John D. de Boer , R. Godard , José J. López-Moreno , Gregorio J. Molina-Cuberos
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引用次数: 0
Abstract
In this work, we investigate the shadowing effect of the boom and the gondola on electrical conductivity measurement in the stratosphere using a Relaxation Probe (RP). By taking the examples of the terrestrial flight for the Huygens experiment and the Huygens mission to Titan, our numerical simulations demonstrate that this effect should be taken into account, particularly for the resistance of the electrode-ionized medium during both the apogee and descent of a balloon. The fact that a signal seems a perfect exponential does not allow one to accept the hypothesis of a measurement at face value, and a correction factor should be applied. Our numerical simulations show that the resistance and the capacitance are almost constant, independent of the potential of the electrode. This makes the correction of the data an easy task. This analysis was carried out using finite element methods to model a complex electrode-boom-gondola geometry. In our model, the potential around the electrode-boom-gondola system is described by a Laplace equation, and this corresponds well to the stratospheric environment. We shall emphasize the crucial importance of estimating the floating potential of the gondola during a flight from the relaxation data of the potential. From our numerical simulations, it appears that the resistance may be too high by a factor 1.72, depending of course on the length of the boom. Also, the measurement of the positive ions by the RP for the Huygens mission around Titan does not seem too reliable. In this case, we found a heavy shadowing effect of the gondola. We hope that this work will aid in the optimal design of future planetary missions, taking into account the length of boom and, given the constraints of a mission, whether the boom should be an insulator, or a conducting body.
期刊介绍:
Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered:
• Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics
• Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system
• Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating
• Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements
• Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation
• Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites
• Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind
• Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations
• Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets
• History of planetary and space research