Q 49: Precision Measurements and Metrology VI
Thursday, March 11, 2010, 14:00–16:15, A 310
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14:00 |
Q 49.1 |
A Silent Symphony: Das weltweite Netz der Gravitationswellendetektoren — •Hartmut Grote
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14:15 |
Q 49.2 |
Laser interferometry for next generation geodesy missions — •Benjamin Sheard, Marina Dehne, Christoph Mahrdt, Vitali Mueller, Martin Sommerfeld, Gerhard Heinzel, and Karsten Danzmann
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14:30 |
Q 49.3 |
The LISA mission - a gravitational wave detector in space — •Gerhard Heinzel and Karsten Danzmann
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14:45 |
Q 49.4 |
Modeling interferometers for space based observations of Earth's variable gravity field — •Christoph Mahrdt, Benjamin Sheard, Marina Dehne, Gerhard Heinzel, and Karsten Danzmann
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15:00 |
Q 49.5 |
Das Einstein Teleskop: ein Gravitationswellendetektor der dritten Generation — •Harald Lück für das ET Science Team
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15:15 |
Q 49.6 |
Inter-spacecraft laser ranging and data communication for LISA — •Juan Jose Esteban Delgado, Antonio Garcia Marin, Johannes Eichholz, Iouri Bykov, Joachim Kullmann, Gerhard Heinzel, and Karsten Danzmann
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15:30 |
Q 49.7 |
Inter-spacecraft 2 GHz clock-tone transmission with high phase fidelity at ultra low frequencies — •Simon Barke, Michael Tröbs, Gerhard Heinzel, and Karsten Danzmann
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15:45 |
Q 49.8 |
Implementierung und Kontrolle eines Mode Cleaner Resonators am Ausgang des Gravitationswellendetektors GEO600 — •Mirko Prijatelj und Das GEO600-Team
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16:00 |
Q 49.9 |
The GEO600 Squeezed Light Laser — •Henning Vahlbruch, Alexander Khalaidovski, Nico Lastzka, Christian Graef, Karsten Danzmann, and Roman Schnabel
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