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  • Chemistry  (10.579)
  • GEOPHYSICS  (2.921)
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  • SPACE RADIATION  (817)
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  • 1
    Publikationsdatum: 2006-01-11
    Beschreibung: The Apollo 17 biological cosmic ray experiment to determine the effect of heavy cosmic ray particles on the brain and eyes is reported. The pocket mouse was selected as the biological specimen for the experiment. The radiation monitors, animal autopsy and animal processing are described, and the radiation effects on the scalp, retina, and viscera are analyzed.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA. Johnson Space Center Apollo 17 Prelim. Sci. Rept.; 14 p
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  • 2
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    In:  CASI
    Publikationsdatum: 2006-01-11
    Beschreibung: The Apollo 17 infrared scanning radiometer (ISR) experiment for mapping lunar surface thermal emission is reported. The instrument, lunar surface coverage, and the data obtained are discussed.
    Schlagwort(e): GEOPHYSICS
    Materialart: Apollo 17 Prelim. Sci. Rept.; 6 p
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  • 3
    Publikationsdatum: 2006-01-11
    Beschreibung: The ultraviolet spectrometer (UVS) onboard the Apollo 17 orbiting spacecraft was used to measure emissions from the lunar atmosphere. The UVS and calibration are discussed along with the lunar atmosphere observations and lunar albedo measurements.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA. Johnson Space Center Apollo 17 Prelimin. Sci. Rept.; 10 p
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  • 4
    Publikationsdatum: 2006-01-11
    Beschreibung: The populations of interplanetary particles were studied by examining the energy spectra in a cosmic ray detector placed in the shade, facing away from the sun. Suprathermal ions of solar origin, and low-energy galactic cosmic rays are discussed.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA. Johnson Space Center Apollo 17 Prelim. Sci. Rept.; 5 p
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  • 5
    Publikationsdatum: 2006-01-11
    Beschreibung: Glass track detectors were exposed to cosmic rays on the moon from December 11 to 13, 1972, during a period of relatively quiet sun activity as inferred from satellite proton counters. From 80 to 400 keV/amu, the differential flux of heavy cosmic ray nuclei decreases roughly as E to the -2nd power; this result together with the greater flux from the solar than the antisolar direction identify these nuclei as solar in origin.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA. Johnson Space Center Apollo 17 Prelim. Sci. Rept.; 4 p
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  • 6
    Publikationsdatum: 2006-01-11
    Beschreibung: On the Apollo 17 mission, a miniature mass spectrometer, called the lunar atmospheric composition experiment (LACE), was carried to the moon as part of the Apollo lunar surface experiments package (ALSEP) to study the composition of and variation in the lunar atmosphere. The instrument was successfully deployed in the Taurus-Littrow valley with its entrance aperture oriented upward to intercept and measure the downward flux of gases at the lunar surface. Initial activation of the LACE instrument occurred on December 27, 1972, approximately 50 hr after sunset, and operation continued throughout the first lunar night. Sunrise brought a high background gas level and necessitated discontinuing operation during lunar daytime except for a brief check near noon. Near sunset, operation was resumed and continued throughout the night. This sequence was repeated for the second and third lunations.
    Schlagwort(e): GEOPHYSICS
    Materialart: NASA. Johnson Space Center Apollo 17 Prelim. Sci. Rept.; 9 p
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  • 7
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    In:  CASI
    Publikationsdatum: 2006-04-05
    Beschreibung: The behaviour of the nonthermal electrons created at the impulsive phase of flares has been deduced from the microwave impulsive bursts and hard X-ray burst by many researchers. There is almost no doubt of the emission mechanisms that radio emissions are due to gyrosynchrotron emission and hard X-rays are collisional bremsstrahlung. However, there remain three controversial problems. One is whether the emission sources of the microwave impulsive burst and hard X-ray burst are common or not. Another is whether the injection of the nonthermal electrons into the source is impulsive or continuous. The other is the relation among the nonthermal electrons, soft X-rays, EUV flash, H-alpha kernels, and white light flares. These three problems are not independent of each other.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA, Washington High Energy Phenomena on the Sun; p 179-187
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  • 8
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    In:  CASI
    Publikationsdatum: 2006-04-05
    Beschreibung: The production of solar flares by the reservoir of energy generated by sunspot magnetic fields is discussed. Electrons play an important part in the flare process since high energy electrons are responsible for X-ray and radio emission. The energy required in the form of protons trapped in sunspot magnetic fields to produce large solar flares is analyzed. A trigger mechanism is described where the particles can be rapidly dumped into the chromosphere when fast electrons are produced by Coulomb collisions and through pion production by the highest energy protons.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA, Washington High Energy Phenomena on the Sun; p 12-18
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  • 9
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    In:  CASI
    Publikationsdatum: 2006-04-02
    Beschreibung: Atmospheric electricity must be considered in the design, transportation, and operation of aerospace vehicles. The effect of the atmosphere as an insulator and conductor of high voltage electricity, at various atmospheric pressures, must also be considered. The vehicle can be protected as follows: (1) By insuring that all metallic sections are connected by electrical bonding so that the current flow from a lightning stroke is conducted over the skin without any gaps where sparking would occur or current would be carried inside; (2) by protecting buildings and other structures on the ground with a system of lightning rods and wires over the outside to carry the lightning stroke into the ground; (3) by providing a zone of protection for launch complexes; (4) by providing protection devices in critical circuits; (5) by using systems which have no single failure mode; and (6) by appropriate shielding of units sensitive to electromagnetic radiation.
    Schlagwort(e): GEOPHYSICS
    Materialart: Terrest. Environ. (Climatic) Criteria Guidelines for Use in Aerospace Vehicle Develop., 1973 Rev.; 28 p
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  • 10
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    In:  CASI
    Publikationsdatum: 2006-04-05
    Beschreibung: A brief summary of the symposium is presented along with an outlook for developments in solar physics.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA, Washington High Energy Phenomena on the Sun; p 625-630
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  • 11
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    In:  CASI
    Publikationsdatum: 2006-04-05
    Beschreibung: Meter-wave pulsations observed at Culgoora are discussed. The characteristics of recorded pulsation events are summarized.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA, Washington High Energy Phenomena on the Sun; p 589-593
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  • 12
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    In:  CASI
    Publikationsdatum: 2006-04-05
    Beschreibung: Consideration is given to whether the modulation of low energy solar cosmic ray nuclei between the sun and earth can be so extreme that the fluxes observed at 1 AU imply (1) that the cosmic ray energy density in the solar atmosphere is comparable to the thermal energy density, and/or (2) that the cosmic ray intensity is sufficient in the solar atmosphere to produce detectable fluxes of secondary particles such as low energy positrons. It was found that such large modulation is compatible with observations, provided that the modulation occurrence is confined within a solar envelope lying within approximately 0.2 to 0.3 AU of the sun. There is, however, no compelling observational evidence to require that the modulation is this large.
