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The D-CIXS X-ray mapping spectrometer on SMART-1

  • M. Grande*
  • , R. Browning
  • , N. Waltham
  • , D. Parker
  • , S. K. Dunkin
  • , B. Kent
  • , B. Kellett
  • , C. H. Perry
  • , B. Swinyard
  • , A. Perry
  • , J. Feraday
  • , C. Howe
  • , G. McBride
  • , K. Phillips
  • , J. Huovelin
  • , P. Muhli
  • , P. J. Hakala
  • , O. Vilhu
  • , J. Laukkanen
  • , N. Thomas
  • D. Hughes, H. Alleyne, M. Grady, R. Lundin, S. Barabash, D. Baker, P. E. Clark, C. D. Murray, J. Guest, I. Casanova, L. C. D'Uston, S. Maurice, B. Foing, D. J. Heather, V. Fernandes, K. Muinonen, S. S. Russell, A. Christou, C. Owen, P. Charles, H. Koskinen, M. Kato, K. Sipila, S. Nenonen, M. Holmstrom, N. Bhandari, R. Elphic, D. Lawrence
*Šī darba korespondējošais autors
  • Rutherford Appleton Laboratory
  • University College London
  • University of Helsinki
  • University of Turku
  • Max Planck Institute for Solar System Research
  • University of Sheffield
  • The Natural History Museum, London
  • IRF
  • University of Colorado Boulder
  • NASA Goddard Space Flight Center
  • Queen Mary University of London
  • Polytechnic University of Catalonia
  • Institut de Recherche en Astrophysique et Planétologie (IRAP)
  • Observ. Midi-Pyrénées
  • ESA Research Department
  • University of Manchester
  • Armagh Observatory
  • University of Southampton
  • JAXA Institute of Space and Astronautical Science
  • Oxford Instruments Group Plc
  • Physical Research Laboratory India
  • Los Alamos National Laboratory

Zinātniskās darbības rezultāts: Devums žurnālamZinātniskais raksts (žurnālā)koleģiāli recenzēts

70 Atsauces (Scopus)

Kopsavilkums

The D-CIXS Compact X-ray Spectrometer will provide high quality spectroscopic mapping of the Moon, the primary science target of the ESA SMART-1 mission. D-CIXS consists of a high throughput spectrometer, which will perform spatially localised X-ray fluorescence spectroscopy. It will also carry a solar monitor, to provide the direct calibration needed to produce a global map of absolute lunar elemental abundances, the first time this has been done. Thus it will achieve ground breaking science within a resource envelope far smaller than previously thought possible for this type of instrument, by exploiting two new technologies, swept charge devices and micro-structure collimators. The new technology does not require cold running, with its associated overheads to the spacecraft. At the same time it will demonstrate a radically novel approach to building a type of instrument essential for the BepiColombo mission and potential future planetary science targets.

OriģinālvalodaAngļu
Lapas (no-līdz)427-433
Lapu skaits7
ŽurnālsPlanetary and Space Science
Sējums51
Izdevuma numurs6
DOIs
Publikācijas statussPublicēts - maijs 2003
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