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Volumn 300, Issue 5625, 2003, Pages 1558-1559

Laboratory simulation of charge exchange - Produced x-ray emission from comets

Author keywords

[No Author keywords available]

Indexed keywords

CALORIMETERS; HEAVY IONS; X RAYS;

EID: 0037567273     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1084373     Document Type: Article
Times cited : (163)

References (24)
  • 1
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    • (1996) Science , vol.274 , pp. 205
    • Lisse, C.M.1
  • 4
    • 0035907046 scopus 로고    scopus 로고
    • C. M. Lisse et al., Science 292, 1343 (2001).
    • (2001) Science , vol.292 , pp. 1343
    • Lisse, C.M.1
  • 13
    • 0037858262 scopus 로고    scopus 로고
    • note
    • The XRS is a precursor of a detector that will fly on the ASTRO-E2 mission, scheduled for launch in February 2005. The wealth of detailed structure in the x-ray line emission seen with the spare XRS detector from the ASTRO-E mission in the laboratory bodes well for cometary observations when ASTRO-E2 launches in 2005. The resolving power of the planned instrumentation may even double from that in the present measurements, and yet more spectral detail may be revealed.
  • 24
    • 0038196051 scopus 로고    scopus 로고
    • note
    • This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under contract W-7405-ENG-48. The research was supported by NASA's Planetary Atmospheres Program under work order W-19,938.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.