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Examples
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Modern professional telescopes use adaptive optics (tiny rapid changes in the mirror to compensate for atmospheric disturbances) and long-baseline interferometry (using several small telescopes to simulate a much larger single telescope) to achieve results nearly equivalent to space-based telescopes.
8/1/08: Launch Pad, day 2 prof_brotherton 2008
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The light version of radio LBI (long-baseline interferometry) is just starting, and may produce reconstructed images of stellar discs (albeit with rather low S/N), and then there's the technique for reconstructing starspots …
Astronomers Find Type Ia Supernova Just Waiting to Happen | Universe Today 2009
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Generally you improve the bounds on such couplings when you have a long-baseline for the photon.
The Screwy Universe Sean 2006
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The MINOS Experiment is a long-baseline neutrino experiment designed to observe the phenomena of neutrino oscillations, an effect which is related to neutrino mass.
Small Things Considered cjohnson 2006
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It is expected that Earth-based ESA stations will take part in controlling Phobos-Grunt, receiving telemetry and making trajectory measurements, including implementation of very long-baseline interferometry (VLBI).
PhysOrg.com - latest science and technology news stories PhysOrg Team 2010
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It is expected that Earth-based ESA stations will take part in controlling Phobos-Grunt, receiving telemetry and making trajectory measurements, including implementation of very long-baseline interferometry (VLBI).
D Mag - News 2010
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The team, led by Makoto Kishimoto from the Max Planck Institute for Radio Astronomy in Bonn, combined infrared imaging from the United Kingdom Infrared Telescope (UKIRT) and some of the first ever infrared long-baseline interferometric measurements from the Keck Observatory to observe the nearby AGN.
Gaea Times (by Simple Thoughts) Breaking News and incisive views 24/7 2009
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The team, led by Makoto Kishimoto from the Max Planck Institute for Radio Astronomy in Bonn, combined infrared imaging from the United Kingdom Infrared Telescope (UKIRT) and some of the first ever infrared long-baseline interferometric measurements from the Keck Observatory to observe the nearby AGN.
Gaea Times (by Simple Thoughts) Breaking News and incisive views 24/7 2009
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This type of instrument is called a long-baseline interferometer.
Signs of the Times 2009
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Atmospheric data are always present in any long-baseline neutrino detector: ATM and LBL provide complementary information on neutrino parameters, information in particular on hierarchy and octant degeneracy.
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