 F, Na, Mg, Al, Si, P, S, Cl, K, Ca, Ti, V, Cr, Mn, Fe, Co, Ni, Cu, Zn, Ga, Sr, Zr, Mo, Ag, Cd, Sn, Sb, Ba, Ce, Nd, Gd, Hf, Tl, Pb, and U.  NBS Technical Note - Page 1521980Full view - About this book
 | Augustus George Vernon-Harcourt - 1880 - 508 pages
...arrived at in the manner indicated. TABLE OF ATOMIC WEIGHTS. H represent Li „ B „ C „ N „ 0 „ F „ Na „ Mg „ Al „ Si „ P „ S „ Cl „ K „ Ca „ Ti „ V „ Cr „ Mn „ Fe „ Co „ Ni „ Cu „ Zn „ As „. Se „ Br „ Sr „ Mo „. Pd „ Ag „ Cd „ Sn „ U... | |
 | 1977 - 388 pages
...030 030 030 CO NI cu ZN GA Ge Y ZR N8 M3 PO AG CO SN SB cs BA LA CE HF TA W RE PT AU PB TH U 8 c N 0 F NA MG AL SI P s CL K CA TI V CR 27 28 29 30 31 32 39 40 41 42 46 47 48 50 51 55 56 57 58 72 73 74 75 78 79 82 90 92 5 6 7 8 9 11 12... | |
 | 1980 - 336 pages
...in collaboration with NBS. The apparatus and methods have reached the stage at which concentrations of many elements (from the set: H, B, C, N, F, Na,...upper beam tube and with the operation of a large, split-annul us Nal crystal surrounding a Ge(LI) detector for Comptonsuppresslon and pair spectrometry.... | |
 | Niren Laxmichand Nagda, Jerome P. Harper - 1989 - 310 pages
...Zn As Se Br Rb Sr Hg Pb Fine Sampling Coarse Interval: 4/7 - 4/14/86 Fine0 Coarse Particles (mass) Na Mg Al Si P S Cl K Ca Ti V Cr Mn Fe Ni Cu Zn As Se Br Rb Sr Hg Pb 850 .., 4.80 0.96 145 12.0 2.70 0.04 2.00 10.0 1.30 12.0 .., 1.20 ..,... | |
 | Jozef M. Pacyna, Brynjulf Ottar - 1989 - 414 pages
...Mo secondary target for elements Ti - Sr, Hg and Pb; Sm secondary target for elements Zr - Ba. 272 Na Mg Al Si P S Cl K Ca Ti V Cr Mn Fe Co Ni Cu Zn Ga 310 60 6.7 16 8.2 8.2 5.6 2.2 3.1 1.2 4.3 1.6 1.2 2.6 2.2 6.0 6.0 4.8 130 45 15 13 6... | |
 | Chintamani Nagesa Ramachandra Rao - 2000 - 322 pages
...8 9 10 11 12 13 14 Cl K Ca Cr Ti Mn Fe 15 16 17 18 19 20 21 I II III IV V VI VII VIII Li Be B C N O F Na Mg Al Si P S Cl K Ca • Ti V Cr Mn Fe Co Ni Cu Zn • XAs Se Br Rb Sr Y Zr Nb Mo How was Mendeleyev's classification of elements an improvement... | |
 | Marsha Creatchman - 1999 - 338 pages
...information on all commonly occurring elements in atmospheric particulate matter including: H, C, N, O, F, Na, Mg, Al, Si, P, S, Cl, K, Ca, Ti, V, Cr, Mn, Fe, Cu, Ni, Zn, As, Sr, Y, Zr, Br, and Pb. The precision and accuracy of these IBA methods are now well... | |
 | Kvetoslav R. Spurny - 2000 - 642 pages
...were typically accumulated for a preset charge of 60 (iC. The spectra were fitted for 29 elements (ie, Na, Mg, Al, Si, P, S, Cl, K, Ca, Ti, V, Cr, Mn, Fe, Ni, Cu, Zn, Ga, Ge, As, Se (in the fine fraction only), Br, Rb, Sr, Y (in the fine fraction only),... | |
 | Michael Clugston, Rosalind Flemming - 2000 - 756 pages
...Mendeleyev also had the foresight to realize that some elements had yet to be discovered. Li Be H B C N O Na Mg Al Si P S Cl K Ca Ti V Cr Mn Fe Co Ni Cu Zn As Se Br Rb Sr Y Zr Nb Mo Ru Rh Pd Ag Cd In Sn Sb Te 1 Cs Ba La Ta W Os Ir Pt Au Hg TI... | |
 | D Williams, R Shimizu - 2000 - 546 pages
...individual particle analysis method. From their spectra, the characteristic X-ray peaks of 20 elements - Na, Mg, Al, Si, P, S, Cl, K, Ca, Ti, V, Cr, Mn, Fe, Ni, Cu, Zn, Br, Ba and Pb - were observed. The particles were classified into 14 emission sources.... | |
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