Examining Buoyancy Waves in the Martian Atmosphere with Mars Climate Sounder Robert M. Edmonds, J.R. Murphy, D.A. Teal New Mexico State University, Department of Astronomy. Introduction. Analysis Cont. MCS Results.

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Pulsar, Gravitational wave, Gravitational wave polarization. K.J.Lee Jul. 2009 NAOC. Outline. Gravity theory, Spacetime geometry Gravitational Wave and its polarization Pulsar, Pulsar timing signal Detect G-wave using pulsar Present uplimit Can we say GR is correct?.

Gravitational Wave Astronomy. Dr. Giles Hammond Institute for Gravitational Research SUPA, University of Glasgow. Universität Jena, August 2010. Statistical techniques are used to analyse analyse data from detectors Consider a measurement of a sine wave in the presence of noise

Gravitational Wave Astronomy. Dr. Giles Hammond Institute for Gravitational Research SUPA, University of Glasgow. Universität Jena, August 2010. First Experiments. Field really originated with J. Weber looking for the effect of strains in space on aluminium bars at room temperature

Searches for bursts of gravitational waves with LIGO, GEO and Virgo E. Katsavounidis MIT for the LIGO Scientific Collaboration and the Virgo Collaboration APS Meeting St. Louis, MO, April 13, 2008. Gravitational wave bursts.

Gravitational Wave Detectors. Course in Inflation, Structure formation and CMB 7 November 2002 Silvio Orsi. GW: My presentation. GW production Upper bounds on GW background Frequency range Detectors for GW: Under construction & future detectors Frequency range & sensitivity Noise

Gravitational Wave Astronomy. Dr. Giles Hammond Institute for Gravitational Research SUPA, University of Glasgow. Universität Jena, August 2010. Gravitational Waves. From our matrix all 3 terms are zero => A particle initially at rest will remain at rest.

Gravitational Wave Astronomy. Dr. Giles Hammond Institute for Gravitational Research SUPA, University of Glasgow. Universität Jena, August 2010. Estimate of Strain Amplitude. The magnitude of the metric stretch in the xx direction is or, using Kepler’s 3 rd law, which gives.

Gravitational Wave Astronomy. Dr. Giles Hammond Institute for Gravitational Research SUPA, University of Glasgow. Universität Jena, August 2010. Interferometry. The EOM applies sidebands onto the carrier light (typically few MHz)

Gravitational Wave Physics. Programme: - new initiative - Group composition (current): 3 staff, 0 postdoc, 2 PhD Investment Budget: under discussion. Jo van den Brand. First science run: May – September 2007.

Gravitational Wave Astronomy. Dr. Giles Hammond Institute for Gravitational Research SUPA, University of Glasgow. Universität Jena, August 2010. Mathematical Tools of GR. The spacetime of gravity is described by a Riemann metric