    Schlagwort(e): SPACE RADIATION
    Materialart: High Energy Phenomena on the Sun; p 418-438
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  • 13
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    In:  CASI
    Publikationsdatum: 2006-04-05
    Beschreibung: Type 3 solar bursts observed by OGO-5, below 600 kHz, were analyzed. Decay times were measured, and collisional decay times were computed for distances out to 1 AU. By fitting power functions to the computed and observed decay times, and using local plasma hypothesis, it was found that the ratio rho of computed observed values varies with heliocentric radial distance according to a power function rho = 3r to the 0.7th power, assuming fundamental emission, and rho = 2r to the 0.7th power, assuming second harmonic emission.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA, Washington High Energy Phenomena on the Sun; p 537-539
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  • 14
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    In:  CASI
    Publikationsdatum: 2006-04-05
    Beschreibung: Large solar flares produce intense soft X-ray emission, indicating the existence of high temperature plasmas that coexist in time with the plasmas responsible for the normally observed brightenings in H-alpha. The time behavior of the X-ray flux, as revealed, for example, by ion chamber detectors on the series of Solrad monitoring satellites, appears to roughly mimic the intensity-time behavior of the H-alpha flare, insofar as start times, times of maximum flux, and approximate decay times are concerned. In recent years, soft X-ray spectra of both active regions and solar flares have been obtained by instruments flown on spacecraft such as the Orbiting Solar Observatory (OSO) series. The disbursing elements used were Bragg crystals, and in the 8 Angstrom region the resolution is typically approximately 1200. This paper discusses the observed characteristics of X-ray flare spectra and spectroscopic diagnostics for determining electron temperatures, electron densities, and departures from ionization equilibrium within the soft X-ray emitting plasma.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA, Washington High Energy Phenomena on the Sun; p 262-275
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  • 15
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    In:  CASI
    Publikationsdatum: 2006-04-05
    Beschreibung: The theory of solar microwave bursts is discussed in terms of gyrosynchrotron emission and absorption in a magnetoactive plasma and other absorption processes by the background medium. Simplified formulas for all turnover frequencies are given. Above about 2 GHz the most likely absorption processes for large bursts are free-free absorption and gyrosynchrotron self-absorption. The former process is capable of producing flux densities which are flat or slowly varying functions of frequency. The latter process sets absolute upper limits on the intensities of microwave bursts, which at a given frequency, depend only on the magnetic field in the source region.
    Schlagwort(e): SPACE RADIATION
    Materialart: High Energy Phenomena on the Sun; p 188-197
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  • 16
    Publikationsdatum: 2006-02-22
    Beschreibung: Energetic protons injected into interplanetary space in solar particle events can interfere with spacecraft operations and experiments and can cause permanent degradation of some components. For future long term interplanetary and planetary missions, techniques were developed which use solar particle event data from 1956 through 1970 to predict the probability of exceeding any value of peak proton intensity or mission proton fluence. Dependences on proton energy (near 10 to 100 MeV), heliocentric distance, and phase of the solar cycle are included. The techniques are described and applied to the Mariner Jupiter/Saturn 1977 mission.
    Schlagwort(e): SPACE RADIATION
    Materialart: JPL Quart. Tech. Rev., Vol. 3, No. 2 (NASA-CR-133863); p 37-44
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  • 17
    Publikationsdatum: 2006-01-11
    Beschreibung: The Apollo 17 biostack experiment to establish the biological efficiency of individual heavy nuclei particles of galactic cosmic radiation are reported. The experiment theory, interaction of heavy nuclei particles with biologic matter, and the total dose of cosmic ionizing radiation are discussed along with the radiation effects of heavy nuclei on Artemia salina eggs, and Bacillus subtilis.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA. Johnson Space Center Apollo 17 Prelim. Sci. Rept.; 10 p
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  • 18
    Publikationsdatum: 2006-01-11
    Beschreibung: Preliminary results are presented of data on the extent of the cosmic ray-induced activity obtained by a sodium iodide thallium-activated crystal flown onboard the Apollo 17 command module. Qualitative identification is reported for the following: Na-24, I-123, I-124, I-125, I-126, and Xe-127.
    Schlagwort(e): SPACE RADIATION
    Materialart: Apollo 17 Prelim. Sci. Rept.; 4 p
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  • 19
    Publikationsdatum: 2006-01-11
    Beschreibung: The lunar surface cosmic ray experiment, consisting of sets of mica, glass, plastic, and metal foil detectors, was successfully deployed on the Apollo 17 mission. One set of detectors was exposed directly to sunlight and another set was placed in shade. Preliminary scanning of the mica detectors shows the expected registration of heavy solar wind ions in the sample exposed directly to the sun. The initial results indicate a depletion of very-heavy solar wind ions. The effect is probably not real but is caused by scanning inefficiencies. Despite the lack of any pronounced solar activity, energetic heavy particles with energies extending to 1 MeV/nucleon were observed. Equal track densities of approximately 6000 tracks/cm sq 0.5 microns in length were measured in mica samples exposed in both sunlight and shade.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA. Johnson Space Center Apollo 17 Prelim. Sci. Rept.; 9 p
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  • 20
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    In:  CASI
    Publikationsdatum: 2006-04-05
    Beschreibung: Curves of the number of type 3 bursts as a function of time are presented for six fixed frequencies (2.8, 1.65, 1.31, 0.995, 0.700, and 0.54 MHz). The curves peak at approximately 0500 UT August 20, 1968, and are symmetrical on both sides. Sakurai (1971) has shown that this time correlates well with the CMP of the McMath Region 9597. The maximum rate of bursts is approximately 150 per hour at the higher frequency of 2.8 MHz. Over 20,000 bursts were counted during the 15-day period from August 13 to August 27 when the active region was visible to the earth. A least-squares normal curve has been fitted to the observational data and calculations of variance and standard deviation are given.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA, Washington High Energy Phenomena on the Sun; p 552-557
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  • 21
    Publikationsdatum: 2006-04-05
    Beschreibung: The propagation in the corona of the magnetohydrodynamic (MHD) disturbance possibly emitted at the explosive stage in the initial phase of a flare is considered. The behavior of the MHD fast-mode wavefront, whose source is located at the flare, is calculated by using eiconal-characteristic method in the High Altitude Observatory (HAO) realistic models of coronal magnetic field and density for the days of some particular flare events. It is shown as the result that the peculiar behavior of Moreton's surface wave and the peculiar appearance in the shape and position of the type 2 burst sources can be consistently understood by considering the refraction, focussing, and formation of shocks of MHD fast-mode disturbance in the actual distribution of Alfven velocity in the corona. Moreton waves seem to appear only when the flare explosion happens to occur at the edge of an active region and faces a low-Alfven-velocity region lying on the surface. The wave, which is initially emitted isotropically is refracted into a direction in which the condition for down-refraction holds to allow chromospheric reentrance of disturbance.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA, Washington High Energy Phenomena on the Sun; p 577-588
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  • 22
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    In:  CASI
    Publikationsdatum: 2006-04-05
    Beschreibung: The use of solar flare models based on specific and detailed observations of solar flares is discussed. A process for determining the validity of various solar models is analyzed. The process relegates the infall-impact model for flares to a secondary role in high energy solar events. The strictly thermal infall-impact model cannot lead to temperatures greater than five million degrees K. Another process is needed to explain the high energy aspects of solar flares which are related to temperatures equal to or greater than 10 to the 7th power degrees K, nonthermal X-ray and radio emissions, white light flares, high energy particles from the sun, and gamma ray producing particles in the sun.
    Schlagwort(e): SPACE RADIATION
    Materialart: High Energy Phenomena on the Sun; p 19-25
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  • 23
    Publikationsdatum: 2006-04-02
    Beschreibung: Earth viewing space missions offer exciting new possibilities in several earth resources disciplines - geography, hydrology, agriculture, geology, and oceanography, to name a few. A most useful tool in planning experiments and applying space technology to earth observation is a statistical description of atmospheric parameters. Four dimensional atmospheric models and a world wide cloud model are used to produce atmospheric attenuation models to predict degradation effects for all classes of sensors for application to earth sensing experiments from spaceborne platforms. To insure maximum utility and application of these products, the development of an interaction model of microwave energy and atmospheric variables provides a complete description of the effects of atmospheric moisture upon microwaves.
    Schlagwort(e): GEOPHYSICS
    Materialart: Terrest. Environ. (Climatic) Criteria Guidelines for Use in Aerospace Vehicle Develop., 1973 Rev.; 21 p
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  • 24
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    In:  CASI
    Publikationsdatum: 2006-03-27
    Beschreibung: The differenced range versus integrated Doppler (DRVID) technique was used to study charged particle changes in the ray path between earth and Mariner 9. For plasma activity near the sun, DRVID data were obtained from August 10 to October 24, 1972, surrounding the Mariner 9 superior conjunction on September 7. If the records are viewed in terms of range change or range change rate, the day-to-day fluctuations in these quantities mask the changes expected due to the varying solar elongation. Thus, while the steady-state total electron content varies by a factor of 4, the columnar content changes show no systematic variations.
