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  • GEOPHYSICS  (494)
  • 1975-1979  (494)
  • 1979  (494)
  • 1
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    Overview - Electric fields (1979)
    In:  Other Sources
    Details
    Publication Date: 2019-08-28
    Description: The electric fields session is designed to review progress in observation, theory, and modeling of magnetospheric electric fields, and to expose important new results. The present report comments on the state and prospects of electric field research, with particular emphasis on relevance to quantitative modeling of the magnetospheric processes. Attention is given to underlying theories and models. Modeling philosophy is discussed relative to explanatory models and representative models. Modeling of magnetospheric electric fields, while in its infancy, is developing rapidly on many fronts employing a variety of approaches. The general topic of magnetospheric electric fields is becoming of prime importance in understanding space plasmas.
    Keywords: GEOPHYSICS
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  • 2
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    Lightning apparent source of environmentally important gases (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-28
    Keywords: GEOPHYSICS
    Type: NASA-NEWS-RELEASE-79-131 , P79-10129
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  • 3
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    Application of space technology to crustal dynamics and earthquake research (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-28
    Description: In cooperation with other Federal government agencies, and the governments of other countries, NASA is undertaking a program of research in geodynamics. The present program activities and plans for extension of these activities in the time period 1979-1985 are described. The program includes operation of observatories for laser ranging to the Moon and to artificial satellites, and radio observatories for very long baseline microwave interferometry (VLBI). These observatories are used to measure polar motion, earth rotation, and tectonic plate movement, and serve as base stations for mobile facilities. The mobile laser ranging and VLBI facilities are used to measure crustal deformation in tectonically active areas.
    Keywords: GEOPHYSICS
    Type: NASA-TP-1464
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  • 4
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    Lightning as an indication of storm severity (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-28
    Description: There is a substantial case for the theory that cloud electrification is related primarily to strong convection and the sizeable relative air motion that it implies; therefore, the electrification and subsequent discharge rates can be related to the air motion environment of thunderstorms. The isoceraunic contour map used by the WMO for observing and measuring thunderstorm occurrence contains no information on flash rates, flash density, flash relationship to storm severity, or flash variation with meteorological environment. A constant-view geosynchronous lightning mapper would permit simultaneous studies of the lightning discharge patterns and the meteorological environment of storms, thus establishing whether or not there is a reliable enough relationship to use the observed flash rates and characteristics as supplemental guidance for storm forecast refinement.
    Keywords: GEOPHYSICS
    Type: NASA. Marshall Space Flight Center Proc.: Workshop on the Need for Lightning Observations from Space; p 153-155
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  • 5
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    The effect of errors in the assignment of the transmission functions on the accuracy of the thermal sounding of the atmosphere (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-28
    Description: In order to test the error of calculation in assumed values of the transmission function for Soviet and American radiometers sounding the atmosphere thermally from orbiting satellites, the assumptions of the transmission calculation is varied with respect to atmospheric CO2 content, transmission frequency, and atmospheric absorption. The error arising from variations of the assumptions from the standard basic model is calculated.
    Keywords: GEOPHYSICS
    Type: NASA-TM-75654 , Conf. of the Soviet-Am. Working Group on Space Meteorol.; Nov 10, 1976 - Nov 22, 1976; Moscow
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  • 6
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    Method for the rapid temperature correction of a transmission in an inhomogeneous atmosphere (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-28
    Description: The value of the transmission function in a heterogeneous atmosphere is determined by iterative correction of values in particular layers. The iterative equation and a set of absolute values of errors is presented in two tables.
    Keywords: GEOPHYSICS
    Type: NASA-TM-75649 , Conf. of the Soviet-Am. Working Group on Space Meteorol.; Nov 10, 1976 - Nov 22, 1976; Moscow
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  • 7
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    On the acceleration of the auroral plasma of the Earth due to conic instability (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-28
    Description: The role of electrostatic conic instability in the diffusion of spilled particles and the acceleration of the auroral plasma of the Earth are numerically investigated by means of quasi-linear equations. Linear increments to the conic instability under magnetospheric conditions are introduced. The quasi-linear equation is averaged along tubes of force taking into account the drift across the magnetic field lines. It is shown that the existence of a conic instability leads to small spills and isotropic distribution of particles, but is also accompanied by significant acceleration of electrons.
    Keywords: GEOPHYSICS
    Type: NASA-TM-75638 , PR-430
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  • 8
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    Multicomponent diffusion and energy characteristics of partially ionized plasma in the ionosphere of a planet (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-28
    Description: The problem of energy and multicomponent ambipolar diffusion of plasma in the lower ionosphere of a planet with a weak magnetic field is considered.
    Keywords: GEOPHYSICS
    Type: NASA-TM-75409 , PREPRINT-123
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  • 9
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    The magnetic anomaly of the Ivreazone (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-28
    Description: A magnetic field survey was made in the Ivreazone in 1969/70. The results were: significant anomaly of the vertical intensity is found. It follows the basic main part of the Ivrea-Verbano zone and continues to the south. The width of the anomaly is about 10 km, the maximum measures about +800 gamma. The model interpretation shows that possibly the anomaly belongs to an amphibolitic body, which in connection with the Ivrea-body was found by deep seismic sounding. Therefore, the magnetic anomaly provides further evidence for the conception that the Ivrea-body has to be regarded as a chip of earthmantle material pushed upward by tectonic processes.
    Keywords: GEOPHYSICS
    Type: NASA-TM-75425
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  • 10
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    The reaction of the atmosphere to solar disturbances (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-28
    Description: The effect of solar flares on the thermosphere and the troposphere is investigated. It is found that during periods of geoeffect solar disturbances, there is a connection between phenomena in the upper and lower atmospheres and that variations in atmospheric parameters correlate with changes in the geomagnetic index.
    Keywords: GEOPHYSICS
    Type: NASA-TM-75500 , All-Union Conf. on Sun Atmosphere Relations in Climate Theory and Weather Forecasts; Oct 30, 1972 - Nov 01, 1972; Moscow
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  • 11
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    Recent results of radio interferometric determinations of a transcontinental baseline, polar motion, and earth rotation (1979)
    In:  Other Sources
    Details
    Publication Date: 2019-08-28
    Description: Results are discussed for radio interferometric observations of extragalactic radio sources with antennas at Haystack Observatory in Massachusetts and the Owens Valley Radio Observatory in California (3900-km baseline) during 14 separate experiments distributed between September 1976 and May 1978. Simultaneous analysis of the data from several experiments yields estimates of changes in the x component of pole position and in earth's rotation (UT1). Comparison with the corresponding results obtained by the Bureau International de l'Heure (BIH) reveals systematic differences. In particular, the trends in the radio interferometric determinations of the changes in pole position are found to agree more closely with those from the International Polar Motion Service and from Doppler observations of satellites than with those from the BIH.
    Keywords: GEOPHYSICS
    Type: Time and the earth''s rotation; Eighty-second Symposium; May 08, 1978 - May 12, 1978; San Fernando; Spain
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  • 12
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    Global distribution of ozone for various seasons (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-28
    Description: A technique which was used to obtain a catalog of the seasonal global distribution of ozone is presented. The technique is based on the simultaneous use of 1964-1975 data on the total ozone content from a worldwide network of ozonometric stations and on the vertical ozone profile from ozone sounding stations.
    Keywords: GEOPHYSICS
    Type: NASA-TM-75435
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  • 13
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    Altitudes of the lower edge of the artificial auroral rays on the basis of the observations in the Zarnitsa-2 experiments (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-28
    Description: Some results of optical television measurements in the Zarnitsa-2 experiment are presented. The altitudes of the lower edge of artificial auroral rays were determined by the triangulation method and are compared with theoretical calculations of these altitudes based on the Jacchia and CIRA models of the atmosphere.
    Keywords: GEOPHYSICS
    Type: NASA-TM-75631
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  • 14
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    Anomaly of the composition of the F-2 equatorial region of the ionosphere during the hours after sunset according to data from the mass-spectrometer experiment on the Cosmos-274 (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-28
    Description: A mass spectrometer on board Cosmos-274 measured concentrations of light atoms and ions. While traversing the geomagnetic equator during the evening hours it recorded on anomalous drop in ionized molecular oxygen and ionized atomic oxygen and nitrogen. A similar, less dramatic, decline was observed in the concentration of neutral atomic oxygen. A possible explanation for this and previously observed behavior is an ascent in altitude of the F layer in the hours after sunset, a possibility which is supported by calculations.
    Keywords: GEOPHYSICS
    Type: NASA-TM-75615 , PR-331
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  • 15
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    Internal gravity waves in the upper atmosphere, generated by tropospheric jet streams (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-28
    Description: A mechanism of internal gravity wave generation by jet streams in the troposphere is considered. Evaluations of the energy and pulse of internal gravity waves emitted into the upper atmosphere are given. The obtained values of flows can influence the thermal and dynamic regime of these layers.
