The Signature of Amphibole in Mafic Alkaline Lavas, a Study in the ...
The Signature of Amphibole in Mafic Alkaline Lavas, a Study in the ...
The Signature of Amphibole in Mafic Alkaline Lavas, a Study in the ...
You also want an ePaper? Increase the reach of your titles
YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.
Nb<br />
88-<br />
94-<br />
88<br />
82-<br />
85-<br />
52-<br />
42-<br />
41-<br />
34-<br />
33-<br />
31-<br />
29-<br />
30-<br />
28-<br />
26-<br />
Ta<br />
4-4<br />
Cr<br />
350-<br />
Co<br />
57-<br />
Ni<br />
229-<br />
Th<br />
7-7<br />
U<br />
2-1<br />
Rare earth elements (p.p.m.)<br />
La<br />
80-5<br />
Ce<br />
1400<br />
Nd<br />
620<br />
Sm<br />
14-23<br />
Eu<br />
409<br />
Tb<br />
1-40<br />
Ho<br />
—<br />
4-6<br />
331-<br />
53-<br />
240-<br />
83<br />
2-2<br />
76-1<br />
139 0<br />
640<br />
1400<br />
3-91<br />
1-30<br />
1-30<br />
4 1<br />
341-<br />
56-<br />
243-<br />
7 1<br />
1-8<br />
73-5<br />
1320<br />
580<br />
11-93<br />
3-70<br />
1-20<br />
—<br />
40<br />
364-<br />
56-<br />
281-<br />
70<br />
1-9<br />
70-3<br />
1250<br />
540<br />
12-31<br />
3-56<br />
1-11<br />
—<br />
4-2<br />
363-<br />
59-<br />
284-<br />
70<br />
20<br />
68-9<br />
1210<br />
540<br />
12-23<br />
3-63<br />
1-20<br />
—<br />
25<br />
382-<br />
60-<br />
297-<br />
4-2<br />
10<br />
38-2<br />
740<br />
360<br />
7-79<br />
2-45<br />
0-85<br />
—<br />
2-2<br />
313-<br />
58-<br />
238-<br />
32<br />
10<br />
30-1<br />
56-7<br />
280<br />
6-99<br />
205<br />
0-78<br />
0-70<br />
1-8<br />
287<br />
54-<br />
196-<br />
30<br />
0-9<br />
25-8<br />
540<br />
270<br />
6-26<br />
200<br />
0-80<br />
0-80<br />
1-7<br />
349-<br />
60-<br />
238-<br />
2-6<br />
0-8<br />
21-9<br />
44-6<br />
21 0<br />
5-39<br />
1-83<br />
063<br />
0 70<br />
1-6<br />
331<br />
56-<br />
222-<br />
2-3<br />
0-8<br />
21-1<br />
42-4<br />
220<br />
5-64<br />
1-71<br />
—<br />
0-90<br />
1-6<br />
317-<br />
55-<br />
215<br />
21<br />
0-8<br />
19-4<br />
39-9<br />
190<br />
5-43<br />
1-64<br />
0-65<br />
0-70<br />
Downloaded from petrology.oxfordjournals.org at McGill University Libraries on September 29, 2011<br />
317<br />
1-4<br />
58-<br />
221-<br />
2-2<br />
0-7<br />
20-2<br />
39-3<br />
200<br />
4-93<br />
1-68<br />
0-56<br />
0-60<br />
1-5<br />
308-<br />
56-<br />
217<br />
2-1<br />
0-6<br />
200<br />
370<br />
190<br />
5-16<br />
1-63<br />
0-64<br />
0 70<br />
1-4<br />
3000<br />
55-<br />
217-<br />
20<br />
0-6<br />
18-8<br />
37-1<br />
190<br />
506<br />
1-59<br />
0-63<br />
—<br />
1-7<br />
277-<br />
54-<br />
235-<br />
2-4<br />
0-8<br />
20-3<br />
380<br />
200<br />
4-99<br />
1-56<br />
0-68<br />
0-70<br />
Yb<br />
1-40<br />
1-50<br />
1-40<br />
1 -40<br />
1-30<br />
1-30<br />
1-20<br />
1-50<br />
1-20<br />
1-30<br />
1-30<br />
1-30<br />
1-30<br />
1-30<br />
1-40<br />
Lu<br />
0-15<br />
0-18<br />
0-17<br />
0-17<br />
0-16<br />
0-14<br />
0 18<br />
0-16<br />
0-16<br />
0-15<br />
0-20<br />
0-20<br />
0-21<br />
0-19<br />
020<br />
Foid<br />
34-78<br />
34-40<br />
33-16<br />
32-36<br />
32-43<br />
15-54<br />
10-67<br />
808<br />
6-11<br />
523<br />
507<br />
4-44<br />
4-29<br />
2-68<br />
—<br />
Opx<br />
—<br />
—<br />
—<br />
—<br />
—<br />
—<br />
—<br />
—<br />
—<br />
—<br />
—<br />
—<br />
-<br />
—<br />
2-72<br />
LOI, loss on ignition.<br />
<strong>The</strong> major elements and <strong>the</strong> trace elements Ba, Rb, Sr, Nb, Zr, Y, V, Cr and Ni were analysed by X-ray fluorescence (XFR) spectrometry at McGill University with a Philips PW 1400<br />
spectrometer. <strong>The</strong> major elements and Ba, V, Co, Cr and Ni were analysed on fused discs us<strong>in</strong>g an a-coefficient technique. Where given, Fe 3+ was calculated as Fe tot - Fe 2 *, where Fe 2 +<br />
was determ<strong>in</strong>ed by titration, o<strong>the</strong>rwise total Fe is given as FeO. <strong>The</strong> analytical precision (1 SD <strong>in</strong> wt %) calculated from 20 replicate analyses on one disc is: Si 005, Al 003, Cr 0001, Mg<br />
0058, Fe 001, Mn 0001, Ni 0004, Ca 001, Na 006, K 0001 and P 0004. <strong>The</strong> o<strong>the</strong>r XRF trace elements were analysed on pressed powder pellets us<strong>in</strong>g a Rh Kb Compton scatter<br />
matrix correction. <strong>The</strong> relative analytical precision <strong>of</strong> <strong>the</strong>se elements is estimated to be 5%. <strong>The</strong> REE, Sc, Hf, Ta, U and Th were analysed by <strong>in</strong>strumental neutron activation at <strong>the</strong> University<br />
de Montreal. <strong>The</strong> samples were irradiated <strong>in</strong> a flux <strong>of</strong> 10 neutrons/cm/s for 4 h <strong>in</strong> a SLOWPOKE II reactor and counted over a period <strong>of</strong> 6 weeks on two Ge detectors with resolutions<br />
<strong>of</strong> 0-6 and 1 -2 keV. <strong>The</strong> relative analytical precisions for La, Sm, Eu, Yb and Sc are estimated to be 5%, and those for Ce, Nd, Ho, Tb, Lu and Ta are ~10%. <strong>The</strong> normative<br />
amounts <strong>of</strong> feldspathoid or orthopyroxene are calculated <strong>in</strong> oxygen units assum<strong>in</strong>g Fe 3+ /Fe to ' = 0-10. See Francis & Ludden (1990) for Fort Selkirk analyses.