The pressure and temperature dependent fluorescence line-shift of strontium tetraborate has been measured concurrently with x-ray diffraction from the pressure standards sodium chloride or gold. Temperature was found to have a small effect on the fluorescence line-shift under pressure. We found a maximum pressure uncertainty of ±1.8 GPa at 25 GPa (7.2%) and 857 K when making no temperature correction. The fluorescence line-shifts for ruby, Alexandrite, and samarium-doped yttrium aluminum garnet were also determined, using our strontium tetraborate calibration to determine pressure and a thermocouple to measure temperature. Fluorescence measurements were extended up to 800 K for ruby and Alexandrite. Temperature was found to have a small effect on the fluorescence line-shift of samarium-doped yittrium aluminum garnet. We found a maximum uncertainty of ±2.7 GPa at 25 GPa (11.1%) and 857 K when no temperature correction was applied. We determined equations relating to the fluorescence line position from these data, which include a cross derivative term to account for the combined effect of pressure and temperature. We present a method to independently determine pressure and/or temperature from combined fluorescence line-shift measurements of a pair of optical sensors.

1.
W. L.
Vos
and
J. A.
Schouten
,
J. Appl. Phys.
69
,
6744
(
1991
).
2.
D. D.
Ragan
,
R.
Gustavsen
, and
D.
Schiferl
,
J. Appl. Phys.
72
,
5539
(
1992
).
3.
A.
Lacam
and
C.
Chateau
,
J. Appl. Phys.
66
,
366
(
1989
).
4.
N. J.
Hess
and
D.
Schiferl
,
J. Appl. Phys.
68
,
1953
(
1990
).
5.
A. H.
Jahren
,
M. B.
Kruger
, and
R.
Jeanloz
,
J. Appl. Phys.
71
,
1579
(
1992
).
6.
H. K.
Mao
,
P. M.
Bell
,
J. W.
Shaner
, and
D. J.
Steinberg
,
J. Appl. Phys.
49
,
3276
(
1978
).
7.
J.
Yen
, Ph.D. thesis,
University of California
Los Angeles,
1986
.
8.
F.
Datchi
,
A.
Dewaele
,
P.
Loubeyre
,
R.
Letoullec
,
Y.
Le Godec
, and
B.
Canny
,
High Press. Res.
27
,
447
(
2007
).
9.
A. F.
Goncharov
,
J. M.
Zaug
,
J. C.
Crowhurst
, and
E.
Gregoryanz
,
J. Appl. Phys.
97
,
094917
(
2005
).
10.
F.
Datchi
,
R.
LeToulloc
, and
Loubeyre
,
J. Appl. Phys.
81
,
3333
(
1997
).
11.
E. H.
Abramson
and
J. M.
Brown
,
Geochim. Cosmochim. Acta
68
,
1827
(
2004
).
12.
J. M.
Brown
,
J. Appl. Phys.
86
,
5801
(
1999
).
13.
F.
Birch
,
J. Geophys. Res.
91
4949
(
1986
).
14.
S.-H.
Shim
,
T. S.
Duffy
, and
T.
Kenichi
,
Earth Planet. Sci. Lett.
203
,
729
(
2002
).
15.
M.
Kunz
,
A. A.
MacDowell
,
W. A.
Caldwell
,
D.
Cambie
,
R. S.
Celestre
,
E. E.
Domning
,
R. M.
Duarte
,
A. E.
Gleason
,
J. M.
Glossinger
,
N.
Kelez
,
D. W.
Plate
,
T.
Yu
,
J. M.
Zaug
,
H. A.
Padmore
,
R.
Jeanloz
,
A. P.
Alivisatos
, and
S. M.
Clark
,
J. Synchrotron Radiat.
12
,
650
(
2005
).
16.
N. J.
Hess
and
D.
Schiferl
,
J. Appl. Phys.
71
,
2082
(
1992
).
17.
Y.
Zhao
,
W.
Barvosa-Carter
,
S. D.
Theiss
,
S.
Mitha
, and
M. J.
Aziz
,
J. Appl. Phys.
84
,
4049
(
1998
).
You do not currently have access to this content.