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The top documents tagged [high resolution spectra]
Problems The ratios e/m of 4 He + and D 2 + ions are very close: m D 2 = 4.0282 amu m He = 4.0026 amu m = 0.0256 amu A high resolution mass spectrometer
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High Mountain Water Cerenkov Array in Mexico to detect Extensive Air Showers (HAWC) Humberto Salazar I BUAP, Puebla & INAOE VII SILAFAE Bariloche, January
233 views
64th OSU International Symposium on Molecular Spectroscopy June 22-26, 2009 José Luis Doménech Instituto de Estructura de la Materia 1 MEASUREMENT OF ROTATIONAL
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EUV-initiated surface changes in polymers A. Bartnik, H. Fiedorowicz, R. Jarocki, J. Kostecki, M. Szczurek Institute of Optoelectronics, Military University
219 views
Star Clusters in the Galactic Center Sgr A* at 30 Workshop Green Bank W.Va March 25, 26, 2004 Donald F. Figer STScI
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THE CHEMICAL ENRICHMENT OF CENTAURI JOHN E. NORRIS RESEARCH SCHOOOL OF ASTRONOMY & ASTROPHYSICS MOUNT STROMLO & SIDING SPRING OBSERVATORIES AUSTRALIAN
218 views
The Seismic Plus Portal E. Michel, C. Renié, K. Belkacem,M. Abed/ SPACEINN-WP3-meeting-1 21-22/10/2013 Observatoire de Paris
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SPECTRAL LINE PARAMETERS FOR THE 9 BAND OF ETHANE Malathy Devi & Chris Benner, W&M Rinsland & Smith, NASA Langley Bob Sams & Tom Blake, PNNL Jean-Marie
216 views
Structure and Evolution of the Milky Way Ken Freeman Research School of Astronomy & Astrophysics RED GIANTS AS PROBES OF THE STRUCTURE AND EVOLUTION OF
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Nathan R. Pillsbury, Timothy S. Zwier, Department of Chemistry, Purdue University, West Lafayette, IN 47907; David F. Plusquellic, NIST, Gaithersburg,
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Requirements on array detectors from the OWL Instrument Concept Studies Sandro D’Odorico European Southern Observatory SDW 2005 TAORMINA
217 views
HESSI Science Objective Impulsive Energy Release in the Corona Acceleration of Electrons, Protons, and Ions Plasma Heating to Tens of Millions of
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