    Schlagwort(e): SPACE RADIATION
    Materialart: Mariner Mars 1971 Proj., Vol. 4; p 471-472
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  • 25
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: An elastic plate model is used to describe the origin of intermediate and deep earthquakes. It is shown that the earth is covered by about eight tectonic plates that have relative motions; along plate boundary lines, one plate thrusting under the other, causes deflection and buckling of the elastic plate structure in regions of maximum curvature that may trigger earthquakes.
    Schlagwort(e): GEOPHYSICS
    Materialart: Significant Accomplishments in Sci.; p 220-223
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  • 26
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: Tracking of the Beacon Explorer-C satellite by a precision laser system was used to measure the polar motion and solid earth tide. The tidal perturbation of satellite latitude is plotted as variation in maximum latitude in seconds of arc on earth's surface as a function of the date, and polar motion is shown by plotting the variation in latitude of the laser in seconds of arc along the earth's surface as a function of date
    Schlagwort(e): GEOPHYSICS
    Materialart: Significant Accomplishments in Sci.; p 216-219
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  • 27
    Publikationsdatum: 2006-03-26
    Beschreibung: A computer program was developed for the calculation of a goid based upon a combination of satellite and surface gravity data. A detailed gravimetric geoid of North America, the North Atlantic, Eurasia, and Australia was derived by using this program.
    Schlagwort(e): GEOPHYSICS
    Materialart: Significant Accomplishments in Sci.; p 212-215
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  • 28
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: Satellite applications in earth and ocean dynamic studies are considered for: earthquake hazard assessment and alleviation; prediction of general ocean circulation, surface currents, and heat transport; monitoring of transient phenomena of the ocean surface, such as sea state and wave conditions, wind-surface interactions and storm searches; and refinement of the global geoid, the gravity and magnetic fields of the earth.
    Schlagwort(e): GEOPHYSICS
    Materialart: Significant Accomplishments in Sci.; p 211
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  • 29
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: Diurnal temperature variations in the upper atmosphere are caused by heating resulting from the absorption of solar energy by ozone near the stratopause and by water vapor in the troposphere. Theoretical temperature variations given as a function of time and height show a discrepancy for the maximum temperature variation. A comprehensive set of acoustic grande soundings establish phase changes with altitude in agreement with the theory although times of maximum and minimum are not aligned at all altitudes.
    Schlagwort(e): GEOPHYSICS
    Materialart: Significant Accomplishments in Sci.; p 205-208
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  • 30
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: Atmospheric radiation models and methods of computing radiation effects are reported that are important both in the meteorological and Earth Resources Satellite programs. Results of using them to compute the atmospheric effects on just the ERTS observations are presented.
    Schlagwort(e): GEOPHYSICS
    Materialart: Significant Accomplishments in Sci.; p 193-195
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  • 31
    Publikationsdatum: 2006-03-26
    Beschreibung: Medium resolution infrared radiometer observations at the 6.7 micrometer and the 11 micrometer regions by satellite during the maximum intensification phase of hurricane Camille show increasing black body temperatures near the center. This is attributed to increased upward vertical motion in the interior of the cyclone, which is an indication of rapid intensification.
    Schlagwort(e): GEOPHYSICS
    Materialart: Significant Accomplishments in Sci.; p 196-200
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  • 32
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: Spectral signatures of phytoplankton and other obscuring effects are considered in order to determine how to best use satellite data. The results of this study were then used to analyze the spectral data obtained from the ERTS-1 multispectral scanner (MSS). The analyzed satellite data were finally compared with surface ship measurements of chlorophyll concentration. It was found that the effects of water turbidity on the multispectral imagery can be discriminated by rationing the two shortest wavelength channels so that the effect of phytoplankton is enhanced.
    Schlagwort(e): GEOPHYSICS
    Materialart: Significant Accomplishments in Sci.; p 190-192
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  • 33
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: Remote sensing by ERTS-1 provides overlapping coverage on sequential days of dynamic changes in Arctic Sea ice and allows for route planning of shipping in the polar region.
    Schlagwort(e): GEOPHYSICS
    Materialart: Significant Accomplishments in Sci.; p 182-186
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  • 34
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: The applicability of multispectral ERTS-1 imagery to polar ice detection, local current effects, map corrections, relative lake depth measurements, and estimates of ice breakup is discussed.
    Schlagwort(e): GEOPHYSICS
    Materialart: Significant Accomplishments in Sci.; p 178-181
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  • 35
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    Publikationsdatum: 2006-03-26
    Beschreibung: An overview is given of research and development activities at the Laboratory for Meteorology and Earth Sciences. Highlights of satellite techniques in earth observation missions and projects are outlined, as are remote sensing methods by aircraft overflights; most noteworthy among these is the development of multispectral scanners that monitor both the reflected infrared solar radiation and the emitted terrestrial radiation. The application of observations to the survey of environmental conditions and resource management is emphasized.
    Schlagwort(e): GEOPHYSICS
    Materialart: Significant Accomplishments in Sci.; p 161-177
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  • 36
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: Lunar gamma ray spectra obtained during Apollo-15 and -16 flights show a natural radioactivity due to potassium, thorium, and uranium as well as a cosmic ray induced activity in the lunar surface due to high neutron interactions produced by (p,n) reaction in the lunar surface. The radioactivity is at a low in the highlands on the backside of the moon; most of the radioactivity is confined to the Oceanus Procellarum/Mare Imbrium region and to the Van de Graff area on the lunar backside.
    Schlagwort(e): SPACE RADIATION
    Materialart: Significant Accomplishments in Sci.; p 132-135
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  • 37
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: Aluminum/silicon and magnesium/silicon concentration measurements along Apollo-15 and -16 lunar groundtracks by X-rays show that the highlands are very rich in aluminum, and that mare basalts cover large areas.
    Schlagwort(e): SPACE RADIATION
    Materialart: Significant Accomplishments in Sci.; p 127-131
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  • 38
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: Spectrometric scans of faint optical emissions from interstellar gas are reported. Systematic variations along the galactic plane in both the intensity and radial velocity of the galactic H alpha suggest that the diffuse emission is strongly associated with three nearby galactic spiral arms.
    Schlagwort(e): SPACE RADIATION
    Materialart: Significant Accomplishments in Sci.; p 88-91
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  • 39
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: Scientific goals and the instrumentation package for the OSO-K/solar flare mission are reported. The problem of determining origin and energetics of solar flares is considered.
    Schlagwort(e): SPACE RADIATION
    Materialart: Significant Accomplishments in Sci.; p 63-68
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  • 40
    Publikationsdatum: 2006-03-26
    Beschreibung: Soft X-ray and hydrogen alpha observations on the structure of a solar flare show the typical flare behavior - a rapid rise to maximum and a gradual exponential decay, with good time correlation between the soft X-rays and H alpha. The emission is identified by Fe XI ion, and the emitting region is contoured on EUV maps.
    Schlagwort(e): SPACE RADIATION
    Materialart: Significant Accomplishments in Sci.; p 54-57
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  • 41
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: The mechanism responsible for the modulation of synchrotron radiation in the meter wave range by a solar flare is examined. The proposed explanation is based on the interaction of a flare generated shock front with a magnetic flux tube extending out into the corona over the flare. As the shock wave propagates through the flux tube, Alfven waves are developing and travelling up the tube toward each other, thereby accelerating electrons and protons by the Fermi mechanism and thus filling the top of the flux tube with energetic electrons. Radial oscillations develop as the shock front becomes parallel to the magnetic field direction and the intensity of the synchrotron radiation is modulated by these oscillations. An OSO-5 experiment detected a hard X-ray burst associated with the flare that produced modulated radio emission and X-ray modulations that are attributed to density fluctuations in the X-ray bursts.
