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  • 1
    Publication Date: 2011-08-16
    Description: Stellar wind flow models associating energy transport with propagation and dissipation of hydrodynamic waves and heat conduction
    Keywords: SPACE RADIATION
    Type: ; ECTRON (
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  • 2
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    Publication Date: 2011-08-16
    Description: Simple two fluid solar wind speed and proton temperature model, discussing nonthermal energy dissipation
    Keywords: SPACE RADIATION
    Type: ; ADEMIE DES SCIENCES
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  • 3
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    Publication Date: 2011-08-16
    Description: The difference in objectives, physical assumptions, and results among the most recent detailed models aimed at understanding energy transport in the solar wind are analyzed. Models have been judged primarily by comparing their predictions against spacecraft observations near 1 AU. However, the observed values of flow speed, density, and temperature fluctuate over a wide range so that the criteria for agreement between theory and observation are necessarily somewhat subjective.
    Keywords: SPACE RADIATION
    Type: Cosmic Electrodynamics; 3; July 197
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  • 4
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    Publication Date: 2011-08-11
    Description: Two-fluid model of solar wind, assuming spherical symmetric flow without rotation, magnetic fields or viscous stress
    Keywords: SPACE RADIATION
    Type: PHYSICAL REVIEW LETTERS
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  • 5
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    Publication Date: 2011-08-12
    Description: Solar wind studied with two fluid model, using proton and electron fluid type heat equations, equation of motion and continuity equation
    Keywords: SPACE RADIATION
    Type: ; ACE(
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  • 6
    Publication Date: 2011-08-19
    Description: During January-August 1978, the global atmospheric angular momentum (M) exhibits distinct patterns of short term momentum interchange across latitudes. In the Northern Hemisphere winter-spring season, 30-50 day modulations of M are present in which momentum enhancements at mid-latitudes (20-30 deg) are closely matched by momentum depressions at high latitudes (50-60 deg). During the same interval there are no corresponding variations in M evident in the Southern Hemisphere. Conversely, during Southern Hemisphere fall-winter, similar anti-correlations in monthly scale momentum excursions are evident between mid and high latitudes. In the Northern Hemisphere, the winter-spring momentum signatures are detected throughout the atmosphere, from the lower troposphere to the stratosphere. During the Southern Hemisphere fall-winter, the modulation patterns are not evident at the higher altitudes. Structural details of the momentum signatures indicate that the coupling is sometimes effective on very short time scales, e.g., 1-2 days, or less. The evidence of distinct anti-correlation between large regions has interesting implications for studies of global atmospheric circulation, and also for studies of the excitation of variations in earth rotation in response to short term modulations of M.
    Keywords: METEOROLOGY AND CLIMATOLOGY
    Type: Advances in Space Research (ISSN 0273-1177); 4; 4, 19
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  • 7
    Publication Date: 2016-06-07
    Description: The two-fluid solar-wind model is extended by including the collisionless dissipation of hydromagnetic waves originating at the sun. A series of solar wind models is generated, parameterized by the total energy flux of hydromagnetic waves at the base of the model. The resulting properties of propagation and dissipating of hydromagnetic waves on this model are presented.
    Keywords: SPACE RADIATION
    Type: Solar Wind; p 248-251
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  • 8
    Publication Date: 2016-06-07
    Description: A description is given of the results of solar wind flow in which the heating is due to (1) propagation and dissipation of hydromagnetic waves generated near the base of the wind, and (2) thermal conduction. A series of models is generated for fixed values of density, electron and proton temperature, and magnetic field at the base by varying the wave intensity at the base of the model. This series of models predicts the observed correlation between flow speed and proton temperature for a large range of velocities. The wave heating takes place in a shell about the sun greater than or approximately equal to 10 R thick. We conclude that large-scale variations observed in the solar wind are probably due mainly to variation in the hydromagnetic wave flux near the sun.
    Keywords: SPACE RADIATION
    Type: Solar Wind; p 219-226
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  • 9
    Publication Date: 2016-06-07
    Description: An attempt is made to establish an ionization source capable of maintaining the nighttime Venus ionosphere. The corpuscular ionization and heating caused by the penetration of solar wind plasma into the nightside ionosphere was suggested as a possible source. Theoretical tests, using an interacting solar wind model, were made of the electron density and the results compared with observed electron density profiles. Results indicate the solar wind could maintain the nighttime ionosphere of Venus.
    Keywords: SPACE RADIATION
    Type: Significant Accomplishments in Sci., 1971; p 79-82
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  • 10
    Publication Date: 2019-06-27
    Description: It is shown that newly born ions in the solar wind result in unstable electrostatic waves propagating parallel and perpendicular to the interplanetary magnetic field. A description of the longitudinal instability is followed by a discussion of its implications for assimilating newly born ions of interstellar and planetary origin into comotion with the solar wind bulk velocity. The transverse electrostatic instability is then considered and it is shown that its growth rate is of the same order as that for transverse electromagnetic instabilities found by Wu and Davidson (1972).
    Keywords: SPACE RADIATION
    Type: Journal of Geophysical Research; 78; Sept. 1
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