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  • General Chemistry  (1.172)
  • Life and Medical Sciences  (310)
  • AIRCRAFT PROPULSION AND POWER
  • Cell & Developmental Biology
  • Earth model, also for more shallow analyses !
  • SOLAR PHYSICS
  • 1975-1979  (1.596)
  • 1945-1949
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  • 1915-1919  (383)
  • 1975  (1.596)
  • 1915  (383)
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  • 1975-1979  (1.596)
  • 1945-1949
  • 1920-1924
  • 1915-1919  (383)
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  • 1
    facet.materialart.
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    In:  Rev. Geophys. Space Phys., Taipei, Elsevier, vol. 13, no. 1, pp. 57-86, pp. RG2001, (ISBN: 0-12-018847-3)
    Publikationsdatum: 1975
    Schlagwort(e): P-waves ; Earth model, also for more shallow analyses ! ; Physical properties of rocks ; Review article
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  • 2
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    In:  Phys. Earth Plan. Int., Luxembourg, U.S. Geological Survey, vol. 10, no. 24, pp. 12-48, pp. B05309, (ISBN 0-471-26610-8)
    Publikationsdatum: 1975
    Schlagwort(e): Earth model, also for more shallow analyses ! ; Seismology ; Review article ; Velocity depth profile ; PEPI ; Dziewonski
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  • 3
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    McGraw-Hill
    In:  New York, 618 pp., McGraw-Hill, vol. I, 383+VIII pp., no. Publ. No. 12, pp. 127, (ISBN 0-521-66034-3, ISBN 0-521-66948-0 paper)
    Publikationsdatum: 1975
    Schlagwort(e): Textbook of geophysics ; Physical properties of rocks ; Earth model, also for more shallow analyses ! ; Textbook of mineralogy ; Textbook of geology
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  • 4
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    Unbekannt
    In:  Phys. Earth Plan. Int., Luxembourg, U.S. Geological Survey, vol. 10, no. 3-4, pp. 12-48, pp. B05309, (ISBN 0-471-26610-8)
    Publikationsdatum: 1975
    Schlagwort(e): Earth model, also for more shallow analyses ! ; Physical properties of rocks ; Seismology ; PEPI ; Dziewonski
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  • 5
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    In:  Geol. Soc. Am. Bull., Taipei, Elsevier, vol. 86, no. 1, pp. 227-236, pp. RG2001, (ISBN: 0-12-018847-3)
    Publikationsdatum: 1975
    Schlagwort(e): P-waves ; Earth model, also for more shallow analyses ! ; Physical properties of rocks ; Laboratory measurements ; GSA
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  • 6
    Publikationsdatum: 2006-01-12
    Beschreibung: Deviations betweeb observed Doppler noise and the noise model during solar conjunction were analyzed. It is tentatively concluded that these deviations are due to short-term fluctuations in solar activity as seen along the signal path, and not to solar/antenna structure effects or system noise temperature.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: The Deep Space Network; p 264-272
    Format: text
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  • 7
    Publikationsdatum: 2006-01-12
    Beschreibung: The results of a study of Doppler data noise during solar conjunctions were presented. During the first half of 1975, a sizeable data base of Doppler data noise (estimates) for the Pioneer 10, Pioneer 11, and Helios 1 solar conjunctions was accumulated. To analyze this data, certain physical assumptions are made, leading to the development of a geometric parameter ("ISI") which correlates strongly with Doppler data noise under varying sun-earth-spacecraft geometries. Doppler noise models are then constructed from this parameter, resulting in the newfound ability to predict Doppler data noise during solar conjunctions, and hence to additionally be in a position to validate Doppler data acquired during solar conjunctions.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: The Deep Space Network; p 231-263
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  • 8
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    In:  CASI
    Publikationsdatum: 2006-01-11
    Beschreibung: Flight vehicles are characterized according to their manner of operation and type of propulsion system; and their associated sources of noise are identified. Available noise reduction technology as it relates to engine cycle design and to powerplant component design is summarized. Such components as exhaust jets, fans, propellers, rotors, blown flaps, and reciprocating-engine exhausts are discussed, along with their noise reduction potentials. Significant aircraft noise reductions are noted to have been accomplished by the application of available technology in support of noise certification rules. Further noise reductions to meet more stringent future noise regulations will require substantial additional technology developments. Improved analytical prediction methods, and well-controlled validation experiments supported by advanced-design aeroacoustic facilities, are required as a basis for an effective integrated systems approach to aircraft noise control.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA/Univ. Conf. on Aeron.; p 103-130
    Format: text
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  • 9
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    In:  CASI
    Publikationsdatum: 2006-01-11
    Beschreibung: Studies conducted outside the effect of the earth's magnetic field during the revolution period by the Prognoz satellite are examined. In particular, the unperturbed solar wind, the flux of charged particles continually given off the sun is studied. Solar activity and its effects on various natural phenomena are discussed.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Mod. Achievements of Cosmonautics (NASA-TT-F-16221); p 57-62
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  • 10
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: Recent research into plasma processes involved in the expansion of the solar wind and the interplanetary medium is reviewed. Emphasized topics deal primarily with processes that drive the solar wind, the gross expansion of the interplanetary medium between 0.5 and 5 AU, recent observational results in the vicinity of 1 AU, and the microstructure of the interplanetary medium. Satellite measurements of the radial profile of the interplanetary medium out to 5 AU are discussed together with model calculations of the solar wind and its possible driving mechanisms. Studies of Alfven and magnetoacoustic waves in the solar wind are summarized. Possible roles are considered for thermal conduction in coronal energy transport, and observations of ion velocity distributions near 1 AU are described.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Reviews of Geophysics and Space Physics; 13; July 197
    Format: text
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  • 11
    Publikationsdatum: 2011-08-16
    Beschreibung: Subordinate 2p(5)4d-2p(5)3p transitions in the neon-like ions from Ca XI through Ni XIX are identified. Such transitions between excited levels have not previously been reported for ionization stages higher than Al IV, although the resonance lines are known through Zn XXI in the neon isoelectronic sequence. Measurement of the solar flux in such transitions may aid in establishing the relative importance of the several cascade processes giving rise to the observed Fe XVII resonance lines.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 199; Aug. 1
    Format: text
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  • 12
    Publikationsdatum: 2011-08-16
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 199; Aug. 1
    Format: text
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  • 13
    Publikationsdatum: 2011-08-16
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astronomy and Astrophysics; 40; 4, Ma; May 1975
    Format: text
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  • 14
    Publikationsdatum: 2011-08-16
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 199; July 15
    Format: text
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  • 15
    Publikationsdatum: 2011-08-16
    Beschreibung: Profiles obtained from NRL Skylab solar spectra of the 1640.4 A feature identified as the H-alpha line of He II are discussed and compared with theoretical profiles derived assuming (1) collisional excitation and (2) radiative recombination as the dominant excitation mechanism. Relative intensities of this line as a function of altitude above and below the solar white-light limb are also given for a representative quiet sun region and for a polar coronal hole.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 199; July 1
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  • 16
    Publikationsdatum: 2011-08-16
    Beschreibung: Previous determinations of the form of the emission-measure distribution function for solar active regions are examined. It is found that two analyses in particular are affected by low quality of either observational or atomic data. An alternative method of analysis is discussed.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 199; July 1
    Format: text
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  • 17
    Publikationsdatum: 2011-08-16