    Schlagwort(e): SPACE RADIATION
    Materialart: Significant Accomplishments in Sci.; p 49-53
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  • 42
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: The structure of an isolated solar flare point observed by vacuum telescope and multichannel spectrophotometer is considered. The tiny bright spot in H alpha photos lasted less than 30 seconds and coincided with a Type-III solar burst; a soft X-ray burst peaked at the time of this event. The small scale structure of the flare point exhibited in miniature the characteristics of a true flare event.
    Schlagwort(e): SPACE RADIATION
    Materialart: Significant Accomplishments in Sci.; p 58-62
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  • 43
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: Solid state low-energy telescopic observations on solar and galactic cosmic rays from 2 AU outward by satellites are evaluated. Plots of solar events leading to large injections of particles from the sun show that low energy slower protons arrive first by many hours before the higher energy protons, and that the higher energy particles are falling off more rapidly.
    Schlagwort(e): SPACE RADIATION
    Materialart: Significant Accomplishments in Sci.; p 38-44
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  • 44
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: Variation of the cosmic ray intensity as a function away from the sun and its radial derivative is studied by plotting satellite cosmic ray measurements against sea level neutron monitor data. Results show that the solar modulation cavity extends well beyond 2 AU and that irregularities in the sun's magnetic field are carried outward radially by the solar wind, thus sweeping low energy cosmic rays out of the solar system and at the same time cooling cosmic rays reaching the earth.
    Schlagwort(e): SPACE RADIATION
    Materialart: Significant Accomplishments in Sci.; p 45-48
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  • 45
    Publikationsdatum: 2006-03-26
    Beschreibung: Cosmic ray electron measurements by individual threshold detector elements show that about 30 percent of observed electron-like galactic cosmic showers are really proton initiated events. The cosmic electron spectrum at about 10 GeV exhibits a consistent dropoff in intensity leading to a best fit at a power law of spectral index -3.2; a break in the spectrum should occur above 10 GeV.
    Schlagwort(e): SPACE RADIATION
    Materialart: Significant Accomplishments in Sci.; p 24-28
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  • 46
    Publikationsdatum: 2006-03-26
    Beschreibung: Explorer satellite observations of modulations in the cosmic ray spectrum during the entire period of the solar cycle show intensity variations in the proton and alpha modulated spectra. A positive correlation between plasma density and variation in cosmic ray intensity is found that breaks during the transition period when higher energy intensity is decreasing as the solar activity increases. It is suggested that the alpha particles lead the proton particles during transition periods and thus make the lag time shorter for high rigidity near the solar maximum and the solar minimum.
    Schlagwort(e): SPACE RADIATION
    Materialart: Significant Accomplishments in Sci.; p 34-37
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  • 47
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: Observations of a quiet-time interplanetary electron component in the 20 keV to 2 MeV energy range are reported. The measurements fill in the gap between the highest-energy known solar wind and the lowest-energy previously observed electron populations, and connect for the first time the entire solar-quiet interplanetary electron spectrum over a dynamic range of nearly 10 to the 12th power in energy.
    Schlagwort(e): SPACE RADIATION
    Materialart: Significant Accomplishments in Sci.; p 29-33
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  • 48
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: A theoretical model in the form of a three-dimensional Monte Carlo calculation is developed that starts with known cosmic ray flux at the top of the atmosphere and follows particles as they interact with the atmosphere for a schematic representation of how atmospheric secondary gamma rays are produced. The model predicts atmospheric secondary gamma radiation as a function of altitude, energy, and zenith angle.
    Schlagwort(e): SPACE RADIATION
    Materialart: Significant Accomplishments in Sci.; p 16-19
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  • 49
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: Charge and particle trajectory measurements during a balloon-borne experiment observing the composition of cosmic rays, are interpreted by plotting differential intensities of various nuclei of both primary and secondary origin above 3 GeV/nucleon. The large spectral difference between carbon plus oxygen and iron is confirmed in the difference between their secondary products. This large difference cannot be explained as being solely due to propagation effects and it is concluded that preferential acceleration of heavy nuclei due to a source effect is present.
    Schlagwort(e): SPACE RADIATION
    Materialart: Significant Accomplishments in Sci.; p 20-23
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  • 50
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    In:  CASI
    Publikationsdatum: 2006-03-26
    Beschreibung: Balloon observations of a low energy flux line at 2 x 0.001 photons cm/2 s/1 from the galactic center region around 470 keV are interpreted as the positron annihilation radiation that occurs on the surface of old neutron stars and is redshifted by their gravitational fields. An astrophysical model is formulated to explain the observed flux that provides for about 0.2 neutron stars per 3 x 10 to the 49th power cubic meters assuming that the disk thickness is about 1.5 x 10 to the 19th power meters.
    Schlagwort(e): SPACE RADIATION
    Materialart: Significant Accomplishments in Sci.; p 9-11
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  • 51
    Publikationsdatum: 2006-04-05
    Beschreibung: In two recent papers it was shown that the metric type 3 emission is closely related to a transient perturbation seen in absorption in the H alpha line. In addition, this perturbation sometimes triggers a flare, sometimes not. This can explain why the type 3 have a poor H alpha flare correlation rate and still are a typical flash phase emission when flare-associated. The characteristics are summarized of the new association proposed. It is assumed that 10 to 100 keV electrons are accelerated in connection with a particular kind of transient H alpha absorbing feature. For as yet undetermined reasons, this process would often, but not always, result in a more efficient acceleration coincident with the early phase of the optical flare. The possibilities that this process could lead occasionally to long lasting subrelativistic particle emissive region are explored.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA, Washington High Energy Phenomena on the Sun; p 615-622
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  • 52
    Publikationsdatum: 2006-04-05
    Beschreibung: The following new hypothesis is proposed. The decay time of plasma waves is much shorter than the time scale of type 3 bursts especially at low frequencies. Accordingly, the time variation of radio flux at a given frequency merely corresponds to the flux of fast electrons passing through the corresponding plasma layer.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA, Washington High Energy Phenomena on the Sun; p 573-576
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  • 53
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    In:  CASI
    Publikationsdatum: 2006-04-05
    Beschreibung: The present state of the theory of type 3 bursts is reviewed by dividing the problem into the exciting agency, radiation source, and propagation of radiation between the source and the observer. In-situ measurements indicate that the excitors are electron streams of energy about 40 keV which are continuously relaxing. An investigation of neutralization of an electron stream indicates that n sub s is much less than 100,000 n sub e, where n sub s is the stream density and n sub e the coronal electron density. In situ observations are consistent with this result. An analysis of propagation of electrons in the current sheets of coronal streamers shows that such propagation at heights greater than 1 solar radius is impossible. The mechanisms for radiation are reviewed; it is shown that fundamental radiation at high frequencies (approximately 100 MHz) is highly beamed in the radial direction and that near the earth second harmonic radiation must be dominant. Because of beaming of the fundamental at high frequencies, it can often be quite weak near the limb so that the second harmonic is dominant. In considering propagation to the observer, the results of scattering of radiation are discussed. The present state of the theory of type 2 bursts is reviewed in the same manner as type 3 bursts.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA, Washington High Energy Phenomena on the Sun; p 558-572
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  • 54
    Publikationsdatum: 2006-04-05
    Beschreibung: Analysis of data from the soft X-ray proportional counter spectrometer on OSO-4 has been continued along the lines of earlier work. It was noticed that the time profiles of X-ray counts from the OSO-4 instrument's 1 to 3 Angstrom detectors for two events showed a very rapid initial decay after maximum, followed by a much more slowly falling section. At least in the case of the larger of the two events, the change of slope seems quite definitely to be discontinuous. Temperatures and emission measures for both flares have been derived, by fitting an emission function to eight-channel count histograms which form the output of the 1 to 3 Angstrom detectors, analyzed into eight energy intervals by pulse-height analysis. The computer program is described. It employs temperature and continuum emission measures in the Culhane-Acton formula and the flux in the 6.7 KeV iron-line feature as free parameters, adjusting them by small amounts in successive iterations until the original historgram is approximately reproduced. A chi-squared is used to examine the agreement between histograms and terminates the iteration accordingly. Account is taken of the proportional counters' energy resolution in the fitting process.