    Keywords: GEOPHYSICS
    Type: NASA-TM-75407
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  • 16
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    On the possibility of analytical approximation of line forms during random disorders of the resonance frequencies in molecular vibration-rotation spectra for satellite sounding (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-27
    Description: The generalization spectral line contour concept and formulas for a two component mixture, as well as consequences of the general formula are discussed. The calculation procedure, initial information, calculation results and comparison of calculations with available experimental data, for radiation absorption in three CO2 bands are presented.
    Keywords: GEOPHYSICS
    Type: NASA-TM-75655
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  • 17
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    Study of the 10 micron continuum of water vapor (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-27
    Description: Radiation attenuation by atmospheric water vapor is considered. A formula based on laboratory data is recommended for approximating continuous absorption in the spectra region in question. Data of full scale measurements and laboratory experiments are compared. It was concluded that only molecular absorption need be taken into account under clear atmospheric conditions during the warm part of the year, while in winter or in cloudy conditions, the effect of aerosol can be significant.
    Keywords: GEOPHYSICS
    Type: NASA-TM-75650
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  • 18
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    Results of the measurement of the vertical profile of ozone up to a height of 70 km by means of the MR-12 and M-100 sounding rockets (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-27
    Description: The photometers used and methods of calculation of the vertical ozone concentration profile are described. The results obtained in several series of MR-12 and M-100 sounding rocket launchings are presented and discussed.
    Keywords: GEOPHYSICS
    Type: NASA-TM-75380
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  • 19
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    SAGE to examine Earth's stratosphere (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-27
    Description: The SAGE mission is discussed along with the role of the Nimbus 7 experiment. Other topics discussed include: ground truth measurements, data collection and processing, SAGE instrumentation, and launch sequence.
    Keywords: GEOPHYSICS
    Type: NASA-NEWS-RELEASE-79-6 , P79-10006
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  • 20
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    Results of measurement of the night corpuscular flux on the MR-12 rockets in the JASPIC project (Soviet part of the program) (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-27
    Description: In June 1978, a joint Soviet-American project (JASPIC) was conducted, the goals of which were: (1) the study of the flows of spilling electrons which act upon the middle-latitude ionosphere under nocturnal conditions (nocturnal corpuscular source of ionization); and (2) the mutual comparison of procedures for recording corpuscular radiations in the upper atmosphere, using meteorological and geophysical rockets.
    Keywords: GEOPHYSICS
    Type: NASA-TM-75691
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  • 21
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    Problems with the interpretation of paleomagnetic measurements due to studies of basalts from the Paleovolcano Vogelsberg in Hessen (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-27
    Description: The palaeomagnetic parameters of more than 5,000 samples of cores taken from 33 drilling holes through innumerable basalt units of the Vogelsberg Paleovolcano in Hessen were measured. Measurements of specimens of thin and thick layers without any gap proved that inclination, natural remanence, susceptibility and Konigsberger factor were dependent on their distance from the surface of units, layers, lamelles, etc. Therefore, representative data for the evaluation of palaeomagnetic measurements can be expected only in the interior part of lava flows and intrusions. The statistic method which enclosed all values of measurements gave significant data which was not appropriate for the interpretation of palaeomagnetic and geological events.
    Keywords: GEOPHYSICS
    Type: NASA-TM-75355
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  • 22
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    International rocket project to compare ozone sensors (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-27
    Keywords: GEOPHYSICS
    Type: NASA-NEWS-RELEASE-79-130 , P79-10128
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  • 23
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    Global Aspects of the Earth's Magnetopause (1979)
    In:  Other Sources
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    Publication Date: 2019-08-14
    Description: Measurable characteristics of the magnetopause are discussed. The Earth's magnetopause is a thin magnetic discontinuity separating the shocked, magnetized plasma of the solar wind from a more tenuous plasma contained by the geomagnetic field. This external magnetosheath plasma flows around the magnetosphere with characteristics that are in approximate agreement with gas dynamic theory. The interplanetary magnetic field carried by this plasma becomes draped over the magnetosphere and its orientation relative to the local geomagnetic field determines the local magnetopause current. Solar wind pressure and interplanetary field direction control the geocentric distance to the magnetopause with high pressures and southware fields moving the equatorial magnetopause to a more earthward location. Evidence suggests that the magnetopause is Kelvin-Helmholtz unstable and surface waves are propagating toward the magnetotail.
    Keywords: GEOPHYSICS
    Type: ESA Magnetospheric Boundary Layers; p 5-13
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  • 24
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    The coordinated federal program for the application of space technology to crustal dynamics and earthquake research (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-13
    Description: The application of space technology to important problems relating to crustal dynamics and earthquake research is described. Federal plans for such applications are summarized.
    Keywords: GEOPHYSICS
    Type: NASA-TM-82215
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  • 25
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    NASA laser systems to study earth's crustal movements (1979)
    In:  CASI
    Details
    Publication Date: 2019-08-13
    Keywords: GEOPHYSICS
    Type: NASA-NEWS-RELEASE-79-117 , P79-10116
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  • 26
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    Balloon-borne atmospheric spectral measurements (1979)
    In:  Other Sources
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    Publication Date: 2019-07-27
    Description: Infrared solar spectra, with .02 per cm resolution, were collected during sunset from a balloon at 40 km on October 27, 1978. Portions of the data obtained during the flight have been compared with theoretical calculations made using the data on the AFGL tape. The results of these comparisons reveal a number of areas of disagreement between theory and experimental results. The areas of disagreement are discussed in detail.
    Keywords: GEOPHYSICS
    Type: Atmospheric effects on radiative transfer; August 29, 30, 1979; San Diego, CA
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  • 27
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    Evaluation of atmospheric trace constituent sensors operating from remote space and airborne platforms (1979)
    In:  CASI
    Details
    Publication Date: 2019-07-20
    Description: A laboratory gas analysis system was developed specifically to make trace level measurements of carbon monoxide. To assure that the data collected with this system are correctly aligned with other established methods for making these measurements, an intercalibration study was conducted. The calibration gas was analyzed by the various participating laboratories and found to contain 1.28 ppm CO. Samples were collected at 25 deg, 35 deg, and 45 deg N for profile data to study the variation in concentrations of CO and CH4 as a function of altitude and latitude in continental air over the eastern seaboard of the United States. The experiment was repeated several months later to determine if there were seasonally dependent variations in the CO and CH4 concentrations.
    Keywords: GEOPHYSICS
    Type: NASA-CR-162365 , GSTR-79-8
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  • 28
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    Gravity anomaly and geoid undulation results in local areas from GEOS-3 altimeter data (1979)
    In:  Other Sources
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    Publication Date: 2019-07-13
    Description: The adjusted GEOS-3 altimeter data, taken as averages within a data frame, have been used to construct free air anomaly and geoid undulation profiles and maps in areas of geophysical interest. Profiles were constructed across the Philippine Trench (at a latitude of 6 deg) and across the Bonin Trench (at a latitude of 28 deg). In the latter case an anomaly variation of 443 mgals in 143 km was derived from the altimeter data. These variations agreed reasonably with terrestrial estimates, considering the predicted point accuracy was about + or - 27 mgals. An area over the Patton Sea mounts was also investigated with the altimeter anomaly field agreeing well with the terrestrial data except for the point directly over the top of the sea mount. It is concluded that the GEOS-3 altimeter data is valuable not only for determining 5 deg and 1 deg x 1 deg mean anomalies, but also can be used to describe more local anomaly variations.
    Keywords: GEOPHYSICS
    Type: The use of artificial satellites for geodesy and geodynamics. Volume 2; May 29, 1978 - Jun 02, 1978; Athens; Greece
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  • 29
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    Laboratory simulation of ionospheric double-layers (1979)
    In:  Other Sources
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    Publication Date: 2019-07-13
    Description: A mechanism for double-layer formation in partially- or fully-ionized plasmas is described, founded on beam-plasma interaction: RF growth along the beam excites a rectified, ponderomotive electric field, which in turn causes charge separation. Laboratory studies of the mechanism are described.
    Keywords: GEOPHYSICS
    Type: Wave instabilities in space plasmas; Jul 31, 1978 - Aug 08, 1978; Helsinki; Finland
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  • 30
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    Siple station experiments on wave-particle interactions in the magnetosphere (1979)
    In:  Other Sources
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    Publication Date: 2019-07-13
    Description: Natural and controlled whistler-mode signals have been used to study nonlinear mechanisms of wave growth and wave-wave interactions (WWI) in the magnetosphere; three general classes of WWI (triggering, suppression, and entrainment) are identified and interpreted in terms of a model based on cyclotron resonance interaction. This model is also used to estimate the wave field intensity associated with different types of WWI. A new type of triggered emission, the band-limited impulse (BLI) is interpreted in terms of the switching of phase-bunched currents. In addition, an experiment to find a threshold for the excitation of the coherent wave instability is discussed, and observed VLF wave-induced transient bursts of X-rays, light and E-region ionization enhancements are considered with regard to a step function wave interacting with all resonant electrons in a given energy range.