    Beschreibung: The topology of the boundaries of penetration (or, inversely, the boundaries of the forbidden regions) of 90-deg pitch-angle equatorial protons with energies less than 100 keV are explored for an equatorial convection E-field which is directed in general from dawn to dusk. Due to the dependence of drift path on energy (or magnetic moment), complex structural features are expected in the proton energy spectra detected by satellites since the penetration distance of a proton is not a monotonically increasing or decreasing function of energy. During a storm when the convection E is enhanced, model calculations predict elongations of the forbidden regions analogous to tail extensions of the plasmasphere. Following a reduction in the convection field, spiral-structured forbidden regions can occur. Structural features inherent to large-scale convection field changes may be seen in the nose-like proton spectrograms observed near dusk by instrumentation on Explorer 45. These nose events are modelled by using an electric field model developed originally by Volland (1973). The strength of the field is related to the Kp index through night-time equatorial plasmapause measurements.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Planetary and Space Science; 23; July 197
    Format: text
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  • 18
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: The overabundance of heavy nuclei in solar cosmic rays of energy below about 10 MeV/nucleon is explained by taking into account the pre-flare ionization states of these nuclei in the region where they are accelerated. A model is proposed which considers two-step accelerations associated with the initial development of solar flares. The first step is closely related to the triggering process of flares, while the second one starts with the development of the explosive phase. Further ionization of medium and heavy nuclei occurs through their interaction with keV electrons accelerated by the first-step acceleration. It is suggested that the role of these electrons is important in producing fully ionized atoms in the acceleration regions.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Planetary and Space Science; 23; June 197
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  • 19
    Publikationsdatum: 2011-08-16
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 41; Apr. 197
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  • 20
    Publikationsdatum: 2011-08-16
    Beschreibung: Energetic particle data are presented from a series of solar flares with a relative abundance of He-3 much higher than that of any previous events. The abundance of protons relative to He nuclei was significantly low in these events; not more than four H-2 and three H-3 were detected during the entire period under study, compared with 1110 He-3 nuclei. Results from these experiments are compared with data available from other investigations, and the limitations the former observations place on theoretical models to explain He-3-rich flares are discussed.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 198; May 15
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  • 21
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: A detailed study of the charge composition of heavy solar cosmic rays measured in the January 25, 1971 solar flare including differential fluxes for the even-charged nuclei from carbon through argon is presented. The measurements are obtained for varying energy intervals for each nuclear species in the energy range from 10 to 35 MeV per nucleon. In addition, abundances relative to oxygen are computed for all the above nuclei in the single energy interval from 15 to 25 MeV per nucleon. This interval contains measurements for all of the species and as a result requires no spectral extrapolations. An upper limit for the abundance of calcium nuclei is also presented. These measurements, when combined with other experimental results, enable the energy dependence of abundance measurements as a function of nuclear charge to be discussed. It is seen that at energies above about 10 MeV per nucleon, the variations of abundance ratios are limited to about a factor of 3 from flare to flare, in spite of large variations in other characteristics of these solar events.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 41; Apr. 197
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  • 22
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: Missions planned for OSO-8 are outlined. Instruments to be included on the satellite comprise a multichannel UV spectrometer, a high-resolution UV spectrometer, an X-ray crystal spectrometer and polarimeter, a hard X-ray telescope, a celestial X-ray spectrometer, a mapping X-ray heliometer, an extrasolar extreme UV monitor, and a soft X-ray telescope. The instruments make up a scientific payload that is larger, transmits data at a greater rate, can be pointed with higher accuracy, and has much better spatial and spectral resolution over a wider range of wavelengths than any payload carried by previous OSO satellites.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Sky and Telescope; 49; June 197
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  • 23
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: Preliminary results are reported for the synthesis of a solar active region from observations with a synthesis radio telescope at a wavelength of 6 cm. Several individual sources are observed in the total-intensity and circular-polarization maps. These are shown to correspond to two large sunspots, two groups of small sunspots, and a plage. A magnetogram indicates that this active region had a bipolar structure with positive polarity concentrated on the main sunspots and negative polarity scattered over the plage and some of the small sunspots. It is noted that several radio bursts were recorded during the observation period and that one corresponded to a H-alpha flare near one of the sunspot groups.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Nature; 257; Oct. 9
    Format: text
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  • 24
    Publikationsdatum: 2011-08-16
    Beschreibung: Evidence is reported for a seasonal variation in the effect of solar sector structure on terrestrial atmospheric vorticity. Graphs showing average response of the 50,000-Pa vorticity area index to solar magnetic sector structure during the time interval extending from 6 days before to 6 days after the time at which a sector boundary is swept past the earth indicate that a 10% drop in the average value occurs at the time of passage, but this effect is observed only during the winter months.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Nature; 255; June 12
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  • 25
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: Published spectroscopic measurements of solar rotation are analyzed to show that when the rotation velocity increases at high latitudes it tends to decrease at low latitudes, and that when the rotation velocity decreases at high latitudes it increases at low latitudes. The high-latitude velocities typically vary over only 20% of the range of those near the equator and the smallest variations of all occurred near latitude 60 deg during the rising portion of the previous solar cycle. The anticorrelation is consistent with a recent suggestion that differential rotation on the sun arises from photospheric wind systems whose strength is determined, ultimately, by oscillations within the sun.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 41; Apr. 197
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  • 26
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: The basic variations in solar wind properties that have been observed at 'stream interfaces' near 1 AU are explained by a gas dynamic model in which a radially propagating stream, produced by a temperature variation in the solar envelope, steepens nonlinearly while moving through interplanetary space. The region thus identified with the stream interface separates the ambient solar wind from the fresh hot material originally in the stream. However, the interface regions given by the present model are thicker than most stream interfaces observed in the solar wind, a fact suggesting that some additional physical process may be important in determining that thickness. Variations in the density, speed, or Alfven pressure alone appear not to produce streams with such an interface.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Journal of Geophysical Research; 80; May 1
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  • 27
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: Plasma and magnetic field observations of interplanetary streams near 1 AU are summarized. Two types of streams have been identified - corotating streams and flare-associated, and other flow patterns are present due to interactions among streams. The theory of corotating streams, which attributes them to a high temperature region near the sun, satisfactorily explains many of the effects observed at 1 AU. A correspondingly complete theory of flare-associated streams does not exist. Streams are a key link in the chain that connects solar and geomagnetic activity. The factors that most influence geomagnetic activity are probably related to streams and determined by the dynamics of streams. The evolution of streams on scales of 27 days and 11 years probably determines the corresponding variations of geomagnetic activity.
