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  • 1
    Publication Date: 2009-03-25
    Print ISSN: 0148-0227
    Electronic ISSN: 2156-2202
    Topics: Geosciences
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  • 2
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    In:  Other Sources
    Publication Date: 2019-07-13
    Description: This paper provides a high level overview of NASA's Mars Science Laboratory. Topics to be explored are the Mission's science goals and objectives, a discussion of the mission phases, an overview of the flight system architecture and the payload, and a discussion of the MSL power system.
    Keywords: Lunar and Planetary Science and Exploration
    Type: 9th European Space Power Conference ESPC 2011; Jun 06, 2011; Sainta Raphael; France
    Format: text
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  • 3
    Publication Date: 2019-07-12
    Description: A proposed instrument would project a narrow laser beam that would be frequency-modulated with a pseudorandom noise (PN) code for simultaneous measurement of range and velocity along the beam. The instrument performs these functions in a low mass, power, and volume package using a novel combination of established techniques. Originally intended as a low resource- footprint guidance sensor for descent and landing of small spacecraft onto Mars or small bodies (e.g., asteroids), the basic instrument concept also lends itself well to a similar application guiding aircraft (especially, small unmanned aircraft), and to such other applications as ranging of topographical features and measuring velocities of airborne light-scattering particles as wind indicators. Several key features of the instrument s design contribute to its favorable performance and resource-consumption characteristics. A laser beam is intrinsically much narrower (for the same exit aperture telescope or antenna) than a radar beam, eliminating the need to correct for the effect of sloping terrain over the beam width, as is the case with radar. Furthermore, the use of continuous-wave (CW), erbium-doped fiber lasers with excellent spectral purity (narrow line width) permits greater velocity resolution, while reducing the laser s power requirement compared to a more typical pulsed solid-state laser. The use of CW also takes proper advantage of the increased sensitivity of coherent detection, necessary in the first place for direct measurement of velocity using the Doppler effect. However, measuring range with a CW beam requires modulation to "tag" portions of it for time-of-flight determination; typically, the modulation consists of a PN code. A novel element of the instrument s design is the use of frequency modulation (FM) to accomplish both the PN-modulation and the Doppler-bias frequency shift necessary for signed velocity measurements. This permits the use of a single low-power waveguide electrooptic phase modulator, while simultaneously mitigating the effects of speckle as a noise source in the coherent detection.
    Keywords: Man/System Technology and Life Support
    Type: NPO-40403 , NASA Tech Briefs, February 2005; 9-10
    Format: application/pdf
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  • 4
    Publication Date: 2019-07-12
    Description: The Thermal and Electrical Conductivity Probe (TECP) is a component of the Microscopy, Electrochemistry, and Conductivity Analyzer (MECA) payload on the Phoenix Lander. TECP will measure the temperature, thermal conductivity and volumetric heat capacity of the regolith. It will also detect and quantify the population of mobile H2O molecules in the regolith, if any, throughout the polar summer, by measuring the electrical conductivity of the regolith, as well as the dielectric permittivity. In the vapor phase, TECP is capable of measuring the atmospheric H2O vapor abundance, as well as augment the wind velocity measurements from the meteorology instrumentation. TECP is mounted near the end of the 2.3 m Robotic Arm, and can be placed either in the regolith material or held aloft in the atmosphere. This paper describes the development and calibration of the TECP. In addition, substantial characterization of the instrument has been conducted to identify behavioral characteristics that might affect landed surface operations. The greatest potential issue identified in characterization tests is the extraordinary sensitivity of the TECP to placement. Small gaps alter the contact between the TECP and regolith, complicating data interpretation. Testing with the Phoenix Robotic Arm identified mitigation techniques that will be implemented during flight. A flight model of the instrument was also field tested in the Antarctic Dry Valleys during the 2007-2008 International Polar year. 2
    Keywords: Electronics and Electrical Engineering
    Type: ARC-E-DAA-TN264
    Format: application/pdf
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  • 5
    Publication Date: 2019-07-13
    Description: The distinctive layer visible in images from Mars Global Surveyor of the Martina polar caps, and particularly in the north polar cap, indicates that the stratigraphy of these 'polar layered deposits' may hold a record of Martian climate history covering millions of years.
    Keywords: Lunar and Planetary Science and Exploration
    Type: Lunar and Planetary Science Conference; Mar 15, 2004 - Mar 19, 2004; Houston, TX; United States
    Format: text
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  • 6
    Publication Date: 2019-07-13
    Description: While the overall architecture of an Entry Descent and Landing (EDL) system may vary depending on specific mission requirementsw, measurements of the rate vector with respect to the surface is a primary requirement for the Terminal Descent Control (TDC) phase of any controlled lander.
    Keywords: Lunar and Planetary Science and Exploration
    Type: Coherent Laser Radar Conference; Oct 16, 2005 - Oct 21, 2005; Kamakura; Japan
    Format: text
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  • 7
    Publication Date: 2019-07-10
    Description: In this paper we discuss the semiconductor diode laser developments which will meet the requirements dictated by the Mars Doppler lidar application, and the development and use of a compact lidar for boundary layer measurements which embodies the same measurement approach as the Mars lidar concept.
    Keywords: Instrumentation and Photography
    Type: Nineteenth International Laser Radar Conference; Part 2; 929-930; NASA/CP-1998-207671/PT2
    Format: text
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  • 8
    Publication Date: 2019-08-15
    Description: We have developed a compact Doppler lidar concept which utilizes recent developments in semiconductor diode laser technology in order to be considered suitable for wind and dust opacity profiling in the Mars lower atmosphere from a surface location. The current understanding of the Mars global climate and meteorology is very limited, with only sparse, near-surface data available from the Viking and Mars Pathfinder landers, supplemented by long-range remote sensing of the Martian atmosphere. The in situ measurements from a lander-based Doppler lidar would provide a unique dataset particularly for the boundary layer. The coupling of the radiative properties of the lower atmosphere with the dynamics involves the radiative absorption and scattering effects of the wind-driven dust. Variability in solar irradiance, on diurnal and seasonal time scales, drives vertical mixing and PBL (planetary boundary layer) thickness. The lidar data will also contribute to an understanding of the impact of wind-driven dust on lander and rover operations and lifetime through an improvement in our understanding of Mars climatology. In this paper we discuss the Mars lidar concept, and the development of a laboratory prototype for performance studies, using, local boundary layer and topographic target measurements.
    Keywords: Instrumentation and Photography
    Type: Tenth Biennial Coherent Laser Radar Technology and Applications Conference; 311-312; NASA/CP-1999-209758
    Format: text
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