    Schlagwort(e): SPACE RADIATION
    Materialart: High Energy phenomena on the Sun; p 276-282
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  • 55
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    In:  CASI
    Publikationsdatum: 2006-04-05
    Beschreibung: The theory of gamma-ray line emission from solar flares is reviewed and revised. It is shown that the line emissions at 0.5, 2.2, 4.4, and 6.1 MeV are due to positron annihilation, deuterium deexcitation following neutron capture on hydrogen, and the deexcitation of excited states in carbon and oxygen. From the observed relative line intensities it is possible to determine the spectrum of accelerated protons in the flare region. This spectrum is found to be very similar to that of charged particles from the flare observed near earth. The total number of protons at the sun is deduced from the observed absolute line intensities for various interaction models.
    Schlagwort(e): SPACE RADIATION
    Materialart: High Energy Phenomena on the Sun; p 301-314
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  • 56
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Schlagwort(e): SPACE RADIATION
    Materialart: Nature Physical Science; 246; Dec
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  • 57
    Publikationsdatum: 2011-08-16
    Beschreibung: A series of solar flares accompanying type II and type IV radio bursts were observed while the active region McMath No. 9740 was on the solar disk. Most of these flares were also associated with solar cosmic rays and SSC geomagnetic storms. The expansion pattern of these disturbances near the earth's orbit is considered. This pattern appears to be useful for studying the propagation of interplanetary shock waves which are generated by solar flares.
    Schlagwort(e): SPACE RADIATION
    Materialart: Nature Physical Science; 246; Dec. 3
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  • 58
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: A review is presented of theories and observations of current sheets in the magnetosphere, emphasizing the magnetopause and tail current sheets. Theoretical models of the magnetopause current sheet can be divided into two types: specular reflection and fluid models containing no external magnetic field, and models with an interplanetary/magnetosheath magnetic field. Our understanding of the first type is much better than of the second, although magnetospheric observations indicate that the external magnetic field plays an important role. Most of the theoretical models of the tail current sheet attempt to arrive at an understanding of the reconnection process or start with the assumption that reconnection is important. Observations are reviewed and implications for the models are discussed.
    Schlagwort(e): GEOPHYSICS
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  • 59
    Publikationsdatum: 2011-08-16
    Beschreibung: Individual particles were analyzed on the collection screens in a Jeolco scanning electron microscope using a Kevex Li-drifted silicon energy dispersive X ray detector. It was found that the bulk of the stratospheric samples studied comes from explosive squib devices. It is pointed out that this finding does not invalidate the extensive results obtained by Bigg et al. (1970, 1971) in previous sampling experiments.
    Schlagwort(e): SPACE RADIATION
    Materialart: Journal of Geophysical Research; 78; Nov. 20
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  • 60
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Schlagwort(e): GEOPHYSICS
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  • 61
    Publikationsdatum: 2011-08-16
    Beschreibung: It is shown that the fields of velocity, eddy viscosity, potential temperature, and specific humidity in a planetary boundary layer are decoupled by the introduction of a free parameter, Q, which combines the effects of thermal and humidity stratification. Solutions of the whole system are shown to be obtainable by the method of trial and error on Q. Results show good agreement when both the thermal and humidity stratification are accounted for.
    Schlagwort(e): GEOPHYSICS
    Materialart: Monthly Weather Review; 101; Aug. 197
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  • 62
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: The expected flux of K alpha line emission from sulfur, argon, calcium, and iron is calculated during both thermal and nonthermal solar X-ray events. Such emission is shown to be weak during the course of most of the nonthermal hard X-ray bursts that Kane and Anderson (1970) have observed. If Compton backscattering is significant at high energies, the flux is reduced still further for disk flares, but it is noted that the strong, near-limb burst of June 26 would have produced about 100 photons /sq cm/sec of sulfur and iron K alpha emission. The impulsive hard X-ray bursts may in general be too short-lived for much K alpha emission. It may be noted that sulfur K alpha emission in particular depends sensitively on the lower-energy limit of the nonthermal electron spectrum, assuming such a sharply defined boundary exists. During soft X-ray bursts, when temperatures of a few 10 to the 7th power K are obtained, K alpha emission from certain iron ions, specifically Fe XVIII-XXIII, may be important.
    Schlagwort(e): SPACE RADIATION
    Materialart: Solar Physics; 32; Sept
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  • 63
    Publikationsdatum: 2011-08-16
    Beschreibung: The stability of the low-frequency waves propagating transverse to the magnetic field of a plasma composed of electrons, protons, and alpha particles with anisotropic electron and ion temperatures is explored. The threshold for the ordinary mode instability and the growth rates have a very strong dependence on the electron temperature anisotropy but have a comparatively weaker dependence on the ion temperature anisotropy, on the relative abundance of helium to hydrogen, and on the relative streaming of two ion species. The threshold for the instability of these low-frequency waves is (m sub e/m sub p) to the 1/2 power times smaller than the one corresponding to high-frequency waves; however, for a relative abundance of helium to hydrogen up to 20% for the relevant known magnetic fields, particle densities, temperatures, and drifts, the solar wind remains below the threshold for this instability.
    Schlagwort(e): SPACE RADIATION
    Materialart: Journal of Geophysical Research; 78; Dec. 1
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  • 64
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: Review of the magnetospheric morphology, using the method of the Delta B topology, where Delta B is the difference between the observed and a reference field. It is confirmed that Delta B continuously decreases inward to close distances from the earth at all local times. Extrapolating the statistical relation between Dst at the ground and the equatorial Delta B obtained from OGO-5 near perigee, it is shown that Dst is 54 gammas, when Delta B is zero at approximately 2 to 3 earth radii. Conversely, for a magnetically quiet condition as defined by Dst = 0, the average equatorial Delta B at these distances is -45 gammas. These results demonstrate the significance of the effects of the magnetospheric equatorial current that exists even at quiet times. A preliminary study of inclination shows that the field lines on the dusk side are more stretched out than on the dawn side. A comparison of declination on both sides indicates that the bending of the field lines toward the tail is greater near dusk than near dawn. These results suggest an appreciable dawn-dusk asymmetry in the configuration of the inner magnetospheric field.
    Schlagwort(e): GEOPHYSICS
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  • 65
    Publikationsdatum: 2011-08-16
    Schlagwort(e): GEOPHYSICS
    Materialart: Planetary and Space Science; 21; Dec. 197
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  • 66
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    Publikationsdatum: 2011-08-16
    Beschreibung: Recently, Svalgaard and Heppner reported two separate features of the polar electromagnetic field that correlate with the dawn-dusk component of the interplanetary magnetic field. This work attempts to explain these findings in terms of properties of the open magnetosphere. The topology and qualitative properties of the open magnetosphere are first studied by means of a simple model, consisting of a dipole in a constant field. Many such properties are found to depend on the separation line, a curve connecting neutral points and separating different field line regimes. In the simple model it turns out that the electric field in the central polar cap tends to point from dawn to dusk for a wide variety of external fields, but, near the boundary of the polar cap, electric equipotentials are deformed into crescents.
    Schlagwort(e): GEOPHYSICS
    Materialart: Journal of Geophysical Research; 78; Nov. 1
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  • 67
    Publikationsdatum: 2011-08-16
    Schlagwort(e): SPACE RADIATION
    Materialart: Solar Physics; 31; July 197
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  • 68
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    Publikationsdatum: 2011-08-16
    Beschreibung: Recent calculations suggest that three of the Galilean satellites are very effective in limiting the fluxes of energetic electrons and protons diffusing inward from Jupiter's outer magnetosphere. Electron and proton densities with and without lunar effects are plotted as functions of the distance from the center of the planet in units of Jupiter radii. Both electrons and protons in the model come from the solar wind. The trajectory of Pioneer 10 in magnetic coordinates is examined and the period of greatest danger to the spacecraft is discussed.