    Keywords: GEOPHYSICS
    Type: Wave instabilities in space plasmas; Jul 31, 1978 - Aug 08, 1978; Helsinki; Finland
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  • 31
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    Magnetospheric multiharmonic instabilities (1979)
    In:  Other Sources
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    Publication Date: 2019-07-13
    Description: The paper discusses linear convective growth rates of instabilities of electrostatic multiple electron cyclotron harmonic waves in a plasma consisting of a hot electron component with a loss-cone type of free energy source and a cold electron component of presumably ionospheric origin. When the ratio of cold to hot electron temperature is small, the cold upper hybrid frequency controls the harmonic bands that can be nonconvectively stable. When this ratio increases above a few times 0.01, nonconvective instability disappears simultaneously for each harmonic band, when the density ratio is less than unity. A consistent interpretation of the spatial localization and harmonic frequency bandwidths of the observed waves can be made assuming linear convective saturation, provided that the cold electrons have temperatures considerably in excess of those in the ionosphere.
    Keywords: GEOPHYSICS
    Type: Wave instabilities in space plasmas; Jul 31, 1978 - Aug 08, 1978; Helsinki; Finland
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  • 32
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    Chorus, energetic electrons and magnetospheric substorms (1979)
    In:  Other Sources
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    Publication Date: 2019-07-13
    Description: The paper investigates possible chorus generation mechanisms by means of simultaneous OGO-5 measurements of chorus, energetic (79 + or - 23 keV) electron fluxes and pitch angle distributions, and ambient magnetic fields. Further, the solar wind data during high-latitude dayside chorus events are examined. It is reported that the highly eccentric orbit had an apogee of 24 earth radii and an inclination of 30 deg to the geographic equator.
    Keywords: GEOPHYSICS
    Type: Wave instabilities in space plasmas; Jul 31, 1978 - Aug 08, 1978; Helsinki; Finland
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  • 33
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    Does ELF chorus show evidence of power line stimulation (1979)
    In:  Other Sources
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    Publication Date: 2019-07-13
    Description: A study to determine the effect of power line radiation on the stimulation of the ELF chorus detected on OGO-5 is presented. Chorus shows a maxima over the Eastern USSR, Greenland, and Central Siberia and minima over central and Eastern Canada, a distribution different than the OGO-3. This discrepancy is explained as due to data oversampling in the previous study; the OGO-5 data were reanalyzed with the oversampling removed, showing that none of the longitudinal maxima or minima are statistically significant. It is concluded that there is no significant correlation between longitude and chorus occurrence which implies that there is little or no evidence of power line harmonic radiation effects on chorus triggering.
    Keywords: GEOPHYSICS
    Type: Wave instabilities in space plasmas; Jul 31, 1978 - Aug 08, 1978; Helsinki; Finland
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  • 34
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    Effects of power line radiation into the magnetosphere (1979)
    In:  Other Sources
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    Publication Date: 2019-07-13
    Description: Observations of the effects of VLF power line radiation on whistler-mode waves in the magnetosphere are reviewed. High-altitude OGO-3 spectral data reveal evidence of enhanced chorus activity over populated regions starting at harmonics of the power-line frequencies. Low-altitude Ariel 3 measurements of 3.2 kHz noise intensity also indicate an enhancement of VLF activity over populated areas and their conjugates, however the relative importance of power line radiation, whistlers and spontaneous emissions is not known. The low-altitude polar-orbiting OGO-4 satellite also observed noise spectra at the harmonics of power line frequencies over industrial regions. Ground observations from Eights and Siple, Antarctica indicate that power line radiation effects on magnetospheric ducted paths peak at 3 kHz and near dawn, and exhibit a pronounced decrease on Sundays in the conjugate region, when power consumption is at a minimum. Experiments simulating power line radiation effects have also been performed. It is suggested that power line radiation effects magnetospheric activity by lowering the threshold for wave growth, with the localization of VLF sources acting to localize corresponding particle precipitation without necessarily affecting global average precipitation.
    Keywords: GEOPHYSICS
    Type: Wave instabilities in space plasmas; Jul 31, 1978 - Aug 08, 1978; Helsinki; Finland
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  • 35
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    Study and evaluation of impulse mass spectrometers for ion analysis in the D and E regions of the ionosphere (1979)
    In:  CASI
    Details
    Publication Date: 2019-07-13
    Description: Theoretical and numerical analyses were made of planar, cylindrical and spherical electrode time-of-flight mass spectrometers in order to optimize their operating conditions. A numerical analysis of potential barrier gating in time-of-flight spectrometers was also made. The results were used in the design of several small mass spectrometers. These were constructed and tested in a laboratory space simulator. Detailed experimental studies of a miniature cylindrical electrode time of flight mass spectrometer and of a miniature hemispherical electrode time of flight mass spectrometer were made. The extremely high sensitivity of these instruments and their ability to operate at D region pressures with an open source make them ideal instruments for D region ion composition measurements.
    Keywords: GEOPHYSICS
    Type: NASA-CR-163490
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  • 36
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    Coronal magnetic structure and the latitude and longitude distribution of energetic particles, 1-5 AU (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: The relation of the coronal magnetic field structure to the distribution of approximately 1 MeV protons in interplanetary space between 1 and 5 AU is discussed. After ordering the interplanetary data by its estimated coronal emission source location in heliographic coordinates, the multispacecraft measured proton fluxes are compared with coronal magnetic field structure infrared as observed in soft X-ray photographs and potential field calculations. Evidence for the propagation and possible acceleration of solar flare protons on high magnetic loop structure in the corona is presented. Further, it is shown that corotating proton flux enhancements are associated with regions of low coronal X-ray emission (including coronal holes), usually in association with solar wind stream structure.
    Keywords: GEOPHYSICS
    Type: NASA-CR-161391
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  • 37
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    The influence of variations in ozone concentration on the temperature regime of the atmosphere (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: The results of a study of the effects provided by changes in the concentration of atmospheric ozone on the mean temperatures of the troposphere and lower stratosphere are presented. It was found that ozone must be considered no less important in producing climatic changes than is CO2.
    Keywords: GEOPHYSICS
    Type: NASA-TM-75350 , All-Union Conf.; Oct 30, 1972 - Nov 01, 1972; Moscow
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  • 38
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    Numerical modeling of baroclinic instability (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: The Eady model of baroclinic instability applied to a rotating channel with Ekman layers at the top and bottom is extended to a beta-plane channel. Changes in the shape and position of the boundary separating the regions of axially symmetric and wavelike motion are predicted.
    Keywords: GEOPHYSICS
    Type: NASA-CR-161363
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  • 39
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    Influence of clouds on UV-B penetration to the earth's surface (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: Radiometric measurements of cloud influence on ultraviolet B radiation (UV-B) were obtained. Mathematical models of the influence were defined to lay the groundwork for the construction of the global UV-B climatology from satellite determined ozone data. More refined measurements comparing UV-B radiation with total solar radiation were carried out. The cloudy case is referred to the cloudless sky irradiance and convenient transmission ratios are given An approach to the inversion of scattering data is summarized. An improved characterization of the UV-B radiation from a cloudless sky is also presented.
    Keywords: GEOPHYSICS
    Type: NASA-CR-160428
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  • 40
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    Rocket ozone sounding network data (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: During the period March 1977 through May 1977, three regular monthly ozone profiles were measured at Wallops Flight Center and three regular monthly ozone profiles were measured at the Churchill Research Range. One additional flight was conducted at Wallops Flight Center in support of Nimbus 4 SBUV. Data results and flight profiles for the period covered are presented.
    Keywords: GEOPHYSICS
    Type: NASA-TM-73283
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  • 41
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    Investigation of infrared spectra of atmospheric gases to support stratospheric spectroscopic investigations (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: Four papers are presented which discuss the following: information measures in nonlinear experimental design; information in spectra of collision broadened absorption lines; band analysis by spectral curve fitting; and least squares analysis of Voight shaped lines. Abstracts of five research papers on which the author collaborated and which were delivered at the 34th Symposium of Molecular Spectroscopy (Ohio State University, June 1979) are included along with a subroutine for use with BMDP3R to retrieve the parameters of 10 Voight shaped lines.