    Schlagwort(e): SOLAR PHYSICS
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  • 28
    Publikationsdatum: 2011-08-16
    Beschreibung: A statistical study of the initial phases of a large number of solar particle events provides an approach for an investigation of the variability in the production process and coronal diffusion. A description is given of the procedures which are suitable for identifying the parent flare of an event, taking into account the heliocentric distribution of the flare-associated events. The determination of the proton energy spectrum at the sun is discussed along with the variation of the spectral index with the associated flare heliocentric longitude, questions concerning the source spectra and the acceleration process, and the size distribution of flare associated particle events.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 41; Mar. 197
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  • 29
    Publikationsdatum: 2011-08-16
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 41; Mar. 197
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  • 30
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Journal of Geophysical Research; 80; Apr. 1
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  • 31
    Publikationsdatum: 2011-08-16
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Acoustical Society of America; vol. 57
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  • 32
    Publikationsdatum: 2011-08-16
    Beschreibung: Skylab XUV coronal spectroheliograms and photospheric magnetograms are compared. This comparison shows that, as new bipolar magnetic fields emerge through the solar surface into the corona, the new coronal fields interact with the old ones in a manner that suggests the reconnection of the field lines.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 196; Mar. 15
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  • 33
    Publikationsdatum: 2011-08-16
    Beschreibung: The astrometric technique used to derive solar wind speeds from ionic comet-tail orientations has been used to test the suggestion that the radial solar wind speed is higher near the solar poles than near the equator. We find no evidence for the suggested latitude variation.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 196; Mar. 15
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  • 34
    Publikationsdatum: 2011-08-16
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 196; Mar. 1
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  • 35
    Publikationsdatum: 2011-08-16
    Beschreibung: Spectroheliograms obtained with the Naval Research Laboratory's Extreme Ultraviolet Spectrograph (S082A) on Skylab are compared with Kitt Peak National Observatory magnetograms. A principal result is the characteristic reconnection of flux from an emerging bipolar magnetic region to previously existing flux in its vicinity. Examples of the disappearance of magnetic flux from the solar atmosphere are also shown. The results of a particularly simple, potential field calculation are shown for comparison with the Skylab observations.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 40; Jan. 197
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  • 36
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    Publikationsdatum: 2011-08-16
    Beschreibung: An investigation is conducted of the full tidal problem for Mercury, Venus, Earth, and Jupiter, the tide-raising planets, taking into account the complete orbital elements, including eccentricity, inclination, and their variation with time. Data for a comparison of tidal and sunspot dates are listed in a table. The investigation shows that the alignment of the tide-raising planets within 10 degrees is a common phenomenon, occurring approximately every 10.4 years. This alignment is not associated with drastic tidal effects.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Nature; 253; Feb. 13
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  • 37
    Publikationsdatum: 2011-08-16
    Beschreibung: Results of a detailed analysis of solar activity in 1957-1965 are compared with the data on solar activity with variations of cosmic ray activity, and geomagnetic, ionospheric and terrestrial currents. Cosmic ray variations are investigated with reference to the asymmetry of solar hemispheres. All storms in the IGY are classified and a symbolic diagram of the time sequence is drawn up.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Cosmic Rays (; p 125-132
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  • 38
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    Publikationsdatum: 2011-08-16
    Beschreibung: The effects of solar radiation on the near space and biomental earth, the upper atmosphere, and the magnetosphere are discussed. Data obtained from the OSO satellites pertaining to the solar cycle variation of extreme ultraviolet (EUV) radiation are analyzed. The effects of solar cycle variation of the characteristics of the solar wind are examined. The fluid mechanics of shock waves and the specific relationship to the characteristics of solar shock waves are investigated. The solar and corpuscular heating of the upper atmosphere is reported based on the findings of the AEROS and NATE experiments. Seasonal variations of the upper atmosphere composition are plotted based on OGO-6 mass spectrometer data.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Significant Accomplishments in Sci. and Technol.; p 92-138
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  • 39
    Publikationsdatum: 2011-08-16
    Beschreibung: He II 304 A spectroheliograms, obtained with the NRL extreme-ultraviolet slitless spectrograph during the Skylab mission, show spikelike structures at the sun's polar limb which resemble the familiar H-alpha spicules. However, the relatively large size and long life of these He II features has led to distinguishing them by the name 'macrospicules'. The macrospicules appear as protuberances or jets, ranging from 5 to over 60 sec in length, from 5 to 30 sec in width, and from 5 to over 40 minutes in lifetime. Perhaps the most radical departure from H-alpha spicules is that macrospicules occur only within the chromospheric boundaries of coronal holes. Thus macrospicules are most easily visible over the solar poles due to the coronal holes normally present there, and much less frequently at lower latitudes during limb passage of relatively rare, low-latitude coronal holes.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 197; May 1
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  • 40
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    Publikationsdatum: 2011-08-16
    Beschreibung: The relationship between neutron monitor variations and the intensity variations of the interplanetary magnetic field is studied by using Deep River data and Imp series satellite data. In over 80% of the cases studied in 1968, identifiable depressions of the cosmic ray intensity are associated with magnetic field enhancements of several hours duration and intensity above 10 gamma. Conversely, almost every magnetic field enhancement has an identifiable effect (though not necessarily a marked depression) on the cosmic ray intensity. Perpendicular gradient drifts are suggested as one possible mechanism producing the individual decreases, and some ideas on the recovery processes are presented. Long-lasting Forbush decreases are found to be the consequence of the action of several successive magnetic field enhancements. Evidence is presented that indicates that most of these enhancements are caused by the steepening of streams in interplanetary space.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Journal of Geophysical Research; 80; Feb. 1
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  • 41
    Publikationsdatum: 2011-08-16
