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  • GEOPHYSICS  (10)
  • OCEANOGRAPHY  (2)
  • INSTRUMENTATION AND PHOTOGRAPHY
  • 1975-1979  (12)
  • 1
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    Magnetosphere-ionosphere interactions (1979)
    In:  CASI
    Details
    Publication Date: 2006-01-16
    Description: The present understanding of magnetosphere ionosphere interactions is described, and present and future predictive capabilities are assessed. Ionospheric features directly coupled to the magnetosphere to a significant degree are considered, with emphasis given to those phenomena of major interest to forecasters and users.
    Keywords: GEOPHYSICS
    Type: NASA. Marshall Space Flight Center Solar-Terrest. Predictions Proc., Vol. 2; p 476-493
    Format: text
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  • 2
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    Chemical releases (1978)
    In:  Other Sources
    Details
    Publication Date: 2011-08-18
    Description: A Chemical Release Module to be carried into orbit by the shuttle is described. The module would release chemicals from orbiting satellites in order understand processes within the Earth's magnetosphere, atmosphere and ionosphere. A large number of potential experiments are identified, ranging from introducing traceable material into the solar wind in order to study its transport to and within the magnetosphere, to injecting material into the outer magnetosphere to simulate the precipitation of trapped charged particles, to the release of material at lower altitudes to create waves both mechanical and electromagnetic.
    Keywords: GEOPHYSICS
    Type: Alabama Univ. UAH(NASA Workshop on the Use of a Tethered Satellite System; p 135-150
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  • 3
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    Auroral vector electric field and particle comparisons. I - Preliminary convection topology (1977)
    In:  Other Sources
    Details
    Publication Date: 2011-08-17
    Description: Data obtained by Polar 3, launched from northern Norway January 27, 1974, are interpreted. The rocket, which traversed nearly 3 deg of latitude, crossed over a stable IBC II auroral arc in the positive bay region and continued north to a convection boundary which has been identified as the Harang discontinuity. Measurements of the complete electric field vector, of energetic electrons, and of auroral emissions were used to study the convection topology in the premagnetic midnight region. The inverted V nature of the electron precipitations at the convection boundary, compared with the lack of such structure over the arc which was within the positive bay region, is thought to indicate that auroral arcs are likely to be associated with inverted V type precipitation only at or poleward of convection boundaries and their eddy structures.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 82; June 1
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  • 4
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    Auroral vector electric field and particle comparisons. II - Electrodynamics of an arc (1977)
    In:  Other Sources
    Details
    Publication Date: 2011-08-17
    Description: The paper reports the results of energetic auroral electron and vector electric field measurements taken near and above a discrete auroral form and discusses their electrodynamic implications. Height-integrated Hall and Pedersen conductivities are computed in a quantitative fashion along the rocket payload trajectory. These conductivities, together with the electric fields, are used to describe the local auroral electrojet current system and to demonstrate an inverse relationship between the local electric field intensity and the height-integrated Pedersen conductivity. An analysis is presented of the divergence of both the electric field and the horizontal current as an effort to infer space charge densities and magnetic-field-aligned electrical currents near an auroral arc.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 82; June 1
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  • 5
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    A point target model for the synthetic aperture radar detection of ships and ice conditions during a swell (1979)
    In:  Other Sources
    Details
    Publication Date: 2011-08-17
    Description: A running swell affects the synthetic aperture radar (SAR) imagery of ships, smaller icebergs, and other floating objects because the targets signal is no longer matched with the azimuth processor. This effect is analyzed analytically and numerically for the case of conventional image processing.
    Keywords: OCEANOGRAPHY
    Type: IEEE Transactions on Antennas and Propagation; AP-27; Jan. 197
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  • 6
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    Future monitoring of charged particle energy deposition into the upper atmosphere and comments on possible relationships between atmospheric phenomena and solar and/or geomagnetic activity (1975)
    In:  CASI
    Details
    Publication Date: 2016-06-07
    Description: Monitoring of earth's atmosphere was conducted for several years utilizing the ITOS series of low-altitude, polar-orbiting weather satellites. A space environment monitoring package was included in these satellites to perform measurements of a portion of earth's charged particle environment. The charged particle observations proposed for the low-altitude weather satellite TIROS N, are described which will provide the capability of routine monitoring of the instantaneous total energy deposition into the upper atmosphere by the precipitation of charged particles from higher altitudes. Such observations may be of use in future studies of the relationships between geomagnetic activity and atmospheric weather pattern developments. Estimates are given to assess the potential importance of this type of energy deposition. Discussion and examples are presented illustrating the importance of distinguishing between solar and geomagnetic activity as possible causative sources. Such differentiation is necessary because of the widely different spatial and time scales involved in the atmospheric energy input resulting from these various sources of activity.