    Keywords: GEOPHYSICS
    Type: NASA-CR-158716
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  • 42
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    Studies of radiative transfer in the earth's atmosphere with emphasis on the influence of the radiation budget in the joint institute for advancement of flight sciences at the NASA-Langley Research Center (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: Earth and solar radiation budget measurements were examined. Sensor calibration and measurement accuracy were emphasized. Past works on the earth's radiation field that must be used in reducing observations of the radiation field were reviewed. Using a finite difference radiative transfer algorithm, models of the angular and spectral dependence of the earth's radiation field were developed.
    Keywords: GEOPHYSICS
    Type: NASA-CR-158690
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  • 43
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    Transfer of solar radiation in the atmosphere (1979)
    In:  Other Sources
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    Publication Date: 2019-07-13
    Description: Current needs in the field of atmospheric radiative transfer include the development and validation of fast but accurate calculation techniques for use in climate modeling. Progress toward meeting these needs can be made by application of existing computational techniques and use of observational data for radiation transfer across the earth-atmosphere system boundaries. In this study radiative transfer model simulations are compared to satellite observations of reflected solar radiation. Calculations are presented from both detailed and approximate transfer models for the solar radiation reflected from the earth-atmosphere system. These calculations are compared with the measurements made by the Earth Radiation Budget (ERB) experiment on Nimbus 6 in August 1975. Results show good agreement between simulations and observations.
    Keywords: GEOPHYSICS
    Type: AIAA PAPER 79-1038 , American Institute of Aeronautics and Astronautics, Thermophysics Conference; Jun 04, 1979 - Jun 06, 1979; Orlando, FL
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  • 44
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    Synthesis of regional crust and upper-mantle structure from seismic and gravity data (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: Available seismic and ground based gravity data are combined to infer the three dimensional crust and upper mantle structure in selected regions. This synthesis and interpretation proceeds from large-scale average models suitable for early comparison with high-altitude satellite potential field data to more detailed delineation of structural boundaries and other variations that may be significant in natural resource assessment. Seismic and ground based gravity data are the primary focal point, but other relevant information (e.g. magnetic field, heat flow, Landsat imagery, geodetic leveling, and natural resources maps) is used to constrain the structure inferred and to assist in defining structural domains and boundaries. The seismic data consists of regional refraction lines, limited reflection coverage, surface wave dispersion, teleseismic P and S wave delay times, anelastic absorption, and regional seismicity patterns. The gravity data base consists of available point gravity determinations for the areas considered.
    Keywords: GEOPHYSICS
    Type: NASA-CR-165001
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  • 45
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    Reduction and analysis of ATS-6 data (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: The scientific and technological results obtained by an energetic particle spectrometer are summarized. Data on energetic electrons trapped in the Earth's radiation belt near synchronous altitude and on solar particles penetrating to this altitude are discussed.
    Keywords: GEOPHYSICS
    Type: NASA-CR-160052 , ATR-79(7642)-3
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  • 46
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    Magnetospheric reconnection, substorms, and energetic particle acceleration (1979)
    In:  Other Sources
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    Publication Date: 2019-07-13
    Description: The steady state reconnection model of the terrestrial magnetosphere predicts a maximum potential drop of about 100 kV across the tail. During substorms particles are accelerated to energies above 1 MeV. At substorm onset, large inductive emfs may be generated by explosive tearing mode reconnection which is driven nonlinearly unstable by the solar wind and convection stresses on the tail plasma sheet. In the inner magnetosphere, energetic particles are also produced by stochastic wave turbulent acceleration and by convection driven inward radial diffusion.
    Keywords: GEOPHYSICS
    Type: Particle acceleration mechanisms in astrophysics; Jan 03, 1979 - Jan 05, 1979; La Jolla, CA
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  • 47
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    Acceleration in the earth's auroral magnetosphere below 1 R/E/ (1979)
    In:  Other Sources
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    Publication Date: 2019-07-13
    Description: Particle acceleration in the auroral magnetosphere is treated as a combination of d.c. electric field acceleration and wave heating in order to explain observed oblique pitch angle distributions of ions. Coherent electrostatic ion cyclotron waves which have been observed in the acceleration region saturate by ion trapping and thereby heat ions from the initial ionospheric temperatures of less than 1 eV to keV in perpendicular energy. Some of this is converted to parallel energy by the dipole mirror force and mixed with parallel acceleration in d.c. electric fields to produce the observed upstreaming conical pitch distributions of ions.
    Keywords: GEOPHYSICS
    Type: Particle acceleration mechanisms in astrophysics; Jan 03, 1979 - Jan 05, 1979; La Jolla, CA
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  • 48
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    Gravity anomalies near the east Pacific rise with wavelengths shorter than 3300 km recovered from GEOS-3 satellite-to-satellite Doppler tracking data (1979)
    In:  Other Sources
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    Publication Date: 2019-07-13
    Keywords: GEOPHYSICS
    Type: The use of artificial satellites for geodesy and geodynamics. Volume 2; May 29, 1978 - Jun 02, 1978; Athens; Greece
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  • 49
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    Some aspects of stratospheric chemical response to solar particle precipitations. I - Potential roles of N2/A3Sigma/ and ion-chemistry (1979)
    In:  Other Sources
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    Publication Date: 2019-07-13
    Description: Large amounts of long lived N2(A3Sigma) are created by the energy degradation of precipitating solar particles. Laboratory data suggest that in the stratosphere N2(A3Sigma) are efficiently converted into N2O. Through reactions with O(1D), N2O may gradually release NO and thereby influence the long term aspects of stratospheric chemical response. During the daytime, negative ions may transform an active NO(x) into an inactive HNO3. At night both negative and positive ion chemistry generate HO(x). Omission of ionic chemistry results in considerable underestimation of O3 depletion during the initial phases of solar particle events, and thereby introduces significant error in the estimation of the nature of the prompt response.
    Keywords: GEOPHYSICS
    Type: Solar-terrestrial influences on weather and climate; Aug 24, 1978 - Aug 28, 1978; Columbus, OH
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  • 50
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    Energy deposition in the earth's atmosphere due to impact of solar activity-generated disturbances (1979)
    In:  Other Sources
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    Publication Date: 2019-07-13
    Description: Energy deposition in and dynamic responses of the terrestrial atmosphere to solar flare-generated shocks and other physical processes - such as particle precipitation and local heating - are investigated self-consistently in the context of hydrodynamics, the problem being treated as an initial boundary-value problem. It is extremely difficult to construct a general model for the line solar activity-magnetosphere-atmosphere; however, a limited model for this link is possible. The paper describes such a model, and presents some results on energy deposition into the earth's atmosphere due to solar activity-generated disturbances. Results from the present calculations are presented and discussed.
    Keywords: GEOPHYSICS
    Type: Solar-terrestrial influences on weather and climate; Aug 24, 1978 - Aug 28, 1978; Columbus, OH
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  • 51
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    Longitudinal variation of the high altitude X-ray flux during quiet geomagnetic conditions (1979)
    In:  Other Sources
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    Publication Date: 2019-07-13
    Keywords: GEOPHYSICS
    Type: In: Space research XIX; May 29, 1978 - Jun 10, 1978; Innsbruck; Austria
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  • 52
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    Motions of charged particles in the Magnetosphere under the influence of a time-varying large scale convection electric field (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: The motions of charged particles under the influence of the geomagnetic and electric fields were quite complex in the region of the inner magnetosphere. The Volland-Stern type large scale convection electric field was used successfully to predict both the plasmapause location and particle enhancements determined from Explorer 45 measurements. A time dependence in this electric field was introduced based on the variation in Kp for actual magnetic storm conditions. The particle trajectories were computed as they change in this time-varying electric field. Several storm fronts of particles of different magnetic moments were allowed to be injected into the inner magnetosphere from L = 10 in the equatorial plane. The motions of these fronts are presented in a movie format.
    Keywords: GEOPHYSICS
    Type: NASA-TM-79699 , Chapman Conf.: Quantitative Modeling of Magnetospheric Processes; Sep 19, 1978 - Sep 22, 1978; La Jolla, CA; United States
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  • 53
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    Ionospheric research (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: Projects currently in progress on ionospheric research are described. General topics discussed include: planetary atmospheres, the ionosphere and its region, and mass spectroscopy.
    Keywords: GEOPHYSICS
    Type: NASA-CR-158762 , PSU-IRL-SAR-79/1 , SASR-1
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  • 54
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    Middle atmosphere electrodynamics: Report of the workshop on the Role of the Electrodynamics of the Middle Atmosphere on Solar Terrestrial Coupling (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: Significant deficiencies exist in the present understanding of the basic physical processes taking place within the middle atmosphere (the region between the tropopause and the mesopause), and in the knowledge of the variability of many of the primary parameters that regulate Middle Atmosphere Electrodynamics (MAE). Knowledge of the electrical properties, i.e., electric fields, plasma characteristics, conductivity and currents, and the physical processes that govern them is of fundamental importance to the physics of the region. Middle atmosphere electrodynamics may play a critical role in the electrodynamical aspects of solar-terrestrial relations. As a first step, the Workshop on the Role of the Electrodynamics of the Middle Atmosphere on Solar-Terrestrial Coupling was held to review the present status and define recommendations for future MAE research.