    Schlagwort(e): SPACE RADIATION
    Materialart: Science; 182; Dec. 7
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  • 69
    Publikationsdatum: 2011-08-16
    Beschreibung: A computer program is developed which predicts the vertical distribution of an absorbing species in an isotropically-scattering, finite planetary atmosphere from measurements of the upwelling band radiance determined by a vertically traversing 2-channel radiometer. Comparison is made with experiment.
    Schlagwort(e): GEOPHYSICS
    Materialart: Journal of Quantitative Spectroscopy and Radiative Transfer; 13; Dec. 197
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  • 70
    Publikationsdatum: 2011-08-16
    Beschreibung: Measurement of the altitude profile of electron temperature in the ionospheric D region with the aid of a symmetric double probe flown on a Nike-Cajun payload launched on Oct. 13, 1971. The procedure for determining the electron temperature from the parameters of the double probe's current-voltage characteristic under conditions of nonnegligible ion-atom collision frequencies is described. It is shown that in its first lower ionospheric application the technique of the symmetric double probe has yielded the lowest values of electron temperature yet measured and has provided the very first direct measurement of electron temperature in the D region.
    Schlagwort(e): GEOPHYSICS
    Materialart: Journal of Geophysical Research; 78; Nov. 1
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  • 71
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    Publikationsdatum: 2011-08-16
    Beschreibung: Discussion of the temperature-density phase anomaly on the basis of a quasi-three-dimensional model in which the thermosphere dynamics associated with wind circulation is considered in a self-consistent form. Included in this analysis are the first three harmonics, which involve nonlinear coupling between diurnal and semidiurnal tides. It is shown that the phase anomaly with exospheric temperature peaks near 1600 LT and mass density peaks between 1400 and 1445 LT can be reproduced in a self-consistent theory without invoking ad hoc assumptions and boundary conditions that would mask the physical processes to be explored. A number of factors and processes are found to contribute to the phase anomaly, including the semidiurnal and particularly the terdiurnal components, heat advection, diffusion, and energy coupling with the lower atmosphere.
    Schlagwort(e): GEOPHYSICS
    Materialart: Journal of Geophysical Research; 78; Nov. 1
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  • 72
    Publikationsdatum: 2011-08-16
    Schlagwort(e): SPACE RADIATION
    Materialart: Astrophysical Journal; 185; Nov. 1
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  • 73
    Publikationsdatum: 2011-08-16
    Schlagwort(e): SPACE RADIATION
    Materialart: Astrophysical Journal; 186; Dec. 15
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  • 74
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    Publikationsdatum: 2011-08-16
    Beschreibung: The fundamental physical and chemical processes in an idealized planetary ionosphere are considered as a general abstraction, with actual planetary ionospheres representing special cases. After describing the structure of the neutral atmospheres (the barosphere, the thermosphere, and the exosphere) and noting the principal ionizing radiations responsible for the formation of planetary ionospheres, a detailed study is made of the thermal structure of these ionospheres and of the chemical processes and plasma-transport processes occurring in them. The features of equilibrium and realistic models of planetary ionospheres are discussed, and an attempt is made to determine the extent of these ionospheres. Considering the ionosphere as a plasma, a plasma kinetic approach is developed for determining the effects of interactions between individual particles and waves in this plasma. The use of remote-sensing radio techniques and direct measurement or in situ techniques is discussed. Finally, the observed properties of the ionospheres of the Earth, Mars, Venus, and Jupiter are reviewed.
    Schlagwort(e): GEOPHYSICS
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  • 75
    Publikationsdatum: 2011-08-16
    Schlagwort(e): SPACE RADIATION
    Materialart: Astrophysical Journal; 186; Dec. 15
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  • 76
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    Publikationsdatum: 2011-08-16
    Beschreibung: The dependence of the thickness of the helium-enriched shell on the longitudinal position of the parent flares is considered along with the large-scale configuration of the expanding shell in interplanetary space. It is found that shock waves, magnetic bottles, and helium-enriched shells appear to expand eastwards of the meridian plane which crosses the flare region. It seems that the formation of the observed pattern of the shells is influenced by the interplanetary magnetic field between the sun and the earth.
    Schlagwort(e): SPACE RADIATION
    Materialart: Nature Physical Science; 246; Dec. 3
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  • 77
    Publikationsdatum: 2011-08-16
    Beschreibung: The meaning and characteristics of basic and average convection (i.e., electric field) patterns are described. The continuous existence of the basic convection pattern argues against treating magnetic field merging mechanisms as the fundamental cause of magnetospheric convection. However, whether related to merging or to some other mechanism, interplanetary magnetic field conditions significantly modulate the distribution, magnitudes, and boundaries of the convection pattern. A previous correlation between azimuthal angles of the interplanetary magnetic field and asymmetries in polar cap electric field distributions as seen by OGO-6 is reviewed. A new approach is taken to reveal correlations with the north-south angle and magnitude of the interplanetary field as well as additional features which correlate with the azimuthal angle. Both significant correlations and conditions which show a lack of correlation are found. Several aspects of the correlations appear to be particularly important.
    Schlagwort(e): GEOPHYSICS
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  • 78
    Publikationsdatum: 2011-08-16
    Beschreibung: Observations, from the Apollo 16 Spacecraft, in lunar orbit, of the total radiance of the K + F corona, from 3 to 55 solar radii are presented and discussed. The logarithmic slope of the K + F coronal radiance, at distances greater than 20 solar radii, is found to be n equals 1.93, slightly less steep than previous determinations. The photometric axis of the radiance is found to be displaced 3 plus or minus 1 deg north of the ecliptic, at distances greater than 20 solar radii, and this displacement is interpreted as an annual variation due to non-coincidence of the ecliptic and the symmetry axis of the zodiacal cloud.
    Schlagwort(e): GEOPHYSICS
    Materialart: Planetary and Space Science; 21; Dec. 197
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  • 79
    Publikationsdatum: 2011-08-16
    Beschreibung: Evaluation of OSO-5 measurements of the energy spectrum of the diffuse component of the cosmic X-ray flux in the energy range from 14 to 200 keV. A detailed description is given of the X-ray detector employed and of the method of selection and pulse-height analysis of X-ray events. The method employed in eliminating noncosmic X-ray contributions to the total counting rate is discussed. The final energy spectrum is found to be best fitted by a power law which is in essential agreement with that obtained from OSO-3 by Schwartz et al. (1970), in spite of what is regarded as an erroneous correction procedure used by them. In particular, it is suggested that the break in the energy spectrum at 40 keV which they reported may have been produced by an erroneous correction for the radioactivity induced in the detector during each passage through the intense charged-particle fluxes in the South Atlantic Anomaly.
    Schlagwort(e): SPACE RADIATION
    Materialart: Astrophysical Journal; 186; Nov. 15
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  • 80
    Publikationsdatum: 2011-08-16
    Beschreibung: A balloon-borne measurement of the cosmic ray electron spectrum from 10 to 200 GeV is reported in which two new techniques have been used to remove proton background contamination. First, the depth of the spectrometer was more than 40 radiation lengths, the equivalent of more than 3 mean free paths of material, enabling hadronically and electromagnetically induced cascades to be differentiated for a subset of the data. Second, electromagnetic cascade starting points were determined to within plus or minus 0.1 radiation lengths on the basis of a calibration with electrons from 5.4 to 18 GeV at the Stanford Linear Accelerator, greatly reducing the chances for a proton to simulate an electron. The resulting spectrum, when fitted with a power law, is quite steep, -3.2 plus or minus 0.1, but the fit to a power law is marginal.