    Beschreibung: This paper presents particularly simple mathematical formulas for the calculation of force-free fields of constant alpha from the distribution of discrete sources on a flat surface. The advantage of these formulas lies in their physical simplicity and the fact that they can be easily used in practice to calculate the fields. The disadvantage is that they are limited to fields of 'sufficiently small alpha'. These formulas may be useful in the study of chromospheric magnetic fields by the comparison of high-resolution H-alpha photographs and photospheric magnetograms.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 45; Dec. 197
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  • 42
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    Publikationsdatum: 2011-08-16
    Beschreibung: It is shown, for a very simple model of the moon, that the existence of a primordial core magnetic field would give rise to a present day nonzero dipole external field. In the investigation a uniformly magnetized core embedded in a permeable mantle is considered. The significance of the obtained results for the conclusions reported by Runcorn (1975) is discussed. Comments provided by Runcorn to the discussion are also presented.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Nature; 258; Nov. 13
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  • 43
    Publikationsdatum: 2011-08-16
    Beschreibung: The spatial and temperature structures of the X-ray emitting components of low-inductance vacuum-spark plasmas are investigated. The plasmas produced by low-inductance vacuum sparks show striking resemblances to solar-flare plasmas. High-resolution photographs show that the spark plasmas are composed of hot (about 30 million K) compact sources (less than 20 microns) and cooler (about 10 million K) larger sources (of the order of 100 microns). Both types of sources may be produced by the same plasma at different times. The differences between the solar flare iron-line spectrum near 1.9 A and the spark iron-line spectrum are discussed and interpreted.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 201; Oct. 1
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  • 44
    Publikationsdatum: 2011-08-16
    Beschreibung: A model of a coronal region of enhanced Fe XV and Fe XVI emission is developed and its energy balance is examined using extreme ultraviolet observations from OSO-7 together with calculations of possible force-free coronal magnetic field configurations. The coronal emissions overlying the photospheric boundary between regions of opposite magnetic polarity are found to be associated with generally nonpotential (current-carrying) magnetic fields in the forms of arches with footpoints in regions of opposite polarity. The orientation of these arches relative to the neutral line changes with degree of ionization of the emitting ion (which we infer from our limb observations to be a function of height) and may be evidence of differing electric currents along various field lines. The appearance of a coronal arch, seen side-on, can conveniently be represented by a parabola and a detailed analysis shows this to be a realistic approximation that should be generally useful in analyzing two-dimensional pictures of coronal structures.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 43; Aug. 197
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  • 45
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    In:  CASI
    Publikationsdatum: 2012-05-22
    Beschreibung: The problems created by fretting in turbine engines are discussed. The areas of greatest wear identified with the fan, compressor, and turbine blade mountings being the most critical items. Various methods for reducing or eliminating fretting in a turbine engine are described. Vacuum deposition of coatings by sputtering and ion plating are recommended as an economic method of applying thin films to inhibit fretting.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: AGARD Specialists Meeting on Fretting in Aircraft Systems; 17 p
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  • 46
    Publikationsdatum: 2011-08-16
    Beschreibung: Expected wavelengths and relative intensities are obtained from previous calculations for the hitherto unobserved transitions 2p5 3p(1SO) - 2p5 3s(1P1, 3P1) in Fe XVII. A candidate pair of lines at 197.05 A and 242.09 A was found in laboratory spectra and appears to be present in the spectra of a solar active region observed by the OSO-7 Goddard spectroheliograph as well as in the spectrum of a Skylab-observed solar flare.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 43; July 197
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  • 47
    Publikationsdatum: 2011-08-16
    Beschreibung: The abundance of Fe relative to H is obtained by using resonantly scattered intensities of lambda 284 of Fe XV that were measured with OSO-7 and resonantly scattered intensities of L-alpha of H I that were obtained by Gabriel (1971). Because of possible differences in electron densities along lines of sight for these non-simultaneous measurements and in relative calibrations, results are rather uncertain but still indicate that the average Fe abundance relative to H in the corona appears to be at least as large as a recent photospheric abundance. Some limitations in using this method for obtaining abundances are examined for future experiments with simultaneous measurements and well calibrated detectors.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 42; June 197
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  • 48
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    Publikationsdatum: 2011-08-16
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 42; May 1975
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  • 49
    Publikationsdatum: 2011-08-16
    Beschreibung: If hydrogen and helium are immiscible below some critical temperature, gravitational separation could occur in the proto-sun, resulting in a nearly pure helium core and a nearly pure hydrogen shell. We have constructed solar models according to this scenario and find the neutrino flux reduced to 1.5-3 SNU.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 196; Mar. 1
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  • 50
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: Over 500 days of low-frequency (less than 1 MHz) radio observations from the IMP-6 spacecraft have been accumulated to produce a two-dimensional map (frequency vs elongation) of solar type III burst occurrences. This map indicates that most solar bursts in this frequency range are observed at the second harmonic of the plasma frequency, rather than the fundamental. The map also shows that the solar wind electron density varies as an inverse power of heliocentric distance, with the exponent somewhat less than 2 to perhaps 3 or higher.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 45; Nov. 197
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  • 51
    Publikationsdatum: 2011-08-16
    Beschreibung: The absorption spectrum of Si I in the wavelength region between 1500 and 1900 A has been photographed at high resolution. The silicon vapor was produced in a 122-cm-long King furnace at 1800 to 2300 C. Forty-two Rydberg series have been observed from the ground state terms 3p(2)3P and 1D to terms associated with the 3pns and 3pnd configurations. All of the series from these configurations with J less than 4 have been extended with the 3pnd 3D(3) levels reaching n = 56. Numerous perturbations have been observed. This laboratory work has provided the basis for extending the identification of silicon lines in the solar spectrum. Nearly all lines found in the laboratory spectrum are also found in rocket spectrograms of the solar chromosphere. More than 300 lines have been attributed to Si I. The excellent correlation between laboratory and solar Si I lines is illustrated.
