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61.
This article examines the current effort to establish a ‘European space policy’. The authors place this effort in the context of the experience of the 2003 Green and White Papers, the subsequent stalling of the Constitutional Treaty for the EU, and reductions in the EU's financial perspectives. They argue that, despite post-referenda malaise and systemic inertia on the part of several member states, adoption of a space policy is long overdue and should not merely seek to rearrange what is already there or expose yet again what is being done. A full-blooded policy setting in train fundamental change is needed, justifying a political decision at the level of the European Council. The article then offers criteria such a policy should fulfil as well as items the authors view as essential content. They briefly explore issues which could become stumbling blocks but which can be accommodated within the kind of policy this article advocates. 相似文献
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Charles E. Schlemm II Richard D. Starr George C. Ho Kathryn E. Bechtold Sarah A. Hamilton John D. Boldt William V. Boynton Walter Bradley Martin E. Fraeman Robert E. Gold John O. Goldsten John R. Hayes Stephen E. Jaskulek Egidio Rossano Robert A. Rumpf Edward D. Schaefer Kim Strohbehn Richard G. Shelton Raymond E. Thompson Jacob I. Trombka Bruce D. Williams 《Space Science Reviews》2007,131(1-4):393-415
NASA’s MESSENGER (MErcury Surface, Space ENvironment, GEochemistry, and Ranging) mission will further the understanding of
the formation of the planets by examining the least studied of the terrestrial planets, Mercury. During the one-year orbital
phase (beginning in 2011) and three earlier flybys (2008 and 2009), the X-Ray Spectrometer (XRS) onboard the MESSENGER spacecraft
will measure the surface elemental composition. XRS will measure the characteristic X-ray emissions induced on the surface
of Mercury by the incident solar flux. The Kα lines for the elements Mg, Al, Si, S, Ca, Ti, and Fe will be detected. The 12°
field-of-view of the instrument will allow a spatial resolution that ranges from 42 km at periapsis to 3200 km at apoapsis
due to the spacecraft’s highly elliptical orbit. XRS will provide elemental composition measurements covering the majority
of Mercury’s surface, as well as potential high-spatial-resolution measurements of features of interest. This paper summarizes
XRS’s science objectives, technical design, calibration, and mission observation strategy. 相似文献
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Space Science Reviews - 相似文献