Details
| Originalsprache | Englisch |
|---|---|
| Publikationsstatus | Veröffentlicht - 2013 |
| Veranstaltung | 2013 Conference on Lasers and Electro-Optics Europe and International Quantum Electronics Conference, CLEO/Europe-IQEC 2013 - Munich, Deutschland Dauer: 12 Mai 2013 → 16 Mai 2013 |
Konferenz
| Konferenz | 2013 Conference on Lasers and Electro-Optics Europe and International Quantum Electronics Conference, CLEO/Europe-IQEC 2013 |
|---|---|
| Land/Gebiet | Deutschland |
| Ort | Munich |
| Zeitraum | 12 Mai 2013 → 16 Mai 2013 |
Abstract
Applications in gravitational wave detectors [1] require high power lasers with approximately 200 W of single-frequency output in linearly polarized TEM00-mode. Single-frequency signals have been amplified to more than 500 W in master oscillator power amplifier (MOPA) configurations, employing photonic crystal fibers (PCF) [2] as well as chirally coupled core (CCC) fibers [3]. For a PCF amplifier system, a fundamental Gaussian mode power of 203 W was demonstrated in linear polarization [4]. In this contribution we report for the first time measurements of the overlap of high power CCC fiber amplifiers output beam with the TEM00-mode of a scanning non-confocal ring cavity [5].
ASJC Scopus Sachgebiete
- Ingenieurwesen (insg.)
- Elektrotechnik und Elektronik
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2013. Beitrag in 2013 Conference on Lasers and Electro-Optics Europe and International Quantum Electronics Conference, CLEO/Europe-IQEC 2013, Munich, Deutschland.
Publikation: Konferenzbeitrag › Paper › Forschung › Peer-Review
}
TY - CONF
T1 - Fundamental Gaussian mode content measurements on active large core CCC fibers
AU - Karow, M.
AU - Zhu, C.
AU - Kracht, D.
AU - Neumann, J.
AU - Galvanauskas, A.
AU - Wessels, P.
PY - 2013
Y1 - 2013
N2 - Applications in gravitational wave detectors [1] require high power lasers with approximately 200 W of single-frequency output in linearly polarized TEM00-mode. Single-frequency signals have been amplified to more than 500 W in master oscillator power amplifier (MOPA) configurations, employing photonic crystal fibers (PCF) [2] as well as chirally coupled core (CCC) fibers [3]. For a PCF amplifier system, a fundamental Gaussian mode power of 203 W was demonstrated in linear polarization [4]. In this contribution we report for the first time measurements of the overlap of high power CCC fiber amplifiers output beam with the TEM00-mode of a scanning non-confocal ring cavity [5].
AB - Applications in gravitational wave detectors [1] require high power lasers with approximately 200 W of single-frequency output in linearly polarized TEM00-mode. Single-frequency signals have been amplified to more than 500 W in master oscillator power amplifier (MOPA) configurations, employing photonic crystal fibers (PCF) [2] as well as chirally coupled core (CCC) fibers [3]. For a PCF amplifier system, a fundamental Gaussian mode power of 203 W was demonstrated in linear polarization [4]. In this contribution we report for the first time measurements of the overlap of high power CCC fiber amplifiers output beam with the TEM00-mode of a scanning non-confocal ring cavity [5].
UR - http://www.scopus.com/inward/record.url?scp=84900325636&partnerID=8YFLogxK
U2 - 10.1109/CLEOE-IQEC.2013.6801298
DO - 10.1109/CLEOE-IQEC.2013.6801298
M3 - Paper
AN - SCOPUS:84900325636
T2 - 2013 Conference on Lasers and Electro-Optics Europe and International Quantum Electronics Conference, CLEO/Europe-IQEC 2013
Y2 - 12 May 2013 through 16 May 2013
ER -