    Schlagwort(e): SOLAR PHYSICS
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  • 52
    Publikationsdatum: 2011-08-16
    Beschreibung: Cinematographic observations of solar prominences made at Mauna Loa, Hawaii, during the past few years suggest that there is a well-defined subclass of ascending prominences characterized by closed-system transference of chromospheric material along an arch or loop (up one leg and down the other). While this occurs, the entire prominence envelope steadily rises upward and expands through the corona. These prominences are denoted as 'fountains'. Several examples are described. Fountains appear to be well contained by coronal magnetic fields. Their total kinetic energy is of the order of 10 to the 30th power erg, but dissipation is typically quite slow (over time periods of 100 min or so), so that the correlative disturbances (radio bursts, coronal transients, chromospheric brightenings) are generally not spectacular or nonexistent.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 44; Oct. 197
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  • 53
    Publikationsdatum: 2011-08-16
    Beschreibung: Solar limb-brightening curves are discussed for XUV spectral lines formed in the upper chromosphere and transition zone of a quiet region and a polar coronal hole. The spectra were recorded with a slit spectrograph on Skylab. The lines considered are emitted from ions formed within the temperature range from 10,000 to 220,000 K. The limb-brightening curves cover a region from -4 sec within the limb to +20 sec above it. The data from 0 sec to +20 sec are compared with predictions based on both homogeneous and inhomogeneous models of the transition zone. The limb-brightening curve of the O I line at 1355.6 A indicates that O I is formed in spicules. The limb brightening of the He II line at 1640.4 A is consistent with a temperature of formation between about 40,000 and 90,000 K for He II.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 202; Dec. 15
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  • 54
    Publikationsdatum: 2011-08-16
    Beschreibung: The intensities of XUV transition-zone lines from limb spectra of a quiet-sun region and a polar coronal hole are compared. The spectra were obtained with a slit spectrograph on Skylab and cover a region from -12 sec within the limb to 20 sec above it. The lines selected for comparison are formed at temperatures that range from 36,000 to 220,000 K. Lines of the higher-temperature ions, e.g. O v, are significantly less intense in the coronal hole, and lines of lower-temperature ions show little change. Profiles of selected optically thin transition-zone lines from the quiet-sun and coronal-hole spectra are also shown. The lines are broader than expected in ionization equilibrium, and bulk-motion velocities are deduced from the widths of the lines. There appears to be little, if any, statistically significant difference in the velocities obtained from the quiet-sun region and the coronal hole.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 202; Dec. 15
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  • 55
    Publikationsdatum: 2011-08-16
    Beschreibung: The spectral composition and spatial distribution of equatorial coronal emission near 304 A is examined. Spectral scans indicate that the predominant line is from Si XI. Comparisons of observations with calculations of intensity changes with altitude indicate that collisional excitation is important near the sun but that photoexcitation becomes dominant beyond about 1.3 solar radii from the solar center. Observed and calculated intensities are in approximate agreement for abundances and electron densities that are within the range of observed values.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 43; Aug. 197
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  • 56
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 201; Nov. 1
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  • 57
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: Interferometric observations at 17 GHz of several small X-ray flares are presented along with soft X-ray observations of preflare active regions to show that a large mass increase accompanies the formation of an X-ray hot region in the corona. The total amount of energy contained in a hot coronal region is estimated, and a model is proposed in which a significant amount of the hot matter is supplied to the corona from the chromosphere during each flare. According to this model, energy produced by some coronal instability is transported by thermal conduction to the chromosphere, where dense gas is heated and subsequently expands into the corona. It is shown that impulsive heating of the chromosphere by nonthermal electrons cannot be the energy source of this model because the total energy supplied to the hot region during the gradual phase must be much greater than that supplied during the impulsive phase.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 45; Dec. 197
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  • 58
    Publikationsdatum: 2012-05-22
    Beschreibung: Recently advanced simulation techniques have been developed for the digital computer and used as the basis for development of a generalized dynamic engine simulation computer program, called DYNGEN. This computer program can analyze the steady state and dynamic performance of many kinds of aircraft gas turbine engines. Without changes to the basic program, DYNGEN can analyze one- or two-spool turbofan engines. The user must supply appropriate component performance maps and design point information. Examples are presented to illustrate the capabilities of DYNGEN in the steady state and dynamic modes of operation. The analytical techniques used in DYNGEN are briefly discussed, and its accuracy is compared with a comparable simulation using the hybrid computer. The impact of DYNGEN and similar digital programs on future engine simulation philosophy is also discussed.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: AGARD Power Plant Controls for Aero-Gas Turbine Eng.; 23 p
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  • 59
    facet.materialart.
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    In:  Other Sources
    Publikationsdatum: 2016-06-07
    Beschreibung: Engine sealing programs are discussed which are directed toward the two major classes of engine seals: engine shaft seals and primary gas path seals. In addition, some concepts and results from fundamental lubrication research, as it pertains to the lubrication of bearings, are presented.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Aeron. Propulsion; p 305-327
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  • 60
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    In:  Other Sources
    Publikationsdatum: 2016-06-07
    Beschreibung: The JT8D Refan Program for noise reduction is outlined, and the overall objectives and program status, test results, and current noise level predictions are presented.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Aeron. Propulsion; p 81-97
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  • 61
    Publikationsdatum: 2016-06-07
    Beschreibung: The progress in propulsion system noise reduction is reviewed. The noise technology areas discussed include: fan noise; advances in suppression including conventional acoustic treatment, high Mach number inlets, and wing shielding; engine core noise; flap noise from both under-the-wing and over-the-wing powered-lift systems; supersonic jet noise suppression; and the NASA program in noise prediction.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Aeron. Propulsion; p 1-63
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  • 62
    Publikationsdatum: 2016-06-07
    Beschreibung: Some of the specific areas associated with straight jet and turboprop engine installations are outlined where drag reduction and, thus, improved aircraft system performance is obtained. Specific areas constitute air intake sizing for general aviation aircraft, exhaust duct geometries and cooling system arrangements for propeller powered aircraft.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Kansas Univ. Proc. of the NASA, Ind., Univ., Gen. Aviation Drag Reduction Workshop; p 245-256
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  • 63
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    In:  Other Sources
    Publikationsdatum: 2016-06-07
    Beschreibung: The NASA research on scramjet technology for speeds above Mach 5 is reported. A brief overview of the NASA Hypersonic Research Engine (HRE) project is presented with emphasis on the most significant contributions on the HRE to scramjet technology. The work on high-performance airframe-integrated scramjet engines is described, and a new versatile research airplane is discussed with emphasis on propulsion.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Aeron. Propulsion; p 459-474
