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  • 1
    Publication Date: 2014-09-17
    Description: A proposed conceptual design of a 400 kW continuous wave (CW)K sub a band transmitter and associated microwave components to be used for planetary radar and serve as a prototype for future spacecraft uplinks is discussed. System requirements for such a transmitter are presented. Performance of the proposed high-power millimeter wave tube, the gyroklystron is discussed. Parameters of the proposed power amplifier, beam supply, and monitor and control devices are also presented. Microwave transmission line components consisting of signal monitoring devices, signal filtering devices, and an overmoded corrugated feed are discussed. Finally, an assessment of the state of the art technology to meet the system requirements is given and possible areas of difficulty are summarized.
    Keywords: ELECTRONICS AND ELECTRICAL ENGINEERING
    Type: The Telecommun. and Data Acquisition Rept.; p 24-48
    Format: text
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  • 2
    Publication Date: 2019-07-18
    Description: Saccadic eye movements during search for a target embedded in noise are suboptimally guided by information about target location. Our goal is to compare the spatial information used to guide the saccades with that used for the perceptual decision. Three observers were asked to determine the location of a bright disk (diameter = 21 min) in white noise (signal-to-noise ratio = 4.2) from among 10 possible locations evenly spaced at 5.9 deg eccentricity. In the first of four conditions, observers used natural eye movements. In the three remaining conditions, observers fixated a central cross at all times. The fixation conditions consisted of three different presentation times (100, 200, 300 msec), each followed by a mask. Eye-position data were collected, with a resolution of (approximately) 0.2 deg. In the natural viewing condition, we measured. the accuracy with respect to the target and the latency of the first saccade. In the fixation conditions, we discarded trials in which observers broke fixation. Perceptual performance was computed for all conditions. Averaged across observers, the first saccade was correct (closest to the target location) for 56 +/- (SD) % of trials (chance = 10 %) and occurred after a latency of 313 +/- 56 msec. Perceptual performance averaged 53 +/- 4, 63 +/- 4, 65 +/- 2 % correct at 100, 200, and 300 msec, respectively. For the signal-to-noise ratio used, at the time of initiation of the first saccade, there is little difference between the amount of information about target location available to the perceptual and saccadic systems.
    Keywords: Aerospace Medicine
    Type: 1997 European Conference on Visual Perception; Aug 25, 1997 - Aug 29, 1997; Helsinki; Finland
    Format: text
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  • 3
    Publication Date: 2019-08-17
    Description: The Charon/Pluto mass ratio is a fundamental but poorly known parameter of the two-body system. Previous values for the mass ratio have ranged from 0.0837 plus or minus 0.0147 (Null et al., 1993, Astron. J. 105, 2319-2335) to 0.1566 plus or minus 0.0035 (Young et al., 1994, Icarus 108,186-199). We report here a new determination of the Charon/Pluto mass ratio, using five sets of groundbased images taken at four sites in support of Pluto occultation predictions. Unlike the Null et al. and Young et A determinations, where the centers of light for Pluto and Charon could be determined separately, this technique examines the motion of the center of light of the blended Pluto-Charon image. We compute the offsets of the observed center-of-light position of Pluto-Charon from the ephemeris position of the system and fit these offsets to a model of the Pluto-Charon system. The least-squares fits to the five data sets agree within their errors, and the weighted mean mass ratio is 0.117 plus or minus 0.006. The effects of errors in the Charon light fraction, semimajor axis, and ephemeris have been examined and are equal to only a small fraction of the formal error from the fit. This result is intermediate between those of Null et al., and Young et al. and matches a new value of 0.124 plus or minus 0.008 by Null and Owen (1996, Astron. J. 111, 1368-1381). The mass ratio and resulting individual masses and densities of Pluto and Charon are consistent with a collisional origin for the Pluto-Charon system.
    Keywords: Astrophysics
    Type: IS965656 , Icarus (ISSN 0019-1035); 126; 362-372
    Format: text
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  • 4
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    In:  Bull. Seism. Soc. Am., Basel, Inst. f. Geophys., Ruhr-Univ. Bochum, vol. 92, no. 7, pp. 2659-2669, pp. 1019, (ISSN: 1340-4202)
    Publication Date: 2002
    Keywords: paleo ; Crustal deformation (cf. Earthquake precursor: deformation or strain) ; Seismicity ; SAF ; Fault zone ; Geol. aspects ; USA ; BSSA ; J ; w/out ; dot
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  • 5
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    In:  Proc. of the Inst. Electr. Electron. Eng., Leyden, Noordhoff International Publishing, vol. 72, no. 3, pp. 1394-1402, pp. B04306, (ISSN: 1340-4202)
    Publication Date: 1984
    Keywords: Waves ; Seismics (controlled source seismology) ; Wavelet processing ; Inversion ; IEEE
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  • 6
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    In:  Geophysics: The Leading Edge of Exploration, Leyden, Noordhoff International Publishing, vol. 9, no. 3, pp. 34-42, pp. B04306, (ISSN: 1340-4202)
    Publication Date: 1990
    Keywords: Stacking ; Data analysis / ~ processing
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  • 7
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    In:  Bull. Seism. Soc. Am., Leyden, Noordhoff International Publishing, vol. 92, no. 3, pp. 983-997, pp. B04306, (ISSN: 1340-4202)
    Publication Date: 2002
    Keywords: Geol. aspects ; Seismicity ; Fault zone ; SAF ; USA ; Structural geology ; BSSA ; J ; w/out ; dot
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  • 8
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    In:  Science, Leyden, Noordhoff International Publishing, vol. 299, no. 5615, pp. 2015, pp. B04306, (ISSN: 1340-4202)
    Publication Date: 2003
    Keywords: Volcanology ; Earthquake precursor: prediction research ; Review article
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  • 9
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    American Inst. of Physics
    In:  Raleigh, North Carolina, American Inst. of Physics, vol. I, 383+VIII pp., no. Publ. No. 12, pp. 127, (ISBN 0 465 07009 4)
    Publication Date: 1990
    Keywords: Chaotic behaviour ; Textbook of informatics
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  • 10
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    Society of Exploration Geophysicists
    In:  abstract , Tulsa, Oklahoma, Society of Exploration Geophysicists, vol. 339-350, no. 32, pp. 103-108, (ISBN 3-933346-037)
    Publication Date: 1986
    Keywords: Reflection seismics ; Seismics (controlled source seismology)
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