DocumentCode :
2304314
Title :
Set up of a Microbalance to Measure Very Low Masses
Author :
Beltrán, Domingo ; Millan Verdu, C. ; Rubio Alvarez, J. ; Domenech, Cantó ; Santonja Molto, C. ; Luna Molina, R.
Author_Institution :
Univ. Polytech. de Valencia, Valencia
fYear :
2007
fDate :
14-20 Oct. 2007
Firstpage :
337
Lastpage :
340
Abstract :
In the Laboratory of Experimental Astrophysics of the Universidad Politecnica de Valencia we make ices analogs to those that can be found in different astrophysical environments as, for example, interstellar medium and in many objects of our Solar System. We study several characteristics of these ices, like density integrated absorbance of its main absorption bands and refractive inde. In order to obtain the first, we need to measure the thickness (around 1 micrometer) and the mass (around 60 micrograms with relative error around 3%.). The first one is obtained by interferometry with lasers and the second using a quartz crystal microbalance (QCMB). It utilizes the piezoelectric qualities of quartz crystal. The application of an electric field to the gold coated quartz crystal causes a shear deformation (parallel to the gold surface). The crystal can reach the resonance if an alternating electric field is applied at a particular frequency that, for its part, depends on the mass deposited on it.
Keywords :
astronomy; gold; ice; mass measurement; microbalances; quartz; Au-SiO2; astrophysical environment; gold coated quartz crystal; ices; quartz crystal microbalance; quartz crystal piezoelectricity; shear deformation; very low mass measurement; Absorption; Astrophysics; Extraterrestrial measurements; Gold; Ice; Interferometry; Optical refraction; Quantum cascade lasers; Solar system; Thickness measurement;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Sensor Technologies and Applications, 2007. SensorComm 2007. International Conference on
Conference_Location :
Valencia
Print_ISBN :
978-0-7695-2988-2
Type :
conf
DOI :
10.1109/SENSORCOMM.2007.4394944
Filename :
4394944
Link To Document :
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