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A newly developed attachment to the Lambda 9 spectrometer for in situ reflectance measurements of catalysts at temperatures up to 623 K

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Thiede,  Manfred
Inorganic Chemistry, Fritz Haber Institute, Max Planck Society;

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Melsheimer,  Jörg
Inorganic Chemistry, Fritz Haber Institute, Max Planck Society;

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Citation

Thiede, M., & Melsheimer, J. (2002). A newly developed attachment to the Lambda 9 spectrometer for in situ reflectance measurements of catalysts at temperatures up to 623 K. Talk presented at PerkinElmer Colloquium Optical Spectroscopy - COSP 2002. Berlin. 2002-11-11 - 2002-11-12.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-1327-9
Abstract
A newly developed attachment to the Lambda 9 spectrometer for in situ reflectance measurements of catalysts at temperatures up to 623 K

M.Thiede and J.Melsheimer

Fritz-Haber-Institut der Max-Planck-Gesellschaft, Department of Inorganic Chemistry, Faradayweg 4-6, 14195 Berlin, Germany

Abstract

The spectroscopic investigation of catalyst powders under reaction conditions is generally possible only in reflectance.

Two problems occur:

1. Low signal level

Normally the sample is positioned directly at the integrating sphere and all diffusely scattered light from the sample is reflected back into the integrating sphere.
A hot reactor cell cannot be attached directly, it must be positioned as far as possible from the integrating sphere to avoid its heating.
If the reactor cell is attached at some distance from the measurement window of the integrating sphere only a portion of the diffusely scattered light will be reflected back into the sphere. At a distance of 12 mm, for example, this will only be 20%.
In a first setup we bridged the distance with highly reflecting ceramics, to increase the part of light reflected into the sphere (Fig.1).

2. Thermal radiation

The thermal radiation of the hot reactor cell also enters the integrating sphere.At higher temperatures it is significantly stronger than the measurement light from the spectrometer itself. This leads to increased noise and saturation of the detector.

In the newly developed setup we tried

a. to make the distance between integrating sphere and reactor cell with oven as large as possible;
b. to increase the signal level
c. to decrease the surface which causes the thermal radiation, and
d. to bring reactor cell and oven into a vertical position which facilitates the work with powder samples.

These requirements could be fulfilled by the application of a specially formed light conductor made of quartz, in which the light is conducted to the sample and back into the integrating sphere by total reflectance. At the same time, the surface which causes the thermal radiation was reduced (Fig.2).

In this way, we succeeded in improving the signal-to-noise ratio by a factor of 4-5 compared with the first setup.