    Keywords: GEOPHYSICS
    Type: NASA-CP-2090 , Jan 17, 1979 - Jan 19, 1979; Reston, VA; United States
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  • 55
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    Polar motion from laser range measurements of GEOS-3 (1979)
    In:  Other Sources
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    Publication Date: 2019-07-13
    Description: Using two-day arcs of GEOS-3 laser data, simultaneous solutions for pole position components, x sub p and y sub p, and orbit elements have been obtained for the period spanning 3 February to 6 March 1976 using three NASA Goddard Space Flight Center laser stations located near Washington, D.C. (STALAS) and on the islands of Bermuda and Grand Turk. The results are in general agreement with the BIH results. However, because of the locations of the laser sites, the x sub p solution is weaker than the y sub p solution. The x sub p and y sub p estimates were smoothed with a straight line by weighted least squares using the variance associated with the pole estimates as weights in order to reflect the effect of widely different data distributions. The smoothed y sub p differs by one meter with respect to the BIH smoothed values and the smoothed x sub p differs by about two meters. Spectral analysis of the results has identified frequencies associated with the orbital motion indicating the need for further improvements in the model of the physical system.
    Keywords: GEOPHYSICS
    Type: Time and the earth''s rotation; Eighty-second Symposium; May 08, 1978 - May 12, 1978; San Fernando; Spain
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  • 56
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    Determination of polar motion and earth rotation from laser tracking of satellites (1979)
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    Publication Date: 2019-07-13
    Description: Laser tracking of the Lageos spacecraft has been used to derive the position of the earth's pole of rotation at intervals during October, November and December 1976. The estimated precision of the results is 0.01 to 0.02 arcseconds in both x and y components, although the formal uncertainty is an order of magnitude better, and there is general agreement with the Bureau International de l'Heure smoothed pole path to about 0.02 arcseconds. Present orbit determination capability of Lageos is limited to about 25 cm rms fit to data over periods of 5 days and about 50 cm over 50 days. The present major sources of error in the perturbations of Lageos are earth and ocean tides followed by the earth's gravity field, and solar and earth reflected radiation pressure. Ultimate accuracy for polar motion and earth rotation from Lageos after improved modeling of the perturbing forces appears to be of order + or - 5 cm for polar motion over a period of about one day and about + or - 0.2 to + or - 0.3 milliseconds in UT for periods up to 2 or 3 months.
    Keywords: GEOPHYSICS
    Type: Time and the earth''s rotation; Eighty-second Symposium; May 08, 1978 - May 12, 1978; San Fernando; Spain
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  • 57
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    Ionospheric research (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: Research projects in progress are reported. These include: planetary atmospheres, E- and F-region, and D-region.
    Keywords: GEOPHYSICS
    Type: NASA-CR-158759 , PSU-IRL-SAR-79/1 , SASR-1
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  • 58
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    Bibliography of geologic studies using imaging radar (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: Articles concerning imaging studies on the geomorphology, mineralogy, and topology of various landforms are reported. One hundred and ninety citations are listed and an index by National Technical Information service citation number is included. Several illustrations of L-band radar imagery are presented.
    Keywords: GEOPHYSICS
    Type: NASA-CR-158820 , JPL-PUB-79-53 , NASA/JPL Radar Geology Workshop; Jul 16, 1979 - Jul 20, 1979; Snowmass, CO; United States
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  • 59
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    Theoretical studies of the transport and removal processes of Sahara dust (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: The processes controlling the evolution of aerosol particles may be divided into dynamic processes concerned with the motions of air currents and microphysical processes concerned with the growth of the individual particles. The Ames planetary boundary layer model was modified to construct a subsynoptic scale aerosol model to study the long term fate of the Saharan dust. The transport model consists of a mixed layer, a convection layer, and free atmosphere. Conditions used for a preliminary test run and results obtained are described.
    Keywords: GEOPHYSICS
    Type: NASA-CR-162332
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  • 60
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    Geochemical data synthesis and analysis (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: Data obtained at the Goddard Flight Center were collected for the purpose of completing analyses started at Goddard in order to maximize the scientific yield of the geochemistry program which was terminated in 1977. The major analytical task undertaken was to complete Gd analyses on a large number of samples already analyzed by mass spectrometry for other rare earth element abundances at Goddard. Gd values are important for pinning down the central part of the geochemically significant rare earth abundance pattern and are especially useful in the high precision definition of the utilitarian Eu anomaly. Isotope-dilution Gd abundances were obtained for 39 samples. The data are for 27 partition-coefficient samples, six Apollo 15 and 16 breccia samples, four terrestrial impactities, and associated rock standards.
    Keywords: GEOPHYSICS
    Type: NASA-CR-158231
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  • 61
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    Magnetopause structure from satellite observations (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: Observations on magnetopause structure are reported. Major topics covered include: classical reconnection, transport mechanisms, magnetospheric boundary layers, tearing modes, and Jupiter's magnetopause.
    Keywords: GEOPHYSICS
    Type: NASA-CR-162286
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  • 62
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    ATMOS Spacelab 1 science investigation (1979)
    In:  CASI
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    Publication Date: 2019-07-13
    Description: Existing infrared spectra from high speed interferometer balloon flights were analyzed and experimental analysis techniques applicable to similar data from the ATMOS experiment (Spacelab 3) were investigated. Specific techniques under investigation included line-by-line simulation of the spectra to aid in the identification of absorbing gases, simultaneous retrieval of pressure and temperature profiles using carefully chosen pairs of CO2 absorption lines, and the use of these pressures and temperatures in the retrieval of gas concentration profiles for many absorbing species. A search for a new absorption features was also carried out, and special attention was given to identification of absorbing gases in spectral bandpass regions to be measured by the halogen occultation experiment.
    Keywords: GEOPHYSICS
    Type: NASA-TM-80465
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  • 63
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    Proceedings: Workshop on the Need for Lightning Observations from Space (1979)
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    Publication Date: 2019-07-13
    Description: The results of the Workshop on the Need for Lightning Observations from Space held February 13-15, 1979, at the University of Tennessee Space Institute, Tullahoma, Tennessee are presented. The interest and active involvement by the engineering, operational, and scientific participants in the workshop demonstrated that lightning observations from space is a goal well worth pursuing. The unique contributions, measurement requirements, and supportive research investigations were defined for a number of important applications. Lightning has a significant role in atmospheric processes and needs to be systematically investigated. Satellite instrumentation specifically designed for indicating the characteristics of lightning are of value in severe storms research, in engineering and operational problem areas, and in providing information on atmospheric electricity and its role in meteorological processes.
    Keywords: GEOPHYSICS
    Type: NASA-CP-2095 , Feb 13, 1979 - Feb 15, 1979; Tullahoma, TN; United States
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  • 64
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    Gravitational field models for study of Earth mantle dynamics (1979)
    In:  CASI
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    Publication Date: 2019-06-28
    Description: The tectonic forces or stresses due to the small scale mantle flow under the South American plate are detected and determined by utilizing the harmonics of the geopotential field model. The high degree harmonics are assumed to describe the small scale mantle convection patterns. The input data used in the derivation of this model is made up of 840,000 optical, electronic, and laser observations and 1,656 5 deg x 5 deg mean free air anomalies. Although there remain some statistically questionable aspects of the high degree harmonics, it seems appropriate now to explore their implications for the tectonic forces or stress field under the crust.
    Keywords: GEOPHYSICS
    Type: NASA-CR-160083 , NO-R-SAP-8-79-01
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  • 65
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    Ion and electron temperatures in the topside ionosphere (1979)
    In:  CASI
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    Publication Date: 2019-06-28
    Description: Experimental and theoretical ion and electron temperatures in the topside ionosphere were investigated. Experimental results came from an analysis of incoherent scatter data taken at Arecibo, Puerto Rico. Consideration of the energy balance equations gave the theoretical ion and electron temperatures.
    Keywords: GEOPHYSICS
    Type: NASA-CR-163670 , UILU-ENG-79-2505 , AERONOMY-86
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    The damping of seismic waves and its determination from reflection seismograms (1979)
    In:  CASI
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    Publication Date: 2019-06-28
    Description: The damping in theoretical waveforms is described phenomenologically and a classification is proposed. A method for studying the Earth's crust was developed which includes this damping as derived from reflection seismograms. Seismic wave propagation by absorption, attenuation of seismic waves by scattering, and dispersion relations are considered. Absorption of seismic waves within the Earth as well as reflection and transmission of elastic waves seen through boundary layer absorption are also discussed.
