Q 64: Precision measurements and metrology VI
Friday, March 22, 2013, 14:00–15:45, E 001
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14:00 |
Q 64.1 |
A long reference cavity with contribution from thermal noise to frequency instability of below 10−16 — •Sebastian Häfner, Stefan Vogt, Stephan Falke, Christian Lisdat, and Uwe Sterr
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14:15 |
Q 64.2 |
Laser ranging for GRACE follow-on — •Daniel Schütze, Gunnar Stede, Vitali Müller, Alexander Görth, Oliver Gerberding, Christoph Mahrdt, Benjamin Sheard, Gerhard Heinzel, and Karsten Danzmann
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14:30 |
Q 64.3 |
General Astigmatic Gaussian Beam Model — •Evgenia Kochkina, Dennis Schmelzer, Gudrun Wanner, Gerhard Heinzel, and Karsten Danzmann
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14:45 |
Q 64.4 |
Ultra-stable 39.5 cm long optical cavity with reduced thermal noise — •Sana Amairi and Piet O. Schmidt
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15:00 |
Q 64.5 |
Digital unterstützte heterodyn Interferometrie — •Katharina-Sophie Isleif, Sina Köhlenbeck, Oliver Gerberding, Stefan Goßler, Gerhard Heinzel und Karsten Danzmann
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15:15 |
Q 64.6 |
Coating thermal noise interferometer — •Tobias Westphal and the AEI 10m Prototype team
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15:30 |
Q 64.7 |
Control of optical cavities in light-shining-through-a-wall experiments — •Robin Baehre
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