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dc.creatorHaranas, I.en
dc.creatorGkigkitzis, I.en
dc.creatorKotsireas, I.en
dc.creatorHaranas, M. K.en
dc.creatorRekkas, I.en
dc.date.accessioned2015-11-23T10:29:54Z
dc.date.available2015-11-23T10:29:54Z
dc.date.issued2015
dc.identifier10.1016/j.asr.2015.07.002
dc.identifier.issn2731177
dc.identifier.urihttp://hdl.handle.net/11615/28430
dc.description.abstractA corrected gravitational acceleration has been used for the study of the electric streaming potential. The acceleration has been corrected for the oblateness of a spherical body, as well as the rotational velocity of the spherical body. For higher viscosity values we find that on the surface of a spherical body the electric streaming field is slightly higher at the poles when compared to that of the equator. Aboard an orbiting spacecraft, we find that equatorial circular orbits that they carry experiments which use high viscosity fluids result to a higher streaming field values when compared to circular polar orbits. In a similar way, we find that the electric streaming field as well as the electrophoretic velocity of the particle in the fluid considered increases significantly in elliptical orbits as the orbital eccentricity increases, being higher in equatorial orbits and smaller in polar orbits. © 2015 COSPAR. Published by Elsevier Ltd. All rights reserved.en
dc.source.urihttp://www.scopus.com/inward/record.url?eid=2-s2.0-84942134064&partnerID=40&md5=81c4552095b6675f83d0fdf25a5cb863
dc.subjectElectrophoretic velocityen
dc.subjectGravitational potentialen
dc.subjectSpherical harmonicsen
dc.subjectStreaming potentialen
dc.subjectGravitationen
dc.subjectSpheresen
dc.subjectViscosityen
dc.subjectGravitational accelerationsen
dc.subjectHigh viscosity fluidsen
dc.subjectOrbital eccentricityen
dc.subjectRotational velocityen
dc.subjectOrbitsen
dc.titleThe effect of gravitational acceleration in the streaming potential on the surface of a planetary body and in orbit around iten
dc.typejournalArticleen


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