    Keywords: GEOPHYSICS
    Type: TUBS/GAMMA-36
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  • 67
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    Advanced development of atmospheric models (1979)
    In:  CASI
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    Publication Date: 2019-06-28
    Description: A set of atmospheric analysis and prediction models was developed in support of the SEASAT Program existing objective analysis models which utilize a 125x125 polar stereographic grid of the Northern Hemisphere, which were modified in order to incorporate and assess the impact of (real or simulated) satellite data in the analysis of a two-day meteorological scenario in January 1979. Program/procedural changes included: (1) a provision to utilize winds in the sea level pressure and multi-level height analyses (1000-100 MBS); (2) The capability to perform a pre-analysis at two control levels (1000 MBS and 250 MBS); (3) a greater degree of wind- and mass-field coupling, especially at these controls levels; (4) an improved facility to bogus the analyses based on results of the preanalysis; and (5) a provision to utilize (SIRS) satellite thickness values and cloud motion vectors in the multi-level height analysis.
    Keywords: GEOPHYSICS
    Type: NASA-CR-166630
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    Two-dimensional zonal mean flow model (1979)
    In:  CASI
    Details
    Publication Date: 2019-06-28
    Description: The interactions of dynamics, photochemistry and radiation in the stratosphere can be described by the continuity, momentum, and energy equations. A more comprehensive model for stratospheric transport theory was developed for the purpose of aiding predictions of changes in the stratospheric ozone content as a consequence of natural and anthropogenic processes. This model is time dependent and the dependent variables are zonal means of the relevant meteorological quantities which are functions of latitude and height. The detailed formulation of a numerical model both in physics and mathematics is given. A set of fundamental dynamical equations, and the numerical method used in the integration are described.
    Keywords: GEOPHYSICS
    Type: NASA-CR-160071 , R-SAN-27901
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    A rocket-borne data-manipulation experiment using a microprocessor (1979)
    In:  CASI
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    Publication Date: 2019-06-28
    Description: The development of a data-manipulation experiment using a Z-80 microprocessor is described. The instrumentation is included in the payloads of two Nike Apache sounding rockets used in an investigation of energetic particle fluxes. The data from an array of solid-state detectors and an electrostatic analyzer is processed to give the energy spectrum as a function of pitch angle. The experiment performed well in its first flight test: Nike Apache 14.543 was launched from Wallops Island at 2315 EST on 19 June 1978. The system was designed to be easily adaptable to other data-manipulation requirements and some suggestions for further development are included.
    Keywords: GEOPHYSICS
    Type: NASA-CR-158647 , UILU-ENG-79-2503 , AERONOMY-84 , (ISSN 0568-0581)
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    Rocket radio measurement of electron density in the nighttime ionosphere (1979)
    In:  CASI
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    Publication Date: 2019-06-28
    Description: One experimental technique based on the Faraday rotation effect of radio waves is presented for measuring electron density in the nighttime ionosphere at midlatitudes. High frequency linearly-polarized radio signals were transmitted to a linearly-polarized receiving system located in a spinning rocket moving through the ionosphere. Faraday rotation was observed in the reference plane of the rocket as a change in frequency of the detected receiver output. The frequency change was measured and the information was used to obtain electron density data. System performance was evaluated and some sources of error were identified. The data obtained was useful in calibrating a Langmuir probe experiment for electron density values of 100/cu cm and greater. Data from two rocket flights are presented to illustrate the experiment.
    Keywords: GEOPHYSICS
    Type: NASA-CR-157442 , UILU-ENG-79-2504 , AERONOMY-85 , (ISSN 0568-0581)
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    A rocket-borne pulse-height analyzer for energetic particle measurements (1979)
    In:  CASI
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    Publication Date: 2019-06-28
    Description: The pulse-height analyzer basically resembles a time-sharing multiplexing data-acquisition system which acquires analog data (from energetic particle spectrometers) and converts them into digital code. The PHA simultaneously acquires pulse-height information from the analog signals of the four input channels and sequentially multiplexes the digitized data to a microprocessor. The PHA together with the microprocessor form an on-board real-time data-manipulation system. The system processes data obtained during the rocket flight and reduces the amount of data to be sent back to the ground station. Consequently the data-reduction process for the rocket experiments is speeded up. By using a time-sharing technique, the throughput rate of the microprocessor is increased. Moreover, data from several particle spectrometers are manipulated to share one information channel; consequently, the TM capacity is increased.
    Keywords: GEOPHYSICS
    Type: NASA-CR-158645 , UILU-ENG-79-2502 , AERONOMY-83 , (ISSN 0568-0581)
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  • 72
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    A rocket-borne electrostatic analyzer for measurement of energetic particle flux (1979)
    In:  CASI
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    Publication Date: 2019-06-28
    Description: A rocket-borne electrostatic analyzer experiment is described. It is used to measure energetic particle flux (0.9 to 14 keV) in the nighttime midlatitude E region. Energetic particle precipitation is believed to be a significant nighttime ionization source, particularly during times of high geomagnetic activity. The experiment was designed for use in the payload of a Nike Apache sounding rocket. The electrostatic analyzer employs two cylindrical parallel plates subtending a central angle of 90 deg. The voltage waveform supplied to the plates is a series of steps synchronized to the spin of the payload during flight. Both positive and negative voltages are provided, extending the detection capabilities of the instrument to both electrons and protons (and positive ions). The development, construction and operation of the instrument is described together with a preliminary evaluation of its performance in a rocket flight.
    Keywords: GEOPHYSICS
    Type: NASA-CR-158646 , UILU-ENG-79-2501 , AERONOMY-82 , (ISSN 0568-0581)
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  • 73
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    Enhanced CO2 greenhouse to compensate for reduced solar luminosity on early Earth (1979)
    In:  CASI
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    Publication Date: 2019-06-28
    Keywords: GEOPHYSICS
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  • 74
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    A technique for determining daytime atmospheric oxide above 50 km from backscattered ultraviolet measurements (1979)
    In:  CASI
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    Publication Date: 2019-06-28
    Description: Airglow from gamma band resonance fluorescence of nitric oxide near 255 nm is calculated at several solar zenith angles. Data from the Nimbus 4 BUV wavelengths 273.5 to 287.6 nm is used to estimate the Rayleigh and ozone scattering contributions to the BUV 255.5 nm data and the remaining signal is attributed to NO airglow. The low solar zenith angle contributions by NO is less than 0.5%, and the high latitude/high zenith angle contribution exceeds 5%. This technique allows for estimating NO content above 50 km, as well as partitioning that content between the mesosphere and thermosphere.
    Keywords: GEOPHYSICS
    Type: NASA-TM-80325 , NAS 1.15:80325
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  • 75
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    Initial ISEE observations of the bow shock (1979)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: ISEE 1 and 2 magnetic-field profiles across three terrestrial bow shock crossings are shown to illustrate the control of the bow shock structure and upstream waves by solar-wind conditions, especially by the direction of the interplanetary field. The quasi-perpendicular shocks examined have thicknesses of the order of a ion inertial length. Upstream waves observed for field directions of about 45 deg to the shock normal are observed to be carried back towards the bow shock by the solar wind, while propagating upstream at what appears to be the magnetosonic velocity. These studies are continuing.
