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  • 1
    facet.materialart.
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    In:  CASI
    Publikationsdatum: 2019-08-28
    Beschreibung: Statistical mechanics for wall shear turbulence in Couette flow based on Brownian motion and comparison with stochastic theory based on Navier-Stokes equation
    Schlagwort(e): AERODYNAMICS
    Materialart: NASA-SP-4014
    Format: application/pdf
    Standort Signatur Erwartet Verfügbarkeit
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  • 2
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    In:  CASI
    Publikationsdatum: 2019-08-28
    Beschreibung: Annotated bibliography and indexes on aeronautical engineering and aerodynamics - July 1971
    Schlagwort(e): AERODYNAMICS
    Materialart: NASA-SP-7037(07)
    Format: application/pdf
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  • 3
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    Unbekannt
    In:  CASI
    Publikationsdatum: 2019-08-28
    Beschreibung: Analyses of aircraft aerodynamic characteristics
    Schlagwort(e): AERODYNAMICS
    Materialart: NASA-SP-228 , A Symposium Held at Ames Research Center; Oct 28, 1969 - Oct 30, 1969; MOFFETT FIELD, CA; United States
    Format: application/pdf
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  • 4
    facet.materialart.
    Unbekannt
    In:  CASI
    Publikationsdatum: 2019-08-28
    Beschreibung: Annotated reference bibliography on aeronautical engineering documents
    Schlagwort(e): AERODYNAMICS
    Materialart: NASA-SP-7037(01)
    Format: application/pdf
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  • 5
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    Unbekannt
    In:  CASI
    Publikationsdatum: 2019-08-28
    Beschreibung: Annotated bibliography and indexes on aeronautical engineering and aerodynamics - Jan. 1971
    Schlagwort(e): AERODYNAMICS
    Materialart: NASA-SP-7037(02)
    Format: application/pdf
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  • 6
    Publikationsdatum: 2019-08-28
    Beschreibung: We analyze simultaneous, or near-simultaneous, coregistered, digital, photometric images of solar photospheric intensity and line-of-sight magnetic field. Images were made with the Lockheed tunable filter instrument at the Swedish Solar Observatory, La Palma, with the video spectra-spectroheliograph system at the San Fernando Observatory and with the new NASA spectromagnetograph at the National Solar Observatory at Kitt Peak. We study the disk center contrasts of small magnetic elements. While active region faculae are dark at disk center quiet Sun network features are bright. The populations of magnetic field elements that make up these two kinds of features are quite different. Different contrast center-limb functions must be used when estimating their irradiance or luminosity contributions. The disk center contrasts of active region faculae are colar dependent and indicate a depth effect related to the H(-) opacity of the facular atmopshere. This results is important for calibration of monochromatic observations of faculae to bolometric irradiance fluctuations. We emphasize the value of cooperative observations among installations whose differing strengths are complementary.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Journal of Geophysical Research (ISSN 0148-0227); 98; A11; p. 18,911-18,918
    Format: text
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  • 7
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    In:  Other Sources
    Publikationsdatum: 2019-08-28
    Beschreibung: This paper presents an extension of the nonlinear least squares fitting technique of Vinas and Scudder (1986) (VS), which finds the physical and geometrical properties of nondissipational magnetohydrodynamic (MHD) shocks. The new method incorporates plasma temperature observations in the form of normal momentum flux and energy density flux conservation as well as plasma density, velocity, and magnetic field data. The new technique is capable of using known standard deviations in the individual measurement points to properly weight the fitting procedure. The new fitting code is validated through the analysis of synthetic shocks with known physical and geometrical properties. Finally, it is compared to the original VS method and the preaveraged velocity coplanarity technique.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Journal of Geophysical Research (ISSN 0148-0227); 99; A8; p. 14,737-14,746
    Format: text
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  • 8
    Publikationsdatum: 2019-08-28
    Beschreibung: We present the first results of solar active region observations with the recently completed five-element Owens Valley Solar Array. On 1991 October 24, maps of Active Region AR 6891 were obtained at 22 frequencies from 1.2-7.0 GHz to provide brightness temperature spectra at each point. This is the first time that both high spatial and frequency-resolution brightness temperature spectra have been available over such a broad radio-frequency range. We find that over most of the region the spectra fall into one of the two well-defined categories: thermal free-free or thermal gyroresonance. In these cases, we use the spectra to deduce the spatial variation of physical parameters-electron temperature, column emission measure (intergral n(sup 2)(sub e) dl), and the coronal magnetic field strength-in and around the active region. Over a limited area of the region, the spectra resemble neither of the simple types, and alternative interpretations are required. The possibilties include the presence of fine structure that is unresolved at low frequencies; the presence of a small number of nonthermal electrons; or the presence of overlying, cooler 10(exp 6) K material which at low frequencies absorbs the hot (3 x 10(exp 6) K) thermal emission generated below.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: The Astrophysical Journal, Part 1 (ISSN 0004-637X); 420; 2; p. 903-912
    Format: text
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  • 9
    Publikationsdatum: 2019-08-28
    Beschreibung: The theoretical electron density sensitive emission-line ratio R = I(1718.56 a)/I(1486.51 A) in N IV is presented for a range of N(sub e)(approximately equals 10(exp 10) - 10(exp 12)/cu cm) applicable to higher density solar plasmas, such as active regions. A comparison of these calculations with the observed values of R of several solar features obtained with the Naval Research Laboratory's S082B spectrograph on board Skylab reveals general agreement between theory and observation at pointings just above the limb, where line blends with N IV 1718.56 A should be insignificant, which provides experimental support for the accuracy of the line ratio calculations.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal, Part 1 (ISSN 0004-637X); 432; 2; p. 806-808
    Format: text
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  • 10
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    In:  Other Sources
    Publikationsdatum: 2019-08-28
    Beschreibung: Sixteen years of Wilcox Solar Observatory (WSO) magnetogram data have been studied to determine the solar cycle variation and latitude dependence of the east-west inclination of photospheric magnetic field lines. East-west inclination is here defined as the angle between a field line and its local radial vector, as projected onto the plane of the latitude and line of sight. Inclination is determined by a least-squares fit of observed magnetic fields to a simple projection model, and is found to depend on polarity and to change with the solar cycle. Leading and following polarities are tipped towards each by about 9 deg and have an overall net tilt in the direction of rotation (to the west) of 0.6 deg. New cycles are seen to begin at high latitudes and to grow through the lower latitudes over approximately 5 years, providing evidence for an extended cycle length of 16-18 years.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics (ISSN 0038-0938); 153; 2-Jan; p. 131-141
    Format: text
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