Please use this identifier to cite or link to this item:
|Title:||Type 1A fibre bragg grating photosensitivity and the development of optimum temperature invariant type i - type ia strain sensors||Authors:||Kalli, Kyriacos
Simpson, Alexander George
|Keywords:||Bragg gratings;Optical fibers;Strain gages;Fibers||Category:||Electrical Engineering - Electronic Engineering - Information Engineering||Field:||Engineering and Technology||Issue Date:||Apr-2004||Publisher:||Spie Digital Library||Source:||Proceedings of SPIE - The International Society for Optical Engineering,2004, vol. 5459, pp. 118-127; Optical Sensing; Strasbourg; France; 27 April 2004 through 29 April 2004||Journal:||Proceedings of SPIE - The International Society for Optical Engineering||Conference:||Optical Sensing||Abstract:||Type 1A fibre Bragg gratings (FBG) form only after the erasure of a standard grating in hydrogenated germanosilicate fibre, under prolonged UV exposure. They are distinct from other grating types as they exhibit a uniquely large increase in the mean index of the core, readily identifiable by a large red shift in the Bragg wavelength. Type 1A gratings can surpass the conventional mean index change by a factor of six with a typical red shift of up to 20nm, interpreted as a mean index increase of up to 1.9×10 -2. Importantly, 1A gratings have been shown to exhibit the lowest temperature coefficient of all FBG, which makes them ideal for use as temperature compensated, dual grating sensors. We report on the formation of Type 1A gratings and the correlation between the mean index change of the grating and the growth of a loss band at close to 1400nm that is associated with the formation of OH centres within the fibre. We present annealing data comparing the decay of Type 1 and Type 1A gratings. Finally, we demonstrate a dual temperature compensated strain sensor system, based on two adjoining Type 1 and Type 1A gratings, which have been formed using a common phase mask, yet with central wavelengths many nm apart.||ISSN:||0277-786X||DOI:||10.1117/12.545299||Rights:||© 2004 SPIE.||Type:||Conference Papers|
|Appears in Collections:||Άρθρα/Articles|
Show full item record
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.