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A method is described whereby a conventional non-Doppler radar may be used in the measurement and detection of atmospheric turbulence. The technique involves the measurement of the average echo power and the variance of the fluctuation spectrum in each of two separated pulse volumes, and corresponding measure ments of echo power and variance of the detected signals in a channel representing the predetection sum of the signals from those two volumes. It is shown that the variance of the sum channel is the power-weighted sum of the variances in the independent channels plus a term dependent upon the difference in mean radial velocity of the associated pulse volumes. Accordingly, the difference in mean radial velocity can be measured. When the spacing of the sampled volumes is adjusted to represent distance along an aircraft flight plan, the measurement is a measure of the turbulence to be experienced in traversing the space between those volumes. Specific systems for accomplishing the measure ment are discussed. 相似文献
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G. Kminek J.D. Rummel C.S. Cockell R. Atlas N. Barlow D. Beaty W. Boynton M. Carr S. Clifford C.A. Conley A.F. Davila A. Debus P. Doran M. Hecht J. Heldmann J. Helbert V. Hipkin G. Horneck T.L. Kieft G. Klingelhoefer M. Meyer H. Newsom G.G. Ori J. Parnell D. Prieur F. Raulin D. Schulze-Makuch J.A. Spry P.E. Stabekis E. Stackebrandt J. Vago M. Viso M. Voytek L. Wells F. Westall 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
In this paper we present the findings of a COSPAR Mars Special Regions Colloquium held in Rome in 2007. We review and discuss the definition of Mars Special Regions, the physical parameters used to define Mars Special Regions, and physical features on Mars that can be interpreted as Mars Special Regions. We conclude that any region experiencing temperatures > −25 °C for a few hours a year and a water activity > 0.5 can potentially allow the replication of terrestrial microorganisms. Physical features on Mars that can be interpreted as meeting these conditions constitute a Mars Special Region. Based on current knowledge of the martian environment and the conservative nature of planetary protection, the following features constitute Mars Special regions: Gullies and bright streaks associated with them, pasted-on terrain, deep subsurface, dark streaks only on a case-by-case basis, others to be determined. The parameter definition and the associated list of physical features should be re-evaluated on a regular basis. 相似文献
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