    Schlagwort(e): SPACE RADIATION
    Materialart: Journal of Geophysical Research; 78; Nov. 1
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  • 81
    Publikationsdatum: 2011-08-16
    Beschreibung: We have observed a chromospheric brightening in the H alpha and Ca II K lines with a diameter of about 1 arc second. The time structure of this event, obtained with a relative resolution of 1 second, shows the rise time to be 4 seconds, the lifetime (FWHM) to be 20 seconds, and the decay time to be 5 seconds. This imposes new constraints on flare-point models. These restrictions can be accommodated easily by either an infall-impact flare model or a model invoking the precipitation of high-energy particles from the corona.
    Schlagwort(e): SPACE RADIATION
    Materialart: Astrophysical Journal; 185; Nov. 1
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  • 82
    Publikationsdatum: 2011-08-16
    Beschreibung: Abundances and isotopic compositions of He, Ne, Ar, and Xe have been measured in eight recently fallen chondrites. Ratios of concentrations of cosmic ray-produced He-3, Ne-21, Ne-22, and Ar-38 indicate that all eight samples experienced less than average cosmic ray shielding. He-3 and Ne-21 exposure ages were calculated using shielding corrected chondritic production rates and the measured Ne-22/Ne-21. Exposure ages calculated from Na-22/Ne-22 and Al-26/Ne-21 ratios and constant relative production rates show a bias between the two ages due to variations in Na-22/Al-26. Arguments are presented that this bias is due to irradiation hardness differences, and therefore the use of constant values for both the Na-22/Ne-22 and Al-26/Ne-21 production ratios is not permitted.
    Schlagwort(e): SPACE RADIATION
    Materialart: Geochimica et Cosmochimica Acta; 37; Nov. 197
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  • 83
    Publikationsdatum: 2011-08-16
    Beschreibung: Results of measurements by a balloon-borne ionization spectrometer of the energy dependence of high-energy cosmic-ray charge composition. The results presented are greatly improved over those obtained earlier by Ormes et al. (1971) by the use of a multidimensional charge analysis with more efficient background rejection, and a more accurate energy determination. Complex couplings between the charge, energy, and trajectory information were taken into account and are discussed. The spectra of individual elements up to oxygen and of groups of nuclei up through iron were measured up to almost 100 GeV per nucleon. The energy spectrum of the secondary nuclei, B + N, is found to be steeper than that of the primary nuclei, C + O, in agreement with Smith et al. (1973). The most dramatic finding is that the spectrum of the iron nuclei is flatter than that of the carbon and oxygen nuclei by 0.57 plus or minus 0.14 of a power.
    Schlagwort(e): SPACE RADIATION
    Materialart: Astrophysical Journal; 186; Nov. 15
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  • 84
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    Publikationsdatum: 2011-08-16
    Beschreibung: Magnetic hysteresis loops and the derived hysteresis ratios R sub H and R sub I are used to classify the various natural dilute magnetic materials. R sub I is the ratio of saturation isothermal remanence (I sub R) to saturation (I sub S) magnetization, and R sub H is the ratio of remanent coercive force (H sub R) to coercive force (H sub C). The R sub H and R sub I values depend on grain size, the characteristics of separate size modes in mixtures of grains of high and low coercivity, and the packing characteristics. Both R sub H and R sub I are affected by thermochemical alterations of the ferromagnetic fraction. Hysteresis loop constriction is observed in lunar samples, chondrite meteorites, and thermochemically altered basaltic rocks, and is due to mixtures of components of high and low coercivity. Discrete ranges of R sub H and R sub I for terrestrial and lunar samples and for chondrite meteorites provide for a classification of these natural materials based on their hysteresis properties.
    Schlagwort(e): GEOPHYSICS
    Materialart: Earth and Planetary Science Letters; 20; 1, Se; Sept
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  • 85
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: A list of emission lines in the spectra of solar flares between 6 and 25 A has been compiled using data obtained with a KAP crystal spectrometer on the OSO-5 satellite. The emission lines have been classified according to their sensitivity to flare activity. This classification provides a method for discriminating between iron in high stages of ionization (Fe XX-Fe XXV) and lower stages (Fe XVII-Fe XIX), the lines of which are both present in the same spectral region during flares. Identifications consistent with these classifications are proposed. Anomalous intensities in the spectra of Fe XVII and Fe XX are pointed out, and implications of the observations for models of the X-ray emitting regions are discussed.
    Schlagwort(e): SPACE RADIATION
    Materialart: Solar Physics; 31; July 197
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  • 86
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: Certain results regarding the ratio of cosmic-ray sources (CRS) and Solar System abundances are the same as those obtained from explosive nucleosynthesis. Such a model is consistent with the fact that in the Solar System Mg, Si, and Fe are believed to be produced by explosive nucleosynthesis, whereas C and O are mainly products of other processes. The model considered explains the carbon-to-oxygen ratio in the cosmic rays.
    Schlagwort(e): SPACE RADIATION
    Materialart: Nature Physical Science; 246; Nov. 26
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  • 87
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: Knowledge of the total gamma-ray production rate per H atom from the decay of neutral pions produced in interstellar cosmic-ray interactions is essential for determining the possible amount of interstellar H2. This production rate is recalculated here using the latest accelerator data on neutral pion production in p-p interactions up to about 1500 GeV. A simple but accurate approximation used here resolves the past disagreement over the magnitude of this rate. An upper limit is obtained of (1.51 plus or minus 0.23) times 10 to the -25th power/sec, consistent with the observed upper limit of 1.6 times 10 to the -25th power/sec.
    Schlagwort(e): SPACE RADIATION
    Materialart: Astrophysical Journal; 185; Oct. 15
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  • 88
    Publikationsdatum: 2011-08-16
    Beschreibung: The ultraviolet earth radiance data from the backscatter ultraviolet experiment on Nimbus 4 have been inverted to infer ozone profiles using a single Rayleigh scattering model. Two methods of solution give essentially the same results. Comparison of these profiles with simultaneous rocket sounding data shows satisfactory agreement at low and middle latitudes. Vertical cross-sections of ozone mixing ratio along the orbital tracks indicate that while the gross characteristics of the ozone field above 10 mb are under photochemical control, the influence of atmospheric motions can be found up to the 4 mb level.
    Schlagwort(e): GEOPHYSICS
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  • 89
    Publikationsdatum: 2011-08-16
    Beschreibung: Review of some of the procedures and results of the double monochromator and colinear photometer Nimbus-4 satellite experiment that measures ultraviolet terrestrial radiance, Lambert reflectivity of the lower boundary of the scattering atmosphere, and extraterrestrial solar irradiance. The experiment has produced nearly three years of almost continuous data which are being used to infer the high-level ozone distribution and total ozone on a global basis. The high-level ozone data have been verified by independent coincident rocket ozone soundings, and the total ozone values show good agreement with Dobson spectrophotometer determinations. An increase has been observed in equatorial radiance at 2550 A relative to 2900 A, which seems to indicate that the amount of ozone in the upper stratosphere is related to the eleven-year solar cycle.
    Schlagwort(e): GEOPHYSICS
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  • 90
    Publikationsdatum: 2011-08-16
    Beschreibung: Recent Jimsphere/Jimsonde measurements of tropospheric temperature profile spectra in the wavelength band from 50 to 2000 meters above the atmospheric boundary layer, taken over Cape Kennedy, Florida, are summarized. The results suggest that the spectra can be represented in the nondimensional form (omega sub g/sigma sub w)phi(k)/sigma sub T squared = S(K), where phi(k) is the temperature profile spectrum at wave number k, omega sub g is the Brunt-Vasala frequency, sigma sub w and sigma sub T denote the standard deviations of the vertical velocity and temperature profiles, and S is a universal function of nondimensional wave number K = k sigma sub w/omega sub g.
