منابع مشابه
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In anticipation of new observational results for Jupiter’s axial moment of inertia and gravitational zonal harmonic coefficients from the forthcoming Juno orbiter, we present a number of preliminary Jupiter interior models. We combine results from ab initio computer simulations of hydrogen-helium mixtures, including immiscibility calculations, with a new nonperturbative calculation of Jupiter’s...
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Three reviews of radio emission from Jupiter have appeared recently (1, 2, 3) and at least one more is currently in press. The present review primarily covers work since 1961. It would be not too strong to suggest that explanations of Jupiter's emission now are in the second generation, with most observational phenomena fairly well established. The salient observed features are not widely known...
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Attaining in situ data from planets in our solar system is an extremely difficult undertaking. Decades of planning go into designing missions, and careful consideration is made for what measurements should be made to yield the greatest scientific gain, and to make the cost and risks worthwhile. NASA’s Galileo mission, whose detailed planning began in 1970s, studied the Jovian system from 1995 t...
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Decadal-long radial velocity surveys have recently started to discover analogs to the most influential planet of our solar system, Jupiter. Detecting and characterizing these worlds is expected to shape our understanding of our uniqueness in the cosmos. Despite the great successes of recent transit surveys, Jupiter analogs represent a terra incognita, owing to the strong intrinsic bias of this ...
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ژورنال
عنوان ژورنال: ACM SIGCOMM Computer Communication Review
سال: 2015
ISSN: 0146-4833
DOI: 10.1145/2829988.2787508