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  • Other Sources  (8)
  • 2020-2023
  • 2015-2019  (8)
  • 1990-1994
  • 1975-1979
  • 1965-1969
  • 2017  (8)
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  • 2020-2023
  • 2015-2019  (8)
  • 1990-1994
  • 1975-1979
  • 1965-1969
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  • 1
    Publication Date: 2019-07-13
    Description: We report on two NuSTAR observations of the high-mass X-ray binary A 0535+26 taken toward the end of its normal 2015 outburst at very low 3-50 keV luminosities of approximately 1.4 times x 10 (sup 36) ergs per second and approximately 5 times x 10 (sup 35) ergs per second, which are complemented by nine Swift observations. The data clearly confirm indications seen in earlier data that the source's spectral shape softens as it becomes fainter. The smooth exponential rollover at high energies seen in the first observation evolves to a much more abrupt steepening of the spectrum at 20-30 keV. The continuum evolution can be nicely described with emission from a magnetized accretion column, modeled using the compmag model modified by an additional Gaussian emission component for the fainter observation. Between the two observations, the optical depth changes from 0.75 plus or minus 0.04 to 0.56 plus 0.01 (sup) minus 0.04 (sub), the electron temperature remains constant, and there is an indication that the column decreases in radius. Since the energy-resolved pulse profiles remain virtually unchanged in shape between the two observations, the emission properties of the accretion column reflect the same accretion regime. This conclusion is also confirmed by our result that the energy of the cyclotron resonant scattering feature (CRSF) at approximately 45 keV is independent of the luminosity, implying that the magnetic field in the region in which the observed radiation is produced is the same in both observations. Finally, we also constrain the evolution of the continuum parameters with the rotational phase of the neutron star. The width of the CRSF could only be constrained for the brighter observation. Based on Monte Carlo simulations of CRSF formation in single accretion columns, its pulse phase dependence supports a simplified fan beam emission pattern. The evolution of the CRSF width is very similar to that of the CRSF depth, which is, however, in disagreement with expectations.
    Keywords: Astrophysics
    Type: GSFC-E-DAA-TN59952 , Astronomy & Astrophysics (ISSN 0004-6361) (e-ISSN 2197-3504); 608; A105
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  • 2
    Publication Date: 2019-08-13
    Description: Product utility key factors: Near real time, automated production; Flood spatial extent Cloudiness Pixel resolution: 250m; Flood temporal extent; Flash floods short duration on ground?; Landcover--Water under vegetation cover vs open water
    Keywords: Earth Resources and Remote Sensing
    Type: GSFC-E-DAA-TN46195 , Disaster Risk Reduction (DRR) Across the Americas Summit; Sep 03, 2017 - Sep 08, 2017; Buenos Aires; Argentina
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  • 3
    Publication Date: 2019-07-13
    Description: A next-generation lunar lander Guidance, Navigation, and Control (GNC) system, which includes a state-of-the-art optical sensor suite, is proposed in a concept design cycle. The design goal is to allow the lander to softly land within the prescribed landing precision. The achievement of this precision landing requirement depends on proper selection of the sensor suite. In this paper, a robust sensor selection procedure is demonstrated using a Linear Covariance (LinCov) analysis tool developed by Draper.
    Keywords: Spacecraft Design, Testing and Performance
    Type: JSC-CN-38188 , AIAA SciTech 2017 Conference; Jan 09, 2017 - Jan 13, 2017; Grapevine, TX; United States
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  • 4
    Publication Date: 2019-08-26
    Description: An endoscopic illumination system for illuminating a subject for stereoscopic image capture, includes a light source which outputs light; a first complementary multiband bandpass filter (CMBF) and a second CMBF, the first and second CMBFs being situated in first and second light paths, respectively, where the first CMBF and the second CMBF filter the light incident thereupon to output filtered light; and a camera which captures video images of the subject and generates corresponding video information, the camera receiving light reflected from the subject and passing through a pupil CMBF pair and a detection lens. The pupil CMBF includes a first pupil CMBF and a second pupil CMBF, the first pupil CMBF being identical to the first CMBF and the second pupil CMBF being identical to the second CMBF, and the detection lens includes one unpartitioned section that covers both the first pupil CMBF and the second pupil CMBF.
    Keywords: Instrumentation and Photography
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  • 5
    Publication Date: 2020-01-18
    Description: The Autonomy Operating System (AOS) is an open flight software platform with Artificial Intelligence for smart UAVs. It is built to be extendable with new apps, similar to smartphones, to enable an expanding set of missions and capabilities. AOS has as its foundations NASAs core flight executive and core flight software (cFEcFS). Pilot-in-a-Box (PIB) is an expanding collection of interacting AOS apps that provide the knowledge and intelligence onboard a UAV to safely and autonomously fly in the National Air Space, eventually without a remote human ground crew. Longer-term, the goal of PIB is to provide the capability for pilotless air vehicles such as air taxis that will be key for new transportation concepts such as mobility-on-demand. PIB provides the procedural knowledge, situational awareness, and anticipatory planning (thinking ahead of the plane) that comprises pilot competencies. These competencies together with a natural language interface will enable Pilot-in-a-Box to dialogue directly with Air Traffic Management from takeoff through landing. This paper describes the overall AOS architecture, Artificial Intelligence reasoning engines, Pilot-in-a-box competencies, and selected experimental flight tests to date.
    Keywords: Avionics and Aircraft Instrumentation
    Type: ARC-E-DAA-TN43236 , AIAA Aviation Forum 2017; Jun 05, 2017 - Jun 09, 2017; Denver, CO; United States
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  • 6
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    Springer
    In:  International Journal of Earth Sciences, 106 (8). pp. 2999-3003.
    Publication Date: 2020-02-06
    Description: Karl Andrée began studying questions of sedimentology and oceanography in 1908 when working as an assistant at the University of Marburg and he remained faithful to these subjects until his death in 1959. The vast majority of his scientific contributions, however, were published during his time at the University of Königsberg (1915–1945). There he published his fundamental papers on marine geology, all of which adhered strictly to the principles of uniformitarianism, and helped improve our understanding of sedimentary processes and the stratigraphic record. His scientific work has enormous breadth. In the course of 55 years, he published 124 individual papers and books, some of which became classic textbooks. His versatility is particularly evident in his book “Geology of the Seafloor”, which contains many pertinent observations and descriptions still relevant today, even if it has fallen out of fashion. This scientist and university teacher was the first to successfully present the huge field of marine geology in all its facet and to consider the deposition of marine sediments as a function of their geographical distribution.
    Type: Article , PeerReviewed
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  • 7
    Publication Date: 2019-03-11
    Description: The second briefing paper summarizing work being carried-out in AtlantOS. The outcome will be presented to the stakeholders in a briefing event.
    Type: Report , NonPeerReviewed , info:eu-repo/semantics/book
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  • 8
    Publication Date: 2019-03-11
    Description: The first briefing paper summarizing work being carried-out in AtlantOS. The outcome will be presented to the stakeholders in a briefing event
    Type: Report , NonPeerReviewed , info:eu-repo/semantics/book
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