    Schlagwort(e): GEOPHYSICS
    Materialart: Journal of Geophysical Research; 78; Sept. 20
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  • 91
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: Since May 1970, personnel on several campuses of the University of California have been conducting investigations which seek to determine the usefulness of modern remote sensing techniques for studying various components of California's earth resources complex. Emphasis has been given to California's water resources as exemplified by the Feather River project and other aspects of the California Water Plan. This study is designed to consider in detail the supply, demand, and impact relationships. The specific geographic areas studied are the Feather River drainage in northern California, the Chino-Riverside Basin and Imperial Valley areas in southern California, and selected portions of the west side of San Joaquin Valley in central California. An analysis is also given on how an effective benefit-cost study of remote sensing in relation to California's water resources might best be made.
    Schlagwort(e): GEOPHYSICS
    Materialart: An Integrated Study of Earth Resources in the State of Calif. Using Remote Sensing Tech.; 7 p
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  • 92
    Publikationsdatum: 2011-08-16
    Beschreibung: The areas of focus of the Santa Barbara and Riverside groups in conducting water demand studies are the central and southern California regional test sites, respectively. Within each test site, sub-areas have been selected for use in the making of detailed investigations. Within each of these sub-areas an in-depth evaluation is being made as to the capability of remote sensing systems to provide pertinent data relative to water demand phenomena. These more limited sub-areas are: (1) Kern County and the San Joaquin Basin; (2) Chino-Riverside Basin; and (3) the Imperial Valley. Rational for the selection of these subareas included the following: Much of the previous remote sensing research had been conducted in these areas and therefore a great deal of remote sensing imagery and pertinent ground truth for the areas was already available.
    Schlagwort(e): GEOPHYSICS
    Materialart: An Integrated Study of Earth Resources in the State of Calif. Using Remote Sensing Tech.; 71 p
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  • 93
    Publikationsdatum: 2011-08-16
    Beschreibung: The primary test site for water supply investigations continues to be the Feather River watershed in northeastern California. This test site includes all of the area draining into and including the Oroville Reservoir. The principal effort is to determine the extent to which remote sensing techniques, when properly employed, can provide information useful to those persons concerned with the management and planning of lands and facilities for the production of water, using the Oroville Reservoir and the California Water Project as the focus for the study. In particular, emphasis is being placed on determining the cost effectiveness of information derived through remote sensing as compared with that currently being derived through more conventional means.
    Schlagwort(e): GEOPHYSICS
    Materialart: An Integrated Study of Earth Resources in the State of Calif. Using Remote Sensing Tech.; 110 p
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  • 94
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: The barium cloud injection deep into the magnetosphere of Sept. 21, 1971, has revealed that the quiet-time near-equatorial nightside magnetic field is significantly different from that predicted by existing quite-time models. The influence of currents flowing on or near the geomagnetic equator gives the field a more tail-like structure at a distance as close as 5 earth radii. Several models have been tried out to obtain a best fit to the experimental observations of the shape of the field-aligned ion cloud. Although this method does not lead to a unique solution, the most acceptable option emerging from this analysis is a quiet-time tilted image-dipole model with a Williams-Mead tail field and a disclike ring current on the geomagnetic equator.
    Schlagwort(e): GEOPHYSICS
    Materialart: Journal of Geophysical Research; 78; Sept. 1
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  • 95
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: Two shock-like structures (i.e., abrupt step-like increases in number density, bulk speed, and proton temperature) were found in the data from Mariner 5 at 0.98 AU on June 26 and at 0.85 AU on Aug. 29, 1967. The thickness of these 'structures' determined from the magnetic field data was more than 1000 proton Larmor radii. They were also observed by Explorer 33, 34, and 35 at 1 AU, where the thicknesses were much smaller than in the Mariner 5 data. It is suggested that these two structures were nonlinear magnetoacoustic waves that were in the processes of steepening. It is further suggested that shocks would be formed just beyond 1 AU. These structures were not associated with corotating streams, but they could be associated with impressive solar events in which a flare was followed by type 2 and type 4 radio emission and a rare chromospheric wave.
    Schlagwort(e): SPACE RADIATION
    Materialart: Journal of Geophysical Research; 78; Sept. 1
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  • 96
    Publikationsdatum: 2011-08-16
    Beschreibung: This paper reviews the optical data obtained by NASA in the joint NASA-MPE experiment conducted on September 21, 1971, involving the release of a barium cloud at an altitude of about 31,500 km over Colombia, South America. The data indicated an anomalously high rate of elongation and an unexpectedly large rate of deceleration of the main core of the ion cloud. The outermost striational features achieved a steady velocity within a few minutes, thus indicating that they had acquired the velocity of the ambient plasma. From the observed drift of these striations, one deduces an electric field that, when referred to a coordinate system rotating with the earth, has a meridional component directed toward the interior of the magnetic loop of 0.14 mV/m and a component perpendicular to the meridional plane of 0.15 mV/m directed to the west.
    Schlagwort(e): GEOPHYSICS
    Materialart: Journal of Geophysical Research; 78; Sept. 1
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  • 97
    Publikationsdatum: 2011-08-16
    Beschreibung: Amplitudes and phases for the diurnal and semidiurnal variations of thermospheric molecular nitrogen density and temperature are determined from data obtained by six rocket-launched thermosphere probes. The semidiurnal tide is significant for the lower thermosphere variations, where it could dominate in the N2 density at 140 km and in the temperature for altitudes between 170 and 200 km. At exospheric heights, the magnitudes of the semidiurnal modes in density and temperature are significantly smaller than those of the diurnal mode. The temperature phase is height-dependent in both diurnal and semidiurnal components below 200 km, thus contributing to phase differences between N2 density and temperature in both modes. No significant phase differences are apparent between N2 density and thermospheric temperature above 250 km.
    Schlagwort(e): GEOPHYSICS
    Materialart: Journal of Geophysical Research; 78; Sept. 1
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  • 98
    Publikationsdatum: 2011-08-16
    Beschreibung: The atomic oxygen emission line at 6300 A as measured in the nadir direction by a photometer on the polar-orbiting satellite Ogo 4 has been plotted between 40 deg N and 40 deg S latitude on a series of maps for the moon-free periods between Aug. 30, 1967, and Jan. 10, 1968. Readily apparent are the longitudinal and local time variations that occur during the northern fall-winter season. The northern tropical arc is more widespread; the southern arc is not present at all longitudes. The arcs in early evening are strong and distinct, separated by very low emission rates at the magnetic equator. The arcs lie generally along magnetic parallels, move toward the magnetic equator as the night progresses, and, in the early morning hours, decrease in emission rate and degenerate into patches.
    Schlagwort(e): GEOPHYSICS
    Materialart: Journal of Geophysical Research; 78; Sept. 1
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  • 99
    facet.materialart.
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: The possible acceleration of heavy ions by the resonance scattering of radiation near bright stellar objects is examined. Planck spectra are assumed. At any radiation temperature, heavy-ion energies are found to be limited by aberration and Doppler effects. Photoionization is found to limit maximum radiation temperatures and energies for each ion. Collisional ionization by ambient electrons and ions may further limit heavy-ion energies. Because of these limitations, the production of the more energetic cosmic rays by this mechanism appears to be very improbable. If supernova radiation temperatures are high enough, they may produce heavy ions with energies up to several hundreds of MeV per nucleon. O and B stars appear to be able to accelerate certain heavy ions to 200 and 80 MeV per nucleon, respectively.
    Schlagwort(e): SPACE RADIATION
    Materialart: Astrophysical Journal; 184; Sept. 1
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  • 100
    facet.materialart.
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: Photoelectric observations are reported of two occultations of Jupiter's satellite Europa by the satellite Io. The reductions in the intensity during these events exceeds predicted values by 80% and 55% for the nights of June 17, 1973, and June 24, 1973, respectively. It is concluded that Europa has a bright polar cap extending from the north pole to latitude 30 deg. The light curves for the Europa occultations are presented.
    Schlagwort(e): GEOPHYSICS
    Materialart: Nature; 244; Aug. 31
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