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    The equatorial total electron content and shape factor (1979)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: The diurnal variations of electron content and shape factor observed at an equatorial station during sunspot minimum are shown to be consistent with the electron density profiles observed at Jicamarca during sunspot minimum. The rapid increase in electron content and the shape factor at sunrise results from the EUV production of ionization in the E and F regions. Day-to-day variations in daytime electron content are observed to be quite small at the equator. The evening decrease in the shape factor results from an upward drift of the F region at sunset and the evening decay of the E and bottomside F regions. The nighttime peak or plateau in the shape factor is produced by the slow downward drift of the electron density profile. The deep predawn dip in the shape factor is caused by the main peak of the F layer reaching low altitudes where high loss rates cause a large reduction in ionization below 300 km and very flat electron density profile.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 84; Dec. 1
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  • 77
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    A quasi-static model of global atmospheric electricity. II - Electrical coupling between the upper and lower atmosphere (1979)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: The paper presents a model of global atmospheric electricity used to examine the effect of upper atmospheric generators on the global electrical circuit. The model represents thunderstorms as dipole current generators randomly distributed in areas of known thunderstorm frequency; the electrical conductivity in the model increases with altitude, and electrical effects are coupled with a passive magnetosphere along geomagnetic field lines. The large horizontal-scale potential differences at ionospheric heights map downward into the lower atmosphere where the perturbations in the ground electric field are superimposed on the diurnal variation. Finally, changes in the upper atmospheric conductivity due to solar flares, polar cap absorptions, and Forbush decreases are shown to alter the downward mapping of the high-latitude potential pattern and the global distribution of fields and currents.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 84; Dec. 1
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  • 78
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    Height dependence of spread F bubble drift velocities (1979)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: Vertical bubble velocities in equatorial spread F have been investigated analytically by Ott (1978), Osakow and Chaturvedi (1978), all of whom found a proportionality of the vertical velocity to bubble depletion density. The paper presents radar data from two equatorial sites which support theoretical predictions that vertical drift velocities of spread F bubbles increase with height on the bottomside of the F layer. This increase is shown to result from the proportionality of bubble drift velocity to density depletion amplitude, which itself increases with height. The measured rate of increase is found to be dU/dh equals about 2 m/s km. It is concluded that this is consistent with numerical simulation results within a factor of 2.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 84; Dec. 1
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  • 79
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    Digital processing of ionospheric electron content data (1979)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: Ionospheric electron content data contain periodicities that are produced by a diversity of sources including hydromagnetic waves, gravity waves, and lunar tides. Often these periodicities are masked by the strong daily variation in the data. Digital filtering can be used to isolate the weaker components. The filtered data can then be further processed to provide estimates of the source properties. In addition, homomorphic filtering may be used to identify nonlinear interactions in the ionosphere.
    Keywords: GEOPHYSICS
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    Ultraviolet absorption spectrum of methylhydroperoxide vapor (1979)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: The ultraviolet absorption cross sections of methylhydroperoxide, CH3OOH, have been measured over the wavelength range 210 nm to 350 nm at 294 K. It was concluded that solar photolysis is a dominant sink for tropospheric CH3OOH. For midlatitudes the photodissociation rate was estimated for 0 deg, for 30 deg, and for 70 deg zenith angles.
    Keywords: GEOPHYSICS
    Type: Geophysical Research Letters; 6; Dec. 197
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  • 81
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    Counterstreaming of O+ and H+ ions in the plasmasphere (1979)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: Although the ion flux along plasmaspheric flux tubes has been both measured and numerically modeled for many years, it is only recently that H(+)-O(+) counterstreaming, with O(+) upwards, has been studied. The theoretical studies indicate that counterstreaming occurs under special conditions primarily near twilight. It is shown that such counterstreaming arises not only from a combination of particular conditions but is a more fundamental characteristic of the flow of plasma in the closed field-line magnetosphere. The causes of counterstreaming are analyzed showing that it must occur under steady state conditions; it is also shown how diurnal variations modify the steady state pattern.
    Keywords: GEOPHYSICS
    Type: Geophysical Research Letters; 6; Dec. 197
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  • 82
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    Field-aligned current sources in the high-latitude ionosphere (1979)
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    Publication Date: 2019-06-27
    Description: The paper determines the electric potential in a plane which is fed current from a pair of field-aligned current sheets. The ionospheric conductivity is modelled as a constant with an enhanced conductivity annular ring. It is shown that field-aligned current distributions are arbitrary functions of azimuth angle (MLT) and thus allow for asymmetric potential configurations over the pole cap. In addition, ionospheric surface currents are computed by means of stream functions. Finally, the discussion relates these methods to the electrical characteristics of the magnetosphere.
    Keywords: GEOPHYSICS
    Type: Annales de Geophysique; 35; July-Sep
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  • 83
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    Release adiabat measurements on minerals - The effect of viscosity (1979)
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    Publication Date: 2019-06-27
    Description: The paper examines the effect of viscosity in the release adiabat measurements on minerals. The current inversion of pressure-particle velocity data for release from a high-pressure shock state to a pressure-density path usually depends critically upon the assumption that the release process is isentropic. It has been shown that the effective viscosity for geological materials below stresses of 150 GPa must be at least 1000 kg/m/s so that viscous work in the shock state remains small compared to mechanical work recovered upon adiabatic rarefaction. The magnitude of the shear stress in the shock state in minerals and viscosities of engineering materials shocked to pressures below 150 GPa show effective viscosities of about 1000 kg/m/s or less indicating that the conditions for isentropic release of materials from shock states are achieved and that the Riemann integral can be applied to obtain pressure-density states along the release adiabats of minerals.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 84; Dec. 10
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  • 84
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    Acoustic fluidization - A new geologic process (1979)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: A number of geologic processes, particularly seismic faulting, impact crater slumping, and long runout landslides, require the failure of geologic materials under differential stresses much smaller than expected on the basis of conventional rock mechanics. This paper proposes that the low strengths apparent in these phenomena are due to a state of 'acoustic fluidization' induced by a transient strong acoustic wave field. The strain rates possible in such a field are evaluated, and it is shown that acoustically fluidized debris behaves as a newtonian fluid with a viscosity in the range 100,000 to 10,000,000 P for plausible conditions. Energy gains and losses in the acoustic field are discussed, and the mechanism is shown to be effective if internal dissipation in the field gives a Q approximately greater than 100. Whether such values for Q are realized is not known at present. However, acoustic fluidization provides a qualitatively correct description of the failure of rock debris under low differential stresses in the processes of faulting, crater slumping, and long runout landslides. Acoustic fluidization thus deserves serious consideration as a possible explanation of these phenomena.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 84; Dec. 10
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  • 85
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    The mean age of mantle and crustal reservoirs (1979)
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    Publication Date: 2019-06-27
    Description: An analysis of two transport models for trace elements in mantle and crust evolution and related to the observed abundance patterns. In model I, continents are derived by melt extraction over the earth history from undepleted mantle, and the residue forms a depleted mantle which is the current source of mid-ocean ridge basalts. In model II, new additions to continents are derived from a mantle reservoir 2, which becomes more depleted by repeated extraction of melts. The isotopic composition and concentrations of trace elements are shown to reduce to simple mathematical expressions which permit calculations of basic evolutionary parameters. The mean age of the crust mass and isotopic data for the continental crust and the mantle are discussed, concluding with a consideration of their difference in compositions of newly derived crust.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 84; Dec. 10
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  • 86
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    Shape integral method for magnetospheric shapes (1979)
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    Publication Date: 2019-06-27
    Description: A method is developed for calculating the shape of any magnetopause to arbitrarily high precision. The method uses an integral equation which is evaluated for a trial shape. The resulting values of the integral equation as a function of auxiliary variables indicate how close one is to the desired solution. A variational method can then be used to improve the trial shape. Some potential applications are briefly mentioned.
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    Global magnetohydrodynamic simulation of the two-dimensional magnetosphere (1979)
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    Publication Date: 2019-06-27
    Description: The time-dependent magnetohydrodynamic interaction of the solar wind with a two-dimensional dipole magnetic field has been simulated using a novel Lagrangian particle type of MHD code that can treat local low density or vacuum regions without numerical instability. This enables one to simulate the time-dependent magnetic tail. When the solar wind field is southward, a magnetic field line topology consistent with Dungey's model emerges in steady state. The tail, however, is short, and the x-points are only slightly shifted from their vacuum locations, because of strong numerical resistivity. Different configurations resulting from different relative orientations of the solar wind magnetic field and dipole axis are also presented. While the magnetic field is relatively steady, the density and flow in the magnetosheath are turbulent, as are the bow shock and magnetopause; the Kelvin-Helmholtz instability may account for these phenomena. We also model a 'substorm' as the passage of a rotational discontinuity in the solar wind over the dipole. Both 90 and 180 deg shifts to a southward solar wind field cause a violent readjustment of the magnetic tail which eventually settles down to the Dungey configuration.
    Keywords: GEOPHYSICS
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    Computer modeling of events in the inner magnetosphere (1979)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: The first effort at computer simulating the behavior of the inner magnetosphere during a substorm-type event on 19 September 1976 was completed. The computer model simulates many aspects of the behavior of the closed-field-line portion of the earth's magnetosphere, and the auroral and subauroral ionosphere. For these regions, the program self-consistently computes electric fields, electric currents, hot-plasma densities, plasma flow velocities and other parameters. Highlights of the results of our event simulation are presented. Predicted electric fields for several times during the event agree reasonably well with corresponding data from satellite S3-2. Detailed discussion is presented for a case of rapid subauroral flow that was observed on one S3-2 pass and is predicted by the computer runs. The computed global distribution of Birkeland current agrees reasonably well with the observations of Iijima and Potemra.
