by Wm. Robert Johnston
last modified 1 April 2005
| Illustration of effect of gravitational waves on test masses. |
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| Animation (.gif) of spatial distortion from a plus-polarized gravitational wave traveling perpendicular to the computer screen. |
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| Animation (.gif) of a cross-polarized gravitational wave. |
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| Animation (.gif) of a circularly-polarized gravitational wave. |
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| Schematic of an interferometer gravitational wave detector such as LIGO. Numbers indicate laser (1), optics (2), beam splitter (3), recycling mirrors (4), end mirrors (5), and detector (6). |
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| Schematic of an interferometer gravitational wave detector, labeled. |
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| Sunset over LIGO-Hanford in Washington state. |
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| Tumbleweed at LIGO-Hanford, with one arm in the background. |
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| Panoramic mosaic of the LIGO-Hanford facility. |
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| Interior of the LVEA at LIGO-Livingston, Lousiana, taken in summer 2001. |
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| View along one arm of LIGO-Livingston. |
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| Graph of strain PSD for noise floor of various gravitational-wave detectors. |
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| Graph of strain PSD for noise floor of various gravitational-wave detectors, IFOs only. |
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| Graph of strain PSD for noise floor of various gravitational-wave detectors. |
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| Graph of strain PSD for predicted/modeled gravity gradient noise for LIGO-Livingston, compared to Advanced LIGO sensitivity. |
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© 2001-2005 by Wm. Robert Johnston.
Last modified 1 April 2005.
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