21.04.2014 Views

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 ...

SHOW MORE
SHOW LESS

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.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!