    Keywords: GEOPHYSICS
    Type: NASA. Goddard Space Flight Center Possible Relationships between Solar Activity and Meteorol. Phenomena; p 155-159
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  • 7
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    Distribution of energetic positive ion species above a diffuse midnight aurora (1979)
    In:  Other Sources
    Details
    Publication Date: 2019-06-27
    Description: The present paper deals with species-identifying distribution function measurements of auroral primary particles, made during a magnetically quiet presubstorm period above a hydrogen-associated diffuse aurora. Only ions identified as H(+) and He(++) were detected. In the mass spectrum data, the He(++) was not clearly above background. At energies between 2.5 and 12 keV, the He(++)/H(+) intensity ratio had an upper limit of 2 to 4 percent. The same upper limit applies to all other ions, such as He(+) and O(+). Though this would suggest a solar wind source for these ions, an admixture including an appreciable fraction of polar wind protons is not precluded. This situation contrasts sharply with a number of recently reported observations of large intensities of precipitating O(+) ions during magnetic storms, and may be characteristic of undisturbed periods.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 84; Nov. 1
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  • 8
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    Radar observations of a volcanic terrain: Askja Caldera, Iceland (1978)
    In:  CASI
    Details
    Publication Date: 2019-06-27
    Description: Surface roughness spectra of nine radar backscatter units in the Askja caldera region of Iceland were predicted from computer-enhanced like- and cross-polarized radar images. A field survey of the caldera was then undertaken to check the accuracy of the preliminary analysis. There was good agreement between predicted surface roughness of backscatter units and surface roughness observed in the field. In some cases, variations in surface roughness could be correlated with previously mapped geologic units.
    Keywords: GEOPHYSICS
    Type: NASA-CR-157765 , JPL-PUB-78-81
    Format: application/pdf
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  • 9
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    Rocket-borne measurements of the dayside cleft plasma - The Tordo experiments (1977)
    In:  Other Sources
    Details
    Publication Date: 2019-06-27
    Description: Results are presented from low-energy plasma analyzers (12 eV to 12 keV) carried on two rockets launched into the dayside cleft during January 1975. It is concluded that (1) atmospheric interaction becomes important for less than 1-keV electrons at approximately 250 km, (2) characteristics of particles in 'inverted V's' observed in the afternoon cleft are consistent with their interpretation as being due to parallel electric field acceleration from a constant source population, and (3) magnetospheric energetic (greater than 2 keV) electrons intermingle with magnetosheathlike plasma in the cleft.
    Keywords: GEOPHYSICS
    Type: AD-A064473 , AFGL-TR-77-0143 , Journal of Geophysical Research; 82; May 1
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  • 10
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    Auroral vector electric field and particle comparisons. 1: Pre-midnight convection topology (1976)
    In:  CASI
    Details
    Publication Date: 2019-06-27
    Description: Polar 3 was launched in northern Norway on January 27, 1974. Traversing nearly 3 deg latitude, the rocket crossed over a stable IBC II auroral arc in the positive bay region and continued north to a convection boundary which was identified as the Harang discontinuity. Measurement of the complete electric field vector, of energetic electrons and of the auroral N+2 and OI emissions were used to study the convection topology in the pre-magnetic-midnight region. A strong anticorrelation was observed between the electric field and the precipitating energetic electrons. The inverted V nature of the electron precipitations at the convection boundary, compared with the lack of such structure over the arc which was within the positive bay region, leads to the conclusion that auroral arcs are likely to be associated with inverted V type precipitation only at or poleward of convection boundaries and their eddy structures.
    Keywords: GEOPHYSICS
    Type: NASA-TM-X-71130 , X-625-76-108
    Format: application/pdf
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