The Dante is an 18 channel x-ray filtered diode array which records the spectrally and temporally resolved radiation flux from various targets (e.g., hohlraums, etc.) at x-ray energies between 50 eV and 10 keV. It is a main diagnostic installed on the OMEGA laser facility at the Laboratory for Laser Energetics, University of Rochester. The absolute flux is determined from the photometric calibration of the x-ray diodes, filters and mirrors, and an unfold algorithm. Understanding the errors on this absolute measurement is critical for understanding hohlraum energetic physics. We present a new method for quantifying the uncertainties on the determined flux using a Monte Carlo parameter variation technique. This technique combines the uncertainties in both the unfold algorithm and the error from the absolute calibration of each channel into a one sigma Gaussian error function. One thousand test voltage sets are created using these error functions and processed by the unfold algorithm to produce individual spectra and fluxes. Statistical methods are applied to the resultant set of fluxes to estimate error bars on the measurements.

1.
H. N.
Komblum
,
R. L.
Kauffman
, and
J. A.
Smith
,
Rev. Sci. Instrum.
57
,
2179
(
1986
).
2.
C.
Sorce
,
J.
Schein
,
F.
Weber
,
K.
Widmann
,
K.
Campbell
,
E.
Dewald
,
R. E.
Turner
,
O. L.
Landen
,
K.
Jacoby
,
P.
Torres
, and
D.
Pellinen
,
Rev. Sci. Instrum.
77
,
10E518
(
2006
).
3.
E. L.
Dewald
,
K. M.
Campbell
,
R. E.
Turner
,
J. P.
Holder
,
O. L.
Landen
,
S. H.
Glenzer
,
R. L.
Kauffman
,
L. J.
Suter
,
M.
Landon
,
M.
Rhodes
, and
D.
Lee
,
Rev. Sci. Instrum.
75
,
3759
(
2004
).
4.
J. P.
Bourgade
,
B.
Villette
,
J. L.
Boucher
,
J. Y.
Boutin
,
S.
Chiche
,
N.
Dague
,
D.
Gontier
,
J. P.
Jadaud
,
B.
Savale
,
R.
Wrobel
, and
R. E.
Turner
,
Rev. Sci. Instrum.
72
,
1173
(
2001
).
5.
A.
Seifter
and
G. A.
Kyrala
,
Rev. Sci. Instrum.
79
,
10F323
(
2008
).
6.
K. M.
Campbell
,
F. A.
Weber
,
E. L.
Dewald
,
S. H.
Glenzer
,
O. L.
Landen
,
R. E.
Turner
, and
P. A.
Waide
,
Rev. Sci. Instrum.
75
,
3768
(
2004
).
You do not currently have access to this content.