frest%2Fservices%2Fglobal_landslide_catalog%2Fglc_viewer_service%2FFeatureServer&source=sd

To export GLC data, you must agree to the “Terms and Conditions”. We request that anyone using the GLC cite the two sources of this database:

Kirschbaum, D. B., Adler, R., Hong, Y., Hill, S., & Lerner-Lam, A. (2010). A global landslide catalog for hazard applications: method, results, and limitations. Natural Hazards, 52(3), 561–575. doi:10.1007/s11069-009-9401-4. [1]
Kirschbaum, D.B., T. Stanley, Y. Zhou (In press, 2015). Spatial and Temporal Analysis of a Global Landslide Catalog. Geomorphology. doi:10.1016/j.geomorph.2015.03.016. [2]