    Keywords: GEOPHYSICS
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    A kinetic approach to magnetospheric modeling (1979)
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    Publication Date: 2019-06-27
    Description: The earth's magnetosphere is caused by the interaction between the flowing solar wind and the earth's magnetic dipole, with the distorted magnetic field in the outer parts of the magnetosphere due to the current systems resulting from this interaction. It is surprising that even the conceptually simple problem of the collisionless interaction of a flowing plasma with a dipole magnetic field has not been solved. A kinetic approach is essential if one is to take into account the dispersion of particles with different energies and pitch angles and the fact that particles on different trajectories have different histories and may come from different sources. Solving the interaction problem involves finding the various types of possible trajectories, populating them with particles appropriately, and then treating the electric and magnetic fields self-consistently with the resulting particle densities and currents. This approach is illustrated by formulating a procedure for solving the collisionless interaction problem on open field lines in the case of a slowly flowing magnetized plasma interacting with a magnetic dipole.
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    Empirical relationships between interplanetary conditions, magnetospheric flux transfer, and the AL index (1979)
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    Publication Date: 2019-06-27
    Description: Holzer and Slavin (1978) have found that the transfer of magnetic flux to and from the dayside magnetosphere as inferred from observed displacements of the magnetopause surface is correlated with both the magnitude of the auroral zone magnetic index AL and the incident flux of southward IMF. Empirical expressions specifying the rate at which magnetic flux is eroded in terms of interplanetary parameters and the rate of magnetic flux return as a function of AL have been developed. These relations are then used to predict magnetotail magnetic field enhancements from interplanetary and ground based data during an interval of substorm activity. The total magnetic flux in the tail is increased during intervals when the amount of flux transferred into its volume by dayside erosion exceeds the flux lost to the dayside by magnetospheric convection. Using Ogo-5 tail observations it is found for the sample events considered that these magnetic field enhancements can be described by empirical expressions for the magnetic flux transfer rates.
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    Generation of the magnetospheric electric field (1979)
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    Publication Date: 2019-06-27
    Description: The potential electric field in the magnetosphere satisfies two boundary conditions, the outer boundary being the magnetosphere/solar-wind interface (magnetopause) and the inner boundary being the magnetosphere/atmosphere interface (ionosphere). The distribution of the imposed potential between the two boundaries affects, and is affected by, the configuration and motion of plasma in the magnetosphere. The paper surveys various mechanisms that are suspected of playing a role in the establishment of the boundary conditions on the magnetospheric electric field.
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    Effects of the solar wind on magnetospheric dynamics - Energetic electrons at the synchronous orbit (1979)
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    Publication Date: 2019-06-27
    Description: Data on energetic electron fluxes at the synchronous orbit, covering the 1967-1978 time interval, obtained by experiments flown on the ATS-1, ATS-5 and ATS-6 spacecraft, have been analyzed. Long term (year) and short term (days) electron flux averages are found to correlate positively with corresponding averages of the solar wind velocity.
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    The synchronous orbit magnetic field data set (1979)
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    Publication Date: 2019-06-27
    Description: The magnetic field at synchronous orbit is the result of superposition of fields from many sources such as the earth, the magnetopause, the geomagnetic tail, the ring current and field-aligned currents. In addition, seasonal changes in the orientation of the earth's dipole axis causes significant changes in each of the external sources. Main reasons for which the synchronous orbit magnetic field data set is a potentially valuable resource are outlined. The primary reason why synchronous magnetic field data have not been used more extensively in magnetic field modeling is the presence of absolute errors in the measured fields. Nevertheless, there exists a reasonably large collection of synchronous orbit magnetic field data. Some of these data can be useful in quantitative modeling of the earth's magnetic field. A brief description is given of the spacecraft, the magnetometers, the standard graphical data displays, and the digital data files.
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    Prediction of the occurrence and intensity of magnetospheric substorms (1979)
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    Publication Date: 2019-06-27
    Description: The solar wind and IMF data obtained by the Venus probe Mariner 5 (at a distance of 460 earth radii) and by the earthbound Explorer 34 satellite, on June 24, 25, and 26, 1967 were examined. It is demonstrated that the occurrence and intensity of magnetospheric substorms can be predicted about 1-3 hours prior to their onsets by monitoring the energy coupling function at a distance of a few hundred earth radii upstream of the solar wind. It appears that the 'epsilon signal' propagates with different speeds, perhaps depending on the propagation time of disturbances which increase epsilon.
    Keywords: GEOPHYSICS
    Type: AD-A087362 , AFGL-TR-80-0224 , Geophysical Research Letters; 6; Nov. 197
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    Satellite observations of the spatial extent and structure of Pc 3, 4, 5 pulsations near the magnetospheric equator (1979)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: Simultaneous observations of Pc 3, 4, 5 pulsations by five satellites in the pre-noon local time sector at and near synchronous orbit are examined. The periods of these simultaneous pulsations are not the same at the different observation points. This difference is attributed to site dependent resonant conditions. The spatial properties of the temporal phenomenon are demonstrated with observations by ISEE-1 and -2 as they pass through oscillations in a spatially limited region. Fundamental and second harmonic standing Alfven waves are observed simultaneously on the same field line. The periods are consistent with model predictions when the measured plasma composition, which by mass consists mainly of singly ionized oxygen, is taken into account.
    Keywords: GEOPHYSICS
    Type: Geophysical Research Letters; 6; Nov. 197
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  • 96
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    The OI/1S/ state - Its quenching by O2 and formation by the dissociative recombination of vibrationally excited O2/+/ ions (1979)
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    Publication Date: 2019-06-27
    Description: The rate coefficient for the quenching of metastable O(1S) atoms by O2 was measured as a function of temperature from 250 to 550 K. The resulting Arrhenius expression correlates well with previous laboratory work. It is suggested that the much larger value of the rate coefficient inferred from an analysis of artificial auroral experiment, Precede, may be explained by overestimation of the contribution of O(1S) production from O2(+) dissociative recombination. The possibility that O(1S) atoms are produced only by the dissociative recombination of vibrationally excited O2(+) ions is examined; such excited ions would not exist in the Precede experiment because of the rapid cooling of the ions by resonant charge transfer processes.
    Keywords: GEOPHYSICS
    Type: Geophysical Research Letters; 6; Nov. 197
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    Solar activity and total atmospheric ozone (1979)
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    Publication Date: 2019-06-27
    Description: Analyses are presented of the association between two parameters of solar activity (Lyman-alpha and 10.7 cm flux) and global total ozone as determined from Nimbus observations for the period April-December 1970 (IRIS observations), and April 1970-April 1972 (BUV observations); and between Lyman-alpha and global total ozone as observed at ground stations and the ozone concentration in the lower and middle stratosphere in the subtropics for the period 1969-1972. It is shown that the high correlations discussed in other published studies between these solar paramters and nine months of IRIS data resulted from the use of a very limited, seasonally unfiltered data set.
    Keywords: GEOPHYSICS
    Type: Geophysical Research Letters; 6; Nov. 197
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    The concentration of atomic oxygen in the auroral lower thermosphere (1979)
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    Publication Date: 2019-06-27
    Description: A method is described to determine the concentration of atomic oxygen in the altitude range 100 to 160 km in an aurora from the ratio of the volume emission rates of the O(1S) 5577 A to N2(+) in 3914 A emissions. Applying the technique to previously published measurements it is found that the O density at 100 km is typically about 1 x 10 to the 11th per cu cm. The occurrence of densities in excess of 2 x 10 to the 11th per cu cm in the aurora at 100 km is rare.
    Keywords: GEOPHYSICS
    Type: Geophysical Research Letters; 6; Nov. 197
    Format: text
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    Latitudinal distribution of the sources of carbon monoxide in the troposphere (1979)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: A vertically and zonally averaged model of the troposphere has been constructed which calculates photochemical interactions and diffusive North-South transport of trace species. The model can be used to calculate the latitudinal distribution of the source function of a species if its concentration distribution is known. This procedure has been applied to carbon monoxide and large sources have been found outside the industrialized belt in the Northern Hemisphere.
    Keywords: GEOPHYSICS
    Type: Geophysical Research Letters; 6; Nov. 197
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    Actinometric measurements and theoretical calculations of j/O3/, the rate of photolysis of ozone to O/1D/ (1979)
    In:  Other Sources
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    Publication Date: 2019-06-27
    Description: The paper presents an experimental technique which measures j/O3-O(1-D)/, the rate of solar photolysis of ozone to singlet oxygen atoms. It is shown that a flow actinometer carries dilute O3 in N2O into direct sunlight where the O(1D) formed reacts with N2O to form NO which chemiluminescence detects, with a time resolution of about one minute. Measurements indicate a photolysis rate of 1.2 (+ or - .2) x 10 to the -5/s for a cloudless sky, 45 deg zenith angle, 0.345 cm ozone column and zero albedo. Finally, ground level results compare with theoretical calculations based on the UV actinic flux as a function of ozone column and solar zenith angle.
    Keywords: GEOPHYSICS
    Type: Geophysical Research Letters; 6; Nov. 197
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