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  • 64
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    In:  Other Sources
    Publikationsdatum: 2016-06-07
    Beschreibung: The recent developments and future potential of advanced materials for turbine components are described. The components discussed in detail are disks, blades, and vanes.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Aeron. Propulsion; p 209-288
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  • 65
    Publikationsdatum: 2016-06-07
    Beschreibung: Aircraft fuel consumption is discussed in terms of its efficient use, and the conversion of energy from sources other than petroleum. Topics discussed include: fuel from coal and oil shale, hydrogen deficiency of alternate sources, alternate fuels evaluation program, and future engines.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Aeron. Propulsion; p 157-190
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  • 66
    Publikationsdatum: 2016-06-07
    Beschreibung: The fundamental vortex theory for a single rotation propeller with a finite number of blades is reviewed. The theory leads to the specification of a radial distribution of bound circulation on each blade for minimum induced loss, analogous to the elliptic spanwise distribution of bound circulation on a wing for minimum induced drag. A propeller designed in accord with this theory has been tested in a water tunnel where it exhibited high efficiency in spite of localized cavitating flow. A knowledge of the flow field for an optimum propeller is of value to the airframe designer seeking to maximize the performance of the airplane-propeller combination.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Kansas Univ. Proc. of the NASA, Ind., Univ., Gen. Aviation Drag Reduction Workshop; p 273-293
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  • 67
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    Publikationsdatum: 2016-06-07
    Beschreibung: The Supersonic Cruise Airplane Research (SCAR) technology program is reported. Mission requirements, cycle considerations, engine evaluation, and SCAR test results are discussed. It is concluded that improved aerodynamics and structures, greater use of composites, and more-refined active controls are needed in the airframe area for designing an economically viable, environmental acceptable supersonic aircraft.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Aeron. Propulsion; p 441-457
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  • 68
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    In:  Other Sources
    Publikationsdatum: 2016-06-07
    Beschreibung: Current full-scale engine development programs are discussed, and efforts to improve the available technology base are presented. The Lewis full-scale engine test facilities are described. Several typical engine programs and plans for research in aeromechanical instability or flutter are summarized. An overview of Lewis studies of flow distortion and its effects on engine stability is presented. The origins and nature of the distortion problem are summarized, and some of the results and methods for both steady and time-varying distortions are discussed.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Aeron. Propulsion; p 329-385
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  • 69
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    In:  Other Sources
    Publikationsdatum: 2016-06-07
    Beschreibung: The composites research being conducted at Lewis for the application of composite materials to fan and compressor blades, is reviewed. The major areas discussed include the development of improved materials and fabrication methods, recent progress in providing composite fan and compressor blades with improved resistance to foreign object damage, and the development of advanced design and analysis procedures for composite blades.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Aeron. Propulsion; p 191-208
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  • 70
    facet.materialart.
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    Publikationsdatum: 2016-06-07
    Beschreibung: The objectives, scope, and status of the NASA Quiet, Clean, Short-Haul Experimental Engine program are reviewed. The progress reported is concerned with engine design concepts for short-haul aircraft where part of the engine thrust is used to help lift the aircraft. Both under-the-wing, and over-the-wing configurations are discussed.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Aeron. Propulsion; p 65-80
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  • 71
    facet.materialart.
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    In:  CASI
    Publikationsdatum: 2016-06-07
    Beschreibung: The environmental effects are discussed of engine effluents of future large fleets of aircraft operating in the stratosphere. Topics discussed include: atmospheric properties, aircraft engine effluents, upper atmospheric measurements, global air sampling, and data reduction and analysis
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Aeron. Propulsion; p 139-156
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  • 72
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    Publikationsdatum: 2016-06-07
    Beschreibung: The selection of components, control design, simulation, and tests are examined for designing supersonic propulsion systems. Inlet-engine combination under electronic control are shown. Design and test results from the integrated control for afterburning turbofan and supersonic cruise inlet are presented.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Aeron. Propulsion; p 387-440
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  • 73
    facet.materialart.
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    In:  Other Sources
    Publikationsdatum: 2016-06-07
    Beschreibung: The improved technology is discussed of engine main-shaft ball bearings, and spur gears in power transmission drive trains. Much of the technology can be applied to other ball and roller bearings, and to other spur and bevel gears throughout the engine, drive train, and accessory systems.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Aeron. Propulsion; p 289-303
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  • 74
    Publikationsdatum: 2016-06-07
    Beschreibung: Combustor development is discussed as it relates to emissions reduction. The nature of the aircraft pollution problem is examined along with the aircraft pollution standards that have been established by the Environmental Protection Agency. The effect of engine operating conditions on pollutant formation levels is shown, as well as how close present-day engines are to meeting the established standards. The magnitude of the emissions reductions required to meet these standards is indicated. The progress that has been made in evolving the needed emissions reduction technology is the main topic.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Aeron. Propulsion; p 99-137
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  • 75
    facet.materialart.
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    In:  CASI
    Publikationsdatum: 2016-06-07
    Beschreibung: Jet engine components are considered that influence propulsion system integration on the airframe and related aircraft drag areas. Emphasis is placed on high Mach number inlet geometries, boattailed nozzle configurations, propulsive wing installation, wing surface blowing lift, fuselage mounted nacelles, and thrust reversal.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: Kansas Univ. Proc. of the NASA, Ind., Univ., Gen. Aviation Drag Reduction Workshop; p 365-385
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  • 76
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    In:  CASI
    Publikationsdatum: 2019-06-28
    Beschreibung: The preliminary design of an engine which satisfies the requirements of a quiet, clean, general aviation turbofan (QCGAT) engine is described. Also an experimental program to demonstrate performance is suggested. The T700 QCGAT engine preliminary design indicates that it will radiate noise at the same level as an aircraft without engine noise, have exhaust emissions within the EPA 1981 Standards, have lower fuel consumption than is available in comparable size engines, and have sufficient life for five years between overhauls.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA-CR-164222 , R75AEG026-VOL-1
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  • 77
    Publikationsdatum: 2019-06-27
