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Investigation of high-pressure planetary ices by cryo-recovery. I. An apparatus for X-ray powder diffraction from 40 to 315 K, allowing ‘cold loading’ of samples

A low-temperature stage for X-ray powder diffraction in Bragg–Brentano reflection geometry is described. The temperature range covered is 40–315 K, with a temperature stability at the sample within ±0.1 K of the set point. The stage operates by means of a Gifford–McMahon (GM) closed-cycle He refrige...

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Autores principales: Wood, Ian G., Fortes, A. Dominic, Dobson, David P., Wang, Weiwei, Pajdzik, Lucjan, Cosier, John
Formato: Online Artículo Texto
Lenguaje:English
Publicado: International Union of Crystallography 2018
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5988005/
https://www.ncbi.nlm.nih.gov/pubmed/29896057
http://dx.doi.org/10.1107/S1600576718003965
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author Wood, Ian G.
Fortes, A. Dominic
Dobson, David P.
Wang, Weiwei
Pajdzik, Lucjan
Cosier, John
author_facet Wood, Ian G.
Fortes, A. Dominic
Dobson, David P.
Wang, Weiwei
Pajdzik, Lucjan
Cosier, John
author_sort Wood, Ian G.
collection PubMed
description A low-temperature stage for X-ray powder diffraction in Bragg–Brentano reflection geometry is described. The temperature range covered is 40–315 K, with a temperature stability at the sample within ±0.1 K of the set point. The stage operates by means of a Gifford–McMahon (GM) closed-cycle He refrigerator; it requires no refrigerants and so can run for an extended period (in practice at least 5 d) without intervention by the user. The sample is cooled both by thermal conduction through the metal sample holder and by the presence of He exchange gas, at ambient pressure, within the sample chamber; the consumption of He gas is extremely low, being only 0.1 l min(−1) during normal operation. A unique feature of this cold stage is that samples may be introduced into (and removed from) the stage at any temperature in the range 80–300 K, and thus materials which are not stable at room temperature, such as high-pressure phases that are recoverable to ambient pressure after quenching to liquid nitro­gen temperatures, can be readily examined. A further advantage of this arrangement is that, by enabling the use of pre-cooled samples, it greatly reduces the turnaround time when making measurements on a series of specimens at low temperature.
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spelling pubmed-59880052018-06-12 Investigation of high-pressure planetary ices by cryo-recovery. I. An apparatus for X-ray powder diffraction from 40 to 315 K, allowing ‘cold loading’ of samples Wood, Ian G. Fortes, A. Dominic Dobson, David P. Wang, Weiwei Pajdzik, Lucjan Cosier, John J Appl Crystallogr Research Papers A low-temperature stage for X-ray powder diffraction in Bragg–Brentano reflection geometry is described. The temperature range covered is 40–315 K, with a temperature stability at the sample within ±0.1 K of the set point. The stage operates by means of a Gifford–McMahon (GM) closed-cycle He refrigerator; it requires no refrigerants and so can run for an extended period (in practice at least 5 d) without intervention by the user. The sample is cooled both by thermal conduction through the metal sample holder and by the presence of He exchange gas, at ambient pressure, within the sample chamber; the consumption of He gas is extremely low, being only 0.1 l min(−1) during normal operation. A unique feature of this cold stage is that samples may be introduced into (and removed from) the stage at any temperature in the range 80–300 K, and thus materials which are not stable at room temperature, such as high-pressure phases that are recoverable to ambient pressure after quenching to liquid nitro­gen temperatures, can be readily examined. A further advantage of this arrangement is that, by enabling the use of pre-cooled samples, it greatly reduces the turnaround time when making measurements on a series of specimens at low temperature. International Union of Crystallography 2018-04-27 /pmc/articles/PMC5988005/ /pubmed/29896057 http://dx.doi.org/10.1107/S1600576718003965 Text en © I. G. Wood et al. 2018 http://creativecommons.org/licenses/by/2.0/uk/ This is an open-access article distributed under the terms of the Creative Commons Attribution (CC-BY) Licence, which permits unrestricted use, distribution, and reproduction in any medium, provided the original authors and source are cited.http://creativecommons.org/licenses/by/2.0/uk/
spellingShingle Research Papers
Wood, Ian G.
Fortes, A. Dominic
Dobson, David P.
Wang, Weiwei
Pajdzik, Lucjan
Cosier, John
Investigation of high-pressure planetary ices by cryo-recovery. I. An apparatus for X-ray powder diffraction from 40 to 315 K, allowing ‘cold loading’ of samples
title Investigation of high-pressure planetary ices by cryo-recovery. I. An apparatus for X-ray powder diffraction from 40 to 315 K, allowing ‘cold loading’ of samples
title_full Investigation of high-pressure planetary ices by cryo-recovery. I. An apparatus for X-ray powder diffraction from 40 to 315 K, allowing ‘cold loading’ of samples
title_fullStr Investigation of high-pressure planetary ices by cryo-recovery. I. An apparatus for X-ray powder diffraction from 40 to 315 K, allowing ‘cold loading’ of samples
title_full_unstemmed Investigation of high-pressure planetary ices by cryo-recovery. I. An apparatus for X-ray powder diffraction from 40 to 315 K, allowing ‘cold loading’ of samples
title_short Investigation of high-pressure planetary ices by cryo-recovery. I. An apparatus for X-ray powder diffraction from 40 to 315 K, allowing ‘cold loading’ of samples
title_sort investigation of high-pressure planetary ices by cryo-recovery. i. an apparatus for x-ray powder diffraction from 40 to 315 k, allowing ‘cold loading’ of samples
topic Research Papers
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5988005/
https://www.ncbi.nlm.nih.gov/pubmed/29896057
http://dx.doi.org/10.1107/S1600576718003965
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