Raman & Laser-induced Breakdown Spectroscopy (libs) Remote Geochemical Analysis under Venus Atmospheric Pressure
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چکیده
ANALYSIS UNDER VENUS ATMOSPHERIC PRESSURE. S.M. Clegg 1 , S.K. Sharma 2 , A.K. Misra 2 , M.D. Dyar 3 , N. Dallmann 1 , R.C. Wiens 1 , D.T. Vaniman 1 , E. A. Speicher 3 , S.E. Smrekar 4 , A. Wang 5 , S. Maurice 6 , and L. Esposito 7 . 1 Los Alamos National Laboratory, P.O. Box 1663 MS J565, Los Alamos, NM 87545, [email protected], 2 Hawaii Institute of Geophysics and Planetology, University of Hawaii, 2525 Correa Rd., Honolulu, HI, 96822, 3 Dept. of Astronomy, Mt. Holyoke College, South Hadley, MA 01075, 4 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena CA, 91109, Earth & Planetary Sciences, Washington University, 1 Brookings Dr, Saint Louis MO 63130, Centre d’Etude Spatiale des Rayonnements (CESR), Toulouse, France, LASP University of Colorado, 1234 Innovation Drive Boulder, Colorado 80303.
منابع مشابه
Raman and Laser-induced Breakdown Spectroscopy (libs) Geochemical Analysis under Venus Atmospheric
ANALYSIS UNDER VENUS ATMOSPHERIC PRESSURE. S.M. Clegg, M.D. Dyar, S.K. Sharma, A.K. Misra, R.C. Wiens, S.E. Smrekar, S. Maurice and L. Esposito, Los Alamos National Laboratory, P.O. Box 1663 MS J565, Los Alamos, NM 87545, [email protected], Dept. of Astronomy, Mt. Holyoke College, South Hadley, MA 01075, Hawaii Institute of Geophysics and Planetology, University of Hawaii, 2525 Correa Rd., Honolu...
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[1]) with terrestrial standard samples used in this study (red). JA-1 is the most K-rich.. VENUS GEOCHEMICAL ANALYSIS BY REMOTE LASER-INDUCED BREAKDOWN SPECTROSCOPY (LIBS). S. M. Clegg, J. E. Barefield, R. C. Wiens, S. K. Sharma, A. K. Misra, J. Tucker, M. D. Dyar, J. Lambert, S. Smrekar, A. Treiman. Los Alamos National Laboratory, P.O. Box 1663 MS J565, Los Alamos, NM 87545, [email protected], j...
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