    Beschreibung: Results of tests conducted on preliminary design polymeric-composite fan blade for the under the wing (UTW) OCSEE engine are presented. During this phase of the program a total of 17preliminary OCSEE UTW composite fan blades were manufactured for various component tests including frequency characteristics, strain distribution, bench fatigue, dovetail pull, whirligig overspeed and whirligig impact. All tests were successfully completed with the exception of whirligig impact tests. Improvements in local impact capability are being evaluated for the OCSEE blade under other NASA and related programs.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA-CR-134846 , R75AEG411
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  • 78
    Publikationsdatum: 2019-06-27
    Beschreibung: Aft fan noise reduction techniques were investigated. The 1/3 octave band sound data were plotted with the following plots included: perceived noise level vs acoustic angle at 2 fan speeds; PWL vs frequency at 2 fan speeds; and sound pressure level vs frequency at 2 aft angles and 2 fan speeds. The source noise plots included: band pass filter sound pressure level vs acoustic angle at 2 fan speeds; and 2nd harmonic SPL acoustic angle at 2 fan speeds.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA-CR-134850 , R75AEG252-VOL-2
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  • 79
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    In:  CASI
    Publikationsdatum: 2019-06-27
    Beschreibung: High bypass geared turbofan engines and propulsion systems designed for short-haul passenger aircraft are described. The propulsion technology required for future externally blown flap aircraft with engines located both under the wing and over the wing is emphasized. The aerodynamic and mechanical preliminary design of the QCSEE under the wing 1.34 pressure ratio fan with variable blade pitch is presented. Design information is given for two pitch change actuation systems which will provide reverse thrust.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA-CR-134842 , R75AEG213
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  • 80
    Publikationsdatum: 2019-06-27
    Beschreibung: The viability of proposed bearing designs to operate at application conditions is described. Heat rejection variables were defined for the test conditions. Results indicate that there is potential for satisfactory operation of spherical roller bearing in the QCSEE main reduction gear application.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA-CR-134890
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  • 81
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    In:  CASI
    Publikationsdatum: 2019-06-27
    Beschreibung: A component pressure test was conducted on a F101 PFRT combustor to evaluate the emissions levels of this combustor design at selected under the wing and over the wing operating conditions for the quiet clean short haul experimental engine (QCSEE). Emissions reduction techniques were evaluated which included compressor discharge bleed and sector burning in the combustor. The results of this test were utilized to compare the expected QCSEE emissions levels with the emission goals of the QCSEE engine program.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA-CR-134916 , R75AEG449
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  • 82
    Publikationsdatum: 2019-06-27
    Beschreibung: The design and analysis of a composite fan blade for the under the wing (UTW) QCSEE is presented. The blade is designed for a variable pitch, 18 bladed rotor and is constructed from a hybrid composite combination of materials consisting of Kevlar-49, type AS graphite, boron, and S-glass fibers in a PR288 epoxy resin matrix. The blade has an attached platform which is constructed of AS-graphite, PR288 epoxy resin matrix and aluminum honeycomb. The blade is designed to satisfy aerostability and cyclic life and strength requirements with a light weight construction. The attached platform is designed for a fail-safe condition in that it is retainable by the blade, under centrifugal force loading, even in the event of blade to platform bond separation. Details of the blade design and the results of stress, vibration, and impact analysis are included.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA-CR-134840 , R75AEG278
    Format: application/pdf
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  • 83
    Publikationsdatum: 2019-06-27
    Beschreibung: The aerodynamic and mechanical preliminary design of the QCSEE over the wing 1.36 pressure ratio fan is presented. Design information is given for both the experimental and flight designs.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA-CR-134841 , R75AEG381
    Format: application/pdf
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  • 84
    Publikationsdatum: 2019-06-27
    Beschreibung: Tests of a twenty inch diameter, low tip speed, low pressure ratio fan which investigated aft fan noise reduction techniques are reported. The 1/3 octave band sound data are presented for all the configurations tested. The model data are presented on 17 foot arc and extrapolated to 200 foot sideline.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA-CR-134851 , R75AEG252-VOL-3
    Format: application/pdf
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  • 85
    Publikationsdatum: 2019-06-27
    Beschreibung: Tests of a 20 inch diameter, low tip speed, low pressure ratio fan which investigated aft fan noise reduction techniques are reported. These techniques included source noise reduction features of selection of vane-blade ratio to reduce second harmonic noise, spacing effects, and lowering the Mach number through a vane row. Aft suppression features investigated included porosity effects, variable depth treatment, and treatment regenerated flow noise. Initial results and selected comparisons are presented.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA-CR-134849 , R75AEG252-VOL-1
    Format: application/pdf
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  • 86
    facet.materialart.
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    In:  CASI
    Publikationsdatum: 2019-06-27
    Beschreibung: The use of leaning vanes for tone noise reduction was examined in terms of their application in a typical two-stage high pressure ratio fan. In particular for stages designed with outlet guide vanes and zero swirl between stages, leaning the vanes of the first stage stator was studied, since increasing the number of vanes and the gap between stages do not provide the desired advantage. It was shown that noise reduction at higher harmonics of blade passing frequency can be obtained by leaning the vanes.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA-CR-152134
    Format: application/pdf
    Standort Signatur Erwartet Verfügbarkeit
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  • 87
    Publikationsdatum: 2019-06-27
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 40; Feb. 197
    Format: text
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  • 88
    Publikationsdatum: 2019-06-27
    Beschreibung: Numerous mass ejections from the sun have been detected with orbiting coronagraphs. Here for the first time we document and discuss the direct association of a coronagraph observed mass ejection, which followed a 2B flare, with a large interplanetary shock wave disturbance observed at 1 AU. Estimates of the mass and energy content of the coronal disturbance are in reasonably good agreement with estimates of the mass and energy content of the solar wind disturbance at 1 AU. The energy estimates as well as the transit time of the disturbance are also in good agreement with numerical models of shock wave propagation in the solar wind.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 40; Feb. 197
    Format: text
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  • 89
    Publikationsdatum: 2019-06-27
    Beschreibung: The sector structure of the interplanetary magnetic field and the solar wind velocity at the sector boundaries are compared at separations of up to 0.3 AU, 50 deg in heliocentric longitude, and 7 deg in heliographic latitude, using data from Mariner 5 en route to Venus and from the near-earth Explorer 33, 34, and 35 satellites. The polarity pattern of the magnetic sectors is found to be very similar at the two locations, and 18 pairs of corresponding sector boundaries are identified. One-hour averages of solar wind velocities near the boundaries show that the velocities near earth exceed those measured by Mariner 5 by as much as 30%. Two possible explanations of the observed velocity differences are discussed: a preferential acceleration of sector boundaries with distance, possibly caused by stream-stream interactions; and a dependence of the solar wind velocity on heliographic latitude.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Journal of Geophysical Research; 80; Mar. 1
    Format: text
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  • 90
    facet.materialart.
