The XMaS bending magnet beamline at the ESRF has been in regular user operation since the autumn of 1998 and has employed a very simple optical system consisting of a Si <111> monochromator and a toroidal mirror. The ESRF extremely brilliant source (EBS) upgrade program presents the bending magnet beamlines with a series of challenges and exciting new opportunities to extend the range of science performed, with emphasis on in-operando and in-situ studies. Geometrically, the new EBS lattice will move the source for bending magnet beamlines some 3 meters upstream and XMaS will use a newly designed 0.86 Tesla short bend, instead of the present 0.4 Tesla bending magnet. The higher field of the new source increases the available flux at high energies (>25 keV) by an order of magnitude and will result in a smaller brighter beam. To exploit the extended energy range, a dual toroidal mirror system, coated with chromium and platinum, will provide the focusing optics and enable continuous operations from 2.035 keV to 33 keV which will be coupled to a fast scanning LN2 cooled, constant offset monochromator. We report here on the opportunities presented by the new machine lattice and the solutions chosen to deliver a state of the art beamline that utilizes a very wide range of x-ray techniques including scattering and spectroscopy from a broad spectrum of materials characterization.
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15 January 2019
PROCEEDINGS OF THE 13TH INTERNATIONAL CONFERENCE ON SYNCHROTRON RADIATION INSTRUMENTATION – SRI2018
11–15 June 2018
Taipei, Taiwan
Research Article|
January 15 2019
New opportunities for the XMaS beamline arising from the ESRF upgrade program
Paul Thompson;
Paul Thompson
a)
1
XMaS CRG, ESRF
, 71 avenue des Martyrs, 38000 Grenoble, France
3
Dept of Physics, University of Liverpool
, Liverpool, L69 3BX, U.K
a)Corresponding author: pthompso@esrf.fr
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Oier Bikondoa;
Oier Bikondoa
1
XMaS CRG, ESRF
, 71 avenue des Martyrs, 38000 Grenoble, France
2
Dept of Physics, University of Warwick
, Gibbet Hill Road, Coventry, CV4 7AL, U.K
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Laurence Bouchenoire;
Laurence Bouchenoire
1
XMaS CRG, ESRF
, 71 avenue des Martyrs, 38000 Grenoble, France
3
Dept of Physics, University of Liverpool
, Liverpool, L69 3BX, U.K
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Simon Brown;
Simon Brown
1
XMaS CRG, ESRF
, 71 avenue des Martyrs, 38000 Grenoble, France
3
Dept of Physics, University of Liverpool
, Liverpool, L69 3BX, U.K
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Malcolm Cooper;
Malcolm Cooper
2
Dept of Physics, University of Warwick
, Gibbet Hill Road, Coventry, CV4 7AL, U.K
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Tom Hase;
Tom Hase
2
Dept of Physics, University of Warwick
, Gibbet Hill Road, Coventry, CV4 7AL, U.K
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Chris Lucas;
Chris Lucas
3
Dept of Physics, University of Liverpool
, Liverpool, L69 3BX, U.K
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Didier Wermeille
Didier Wermeille
1
XMaS CRG, ESRF
, 71 avenue des Martyrs, 38000 Grenoble, France
3
Dept of Physics, University of Liverpool
, Liverpool, L69 3BX, U.K
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a)Corresponding author: pthompso@esrf.fr
AIP Conf. Proc. 2054, 060030 (2019)
Citation
Paul Thompson, Oier Bikondoa, Laurence Bouchenoire, Simon Brown, Malcolm Cooper, Tom Hase, Chris Lucas, Didier Wermeille; New opportunities for the XMaS beamline arising from the ESRF upgrade program. AIP Conf. Proc. 15 January 2019; 2054 (1): 060030. https://doi.org/10.1063/1.5084661
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