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  • Other Sources  (20)
  • GEOPHYSICS  (6)
  • ASTRODYNAMICS  (5)
  • COMMUNICATIONS  (5)
  • GENERAL  (2)
  • AERODYNAMICS  (1)
  • Lunar and Planetary Science and Exploration  (1)
  • 1
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    In:  CASI
    Publication Date: 2005-04-26
    Keywords: GENERAL
    Type: NACA 1957 Flight Propulsion Conf.; p 1-12
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  • 2
    Publication Date: 2011-08-16
    Description: VLF observations of auroral beams for auroral V-emissions source and characteristics, explaining spectral shape
    Keywords: GEOPHYSICS
    Type: ; ADEMIE DES SCIENCES
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  • 3
    Publication Date: 2016-06-07
    Description: Taking advantage of the improvements to the Earth's gravitation field and tracking station coordinates, an orbital computational consistency of the order of 5 meters was achieved for total position differences between orbital solutions for the Seasat and GEOS-3. The main source of error in these solutions was in the mathematical models that are required to generate these results, i.e., gravitation, atmospheric drag, etc. Different Earth gravitation fields and tracking coordinates were analyzed and evaluated in obtaining these computational results. Comparisons and evaluations of the Seasat results were obtained in terms of different solution types such as the Doppler only, Laser only, Doppler and Laser, etc. Other investigation using the Seasat data were made in order to determine their effect on the computational results at this particular level of consistency.
    Keywords: ASTRODYNAMICS
    Type: Sixth Ann. Flight Mech.(Estimation Theory Symp.; 36 p
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  • 4
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    In:  Other Sources
    Publication Date: 2019-05-30
    Description: Whistler in Alouette I satellite VLF RECORDINGS, variation of time delay with frequency given by Eckersley law time delay and additive correction term
    Keywords: GEOPHYSICS
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  • 5
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    In:  Other Sources
    Publication Date: 2019-05-24
    Description: Subprotonospheric whistler reflections at 1000 km attributed to energy refraction by hydrogen ions
    Keywords: COMMUNICATIONS
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  • 6
    Publication Date: 2019-06-28
    Description: A recent mathematical technique for solving systems of equations is applied in a very general way to the orbit determination problem. The study of this technique, the homotopy continuation method, was motivated by the possible need to perform early orbit determination with the Tracking and Data Relay Satellite System (TDRSS), using range and Doppler tracking alone. Basically, a set of six tracking observations is continuously transformed from a set with known solution to the given set of observations with unknown solutions, and the corresponding orbit state vector is followed from the a priori estimate to the solutions. A numerical algorithm for following the state vector is developed and described in detail. Numerical examples using both real and simulated TDRSS tracking are given. A prototype early orbit determination algorithm for possible use in TDRSS orbit operations was extensively tested, and the results are described. Preliminary studies of two extensions of the method are discussed: generalization to a least-squares formulation and generalization to an exhaustive global method.
    Keywords: ASTRODYNAMICS
    Type: NASA-TM-86230 , NAS 1.15:86230
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  • 7
    Publication Date: 2019-05-24
    Description: Proton whistler /VLF phenomenon observed in satellite data/ discussing propagation in multicomponent plasma and ion cyclotron mode
    Keywords: COMMUNICATIONS
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  • 8
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    In:  Other Sources
    Publication Date: 2019-05-24
    Description: Unusual noise band observed in VLF recordings of Alouette, investigating resonance in plasma surrounding satellite
    Keywords: COMMUNICATIONS
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  • 9
    Publication Date: 2018-06-06
    Description: Infrared heterodyne spectra of isotopic CO2 in the Martian atmosphere were obtained using the Goddard Heterodyne Instrument for Planetary Wind and Composition, HIPWAC, which was interfaced with the 3-meter telescope at the NASA Infrared Telescope Facility- Spectra were colle cted at a resolution of lambda/delta lambda=10(exp 7). Absorption fea tures of the CO2 isotopologues have been identified from which isotop ic ratios of oxygen have been determined. The isotopic ratios O-17/O -16 and O-18/O-16 in the Martian atmosphere can be related to Martian atmospheric evolution and can be compared to isotopic ratios of oxyg en in the Earth's atmosphere. Isotopic carbon and oxygen are importa nt constraints on any theory for the erosion of the Martian primordia l atmosphere and the interaction between the atmosphere and surface o r subsurface chemical reservoirs. This investigation explored the pr esent abundance of the stable isotopes of oxygen in Mars' atmospheric carbon dioxide by measuring rovibrational line absorption in isotop ic species of CO2 using groundbased infrared heterodyne spectroscopy in the vicinity of the 9.6 micron and 10.6 micron CO2 lasing bands. T he target transitions during this observation were O-18 C-12 O-16 as well as O-178 C-12 O-16 and O-16 C-113 O-16 at higher resolving power of lambda/delta lambda=10(exp 7) and with high signal-to-noise ratio (longer integration time) in order to fully characterize the absorpt ion line profiles. The fully-resolved lineshape of both the strong n ormal-isotope and the weak isotopic CO2 lines were measured simultane ously in a single spectrum.
    Keywords: Lunar and Planetary Science and Exploration
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  • 10
    Publication Date: 2019-05-30
    Description: Lower hybrid resonance in VLF range in satellites, noting noise emission due to trapping of electromagnetic wave propagation in transverse magnetic field
    Keywords: GEOPHYSICS
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