LAGRANGE: LAser GRavitational-wave ANtenna at GEo-lunar Lagrange points

We describe a new space gravitational wave observatory design called LAGRANGE that maintains all important LISA science at about half the cost and with reduced technical risk. It consists of three drag-free spacecraft in the most stable geocentric formation, the Earth-Moon L3, L4, and L5 Lagrange po...

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Veröffentlicht in:	arXiv.org 2011-12
Hauptverfasser:	Conklin, J W, Buchman, S, Aguero, V, Alfauwaz, A, Aljadaan, A, Almajed, M, Altwaijry, H, Al-Saud, T, Balakrishnan, K, Byer, R L, Bower, K, Costello, B, Cutler, G D, DeBra, D B, Faied, D M, Foster, C, Genova, A L, Hanson, J, Hooper, K, Hultgren, E, Jaroux, B, Klavins, A, Lantz, B, Lipa, J A, Palmer, A, Plante, B, Sanchez, H S, Saraf, S, Schaechter, D, Sherrill, T, K -L Shu, Smith, E, Tenerelli, D, Vanbezooijen, R, Vasudevan, G, Williams, S D, Worden, S P, Zhou, J, Zoellner, A
Format:	Artikel
Sprache:	eng
Schlagworte:	Charge materials Design Drag Frequency standards Gravitation Gravitational wave antennas Gravitational waves Gyroscopes Inertial reference systems Lagrangian equilibrium points Management systems Moon Sensors Space missions Telescopes
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