    Unbekannt
    In:  CASI
    Publikationsdatum: 2019-06-27
    Beschreibung: A large-scale, three dimensional magnetic field in the interplanetary medium with an expected classical spiral pattern to zeroth order is discussed. Systematic and random deviations which are expected are treated. The sector structure which should be evident at high latitudes is examined. Interplanetary streams are discussed as determining the patterns of magnetic field intensity. It was proposed that the large-scale spiral field can induce a meridional flow which might alter the field geometry somewhat. The nonuniformities caused by streams will probably significantly influence the motion of solar and galactic particles. It was concluded that knowledge of the 3-dimensional field and its dynamical effects can be obtained by in situ measurements by a probe which goes over the sun's poles. Diagrams of the magnetic fields are given.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: NASA-TM-X-70983 , X-692-75-242
    Format: application/pdf
    Standort Signatur Erwartet Verfügbarkeit
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  • 91
    Publikationsdatum: 2019-06-27
    Beschreibung: The design of the 3 1/2-stage turbine is described, and the cold-air performance of the first stage, modified for axial inlet conditions, is presented. The performance of the modified single-stage turbine and of two comtemporary high-stage-loading-factor turbines is compared with that estimated with a reference prediction method.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA-TM-X-3289 , E-8354
    Format: application/pdf
    Standort Signatur Erwartet Verfügbarkeit
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  • 92
    Publikationsdatum: 2019-06-27
    Beschreibung: The measured effects of inlet pressure distortion on the internal flow temperatures and pressures of a TF30-P-3 afterburning turbofan engine are reported. Extensive inner-stage instrumentation combined with stepwise rotation of pressure distortion provided a high degree of circumferential resolution in the data. The steady-state spatial variation in pressures, temperature, and calculated flow velocity and the amplitude and extent of the distorted sectors are given. Data are presented for runs of 77 and 90 percent of low-speed-rotor design speed at pressure distortion levels two-thirds of that required to stall the engine. These data are compared with data taken at clean-inlet conditions. Results indicate that the inlet pressure distortion was quickly attenuated within the compressor, except at the hub of the low-pressure compressor. The distorted sectors also swirled and varied in extent as they passed through the engine. Average velocities within the compressor were about equal to the clean-inlet values.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA-TM-X-3267 , E-8206
    Format: application/pdf
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  • 93
    facet.materialart.
    Unbekannt
    In:  CASI
    Publikationsdatum: 2019-06-27
    Beschreibung: The current state of knowledge about the propagation of aircraft noise was reviewed. The literature on the subject is surveyed and methods for predicting the most important and best understood propagation effects are presented. Available empirical data are examined and the data's general validity is assessed. The methods used to determine the loss of acoustic energy due to uniform spherical spreading, absorption in a homogeneous atmosphere, and absorption due to ground cover are presented. A procedure for determining ground induced absorption as a function of elevation angle between source and receiver is recommended. Other factors that affect propagation, such as refraction and scattering due to turbulence, which were found to be less important for predicting the propagation of aircraft noise, are also evaluated.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA-TM-X-56033
    Format: application/pdf
    Standort Signatur Erwartet Verfügbarkeit
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  • 94
    facet.materialart.
    Unbekannt
    In:  CASI
    Publikationsdatum: 2019-06-27
    Beschreibung: Flow characteristics, such as quadrupole moments are examined in order to study generation of aerodynamic noise. The mean flow quantities are set in accordance with experimental data and the incompressible Navier-Stokes are solved numerically. Isolated downstream sections of a turbulent jet are modelled separately with the mean flow characteristics held constant in time. The flows are allowed to evolve until the fluctuating velocity components reach a statistically steady state. Cross section contour plots of the velocity components and the quadrupole moments at three different downstream positions are presented.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA-CR-132693 , REPT-53
    Format: application/pdf
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  • 95
    Publikationsdatum: 2019-06-27
    Beschreibung: The data reduction program used to analyze the performance of the Aerothermodynamic Integration Model is described. Routines to acquire, calibrate, and interpolate the test data, to calculate the axial components of the pressure area integrals and the skin function coefficients, and to report the raw data in engineering units are included along with routines to calculate flow conditions in the wind tunnel, inlet, combustor, and nozzle, and the overall engine performance. Various subroutines were modified and used to obtain species concentrations and transport properties in chemical equilibrium at each of the internal and external engine stations. It is recommended that future test plans include the configuration, calibration, and channel assignment data on a magnetic tape generated at the test site immediately before or after a test, and that the data reduction program be designed to operate in a batch environment.
    Schlagwort(e): AIRCRAFT PROPULSION AND POWER
    Materialart: NASA-CR-132656 , AIRESEARCH-AP-75-11502
    Format: application/pdf
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  • 96
    Publikationsdatum: 2019-06-27
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 43; Aug. 197
    Format: text
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  • 97
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    Unbekannt
    In:  Other Sources
    Publikationsdatum: 2019-06-27
    Beschreibung: The calculated chemical compositions of the gaseous and condensed phases in the primitive solar nebula are presented for both equilibrium and disequilibrium condensation. The implications for the compositions of individual solar-system bodies will be briefly discussed. Condensation from an otherwise solar-composition gas in which carbon is more abundant than oxygen is mentioned.
    Schlagwort(e): SOLAR PHYSICS
    Format: text
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  • 98
    facet.materialart.
    Unbekannt
    In:  Other Sources
    Publikationsdatum: 2019-06-27
    Beschreibung: EUV observations show many active region loops in lines formed at temperatures between 10,000 and 2,000,000 K. The brightest loops are associated with flux tubes leading to the umbrae of sunspots. It is shown that the high visibility of certain loops in transition region lines is due principally to a sharp radial decrease of temperature to chromospheric values toward the loop axis. The plasma density of these cool loops is not significantly greater than in the hot gas immediately surrounding it. Consequently, the internal gas pressure of the cool material is clearly lower. The hot material immediately surrounding the cool loops is generally denser than the external corona by a factor 3-4. When the active region is examined in coronal lines, this hot high pressure plasma shows up as loops that are generally parallel to the cool loops but significantly displaced laterally.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Solar Physics; 43; Aug. 197
    Format: text
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  • 99
    facet.materialart.
    Unbekannt
    In:  Other Sources
    Publikationsdatum: 2019-06-27
    Beschreibung: A detailed non-LTE analysis of solar CN spectra strongly suggest a revised carbon abundance for the sun. We recommend a value of log carbon abundance = 8.35 plus or minus 0.15 which is significantly lower than the presently accepted value of log carbon abundance = 8.55. This revision may have important consequences in astrophysics.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 202; Nov. 15
    Format: text
    Standort Signatur Erwartet Verfügbarkeit
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  • 100
    facet.materialart.
    Unbekannt
    In:  Other Sources
    Publikationsdatum: 2019-06-27
    Beschreibung: The time dependences of the 2.2- and 0.51-MeV gamma-ray lines from solar flares are calculated, and the results are compared with observations of the 1972 August 4 and 7 flares. The time lag between the nuclear reactions and the formation of these two lines is caused by capture of the neutrons and subsequent deceleration of the positrons and decay of the radioactive nuclei. Our main results are that the calculation is consistent with the observed rise of the 2.2-MeV line on August 4, and it does not require different time dependences for the accelerated protons and high-energy electrons in the flare region. The above lags can explain the delayed gamma-ray emission observed on August 7. Positrons of energies greater than about 10 MeV could be detected in interplanetary space following large solar flares.
    Schlagwort(e): SOLAR PHYSICS
    Materialart: Astrophysical Journal; 202; Dec. 1
    Format: text
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