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Anna Milillo Valeria Mangano Alessandro Mura Stefano Orsini Elisabetta De Angelis Andrea M. Di Lellis Stefano Massetti Christina Plainaki Rosanna Rispoli Stefano Selci Nello Vertolli 《Experimental Astronomy》2011,32(1):37-49
Observation of the lunar exosphere is a tool for remote sensing of the surface properties. The sources of this exosphere are related to the interactions of the lunar surface with the solar radiation, with the solar wind or Earth??s magnetospheric plasma, and with the interplanetary dust and meteorites. In fact, the exospheric particles are continuously created and subsequently lost in the interplanetary space, photo-ionized or re-adsorbed by the surface. Eventually, the estimation of the surface composition is not possible without the knowledge of the active release mechanisms. The relative weight of the different release processes of the various atoms, ions and molecules from the surface is still an open debate. Investigation of the Moon??s release processes and interaction with the near-Earth environment is of crucial importance for both determining the relative process release contribution and understanding the surface evolution of other airless bodies, like Mercury and the giant planets?? moons. In this work, an attempt to analyze the processes that take place on the surface of these small airless bodies, as a result of their exposure to the space environment, has been realized by means of the MonteCarlo Environment Simulation Tool (EST), applied to the Moon. The model results show that the different release processes can be identified by analysing the exospheric energy distribution. Finally, the instrument concept of the ??Analizzatore Lunare di ENA?? (ALENA), part of the MAGIA payload and specifically designed for detecting the high-energy particles released from the lunar surface is presented. 相似文献
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Anna Gandin Nello Minzoni Pierre Courjault-Radé 《International Journal of Earth Sciences》1987,76(3):827-836
In southern and central Sardinia two different Cambrian-Lower Ordovician sedimentary belts occur. The former is exposed in southwestern Sardinia (Iglesiente and Sulcis), and is characterized by shallow-marine siliciclastic and carbonate sediments settled on a continental shelf with lowangle morphology. The latter, exposed in the Nappe Zone (central and southeastern Sardinia), consists of a thick monotonous sequence of siliciclastic deposits settled in a deeper-water basin.The comparative analysis of the sequences and their palinspastic reconstruction lead to recognize an inner and outer shelf respectively in Iglesiente and in northern Sulcis, a transition to the basin in eastern and southern Sulcis and a basin in the eastern areas of Sardinia (Nappe Zone).
Zusammenfassung In Süd- und Zentral-Sardinien gibt es zwei unterschiedliche Sedimentgürtel im Kambrium bis Unterordovizium. Der ältere ist in Südwest-Sardinien (Iglesiente und Sulcis) aufgeschlossen. Er ist aus flachmarinen siliziklastischen und karbonatischen Sedimenten eines kontinentalen Schelfes mit flachem Relief aufgebaut. Der zweite Sedimentgürtel, aufgeschlossen in der Decken-Zone (Zentral- und SE-Sardinien) besteht aus einer mächtigen einheitlichen Folge von siliziklastischen Ablagerungen eines tieferen Beckens.Die vergleichende Analyse der Folgen und die palinspastische Rekonstruktion läßt einen inneren und einen äußeren Schelf im Gebiet von Iglesiente und nördlichen Sulcis erkennen, einen Übergang zum Becken im östlichen und südlichen Sulcis sowie ein Becken im östlichen Sardinien (Decken-Zone).
Résumé En Sardaigne méridionale et centrale, on connaît deux ensembles sédimentaires d'âge cambro-ordovicien. Le premier, exposé dans la partie sud-occidentale de l'île (secteurs de l'Iglesiente et du Sulcis), est caractérisé par des sédiments carbonatés et terrigènes déposés sur un shelf continental morphologiquement régulier et à inclinaison faible.Le second, exposé dans la »zone des nappes« (Sardaigne orientale) est composé d'une séquence terrigène monotone déposée dans un bassin plus profond. L'analyse comparée des séquences et les reconstructions palynspastiques conduisent à reconnaître plusieurs domaines paléogéographiques: un shelf interne dans l'Iglesiente, un shelf externe dans le Sulcis septentrional, une transition vers le bassin profond dans le sud et l'est du Sulcis et ce bassin profond dans la Sardaigne orientale (»zones des nappes«).
, . - (Iglesiente Sulcis) , , . , ( - ), , . : Iglesiente, — Sulcis, — Sulcis, — .相似文献
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