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MIT Haystack Observatory: Research Experiences for Teachers

http://www.haystack.mit.edu/edu/ret/index.html

Research Experiences for Teachers. Research Experiences for Undergraduates. Research Experiences for Teachers. Research Experiences for Teachers. RESEARCH EXPERIENCES FOR TEACHERS PROGRAM. Project for 2015:The Cryosphere is white, but not all is frozen water. Mentors: Pedro Elosegui and Michael Hecht. But imagine a world where winters are so cold that the air itself freezes to the ground? A meeting will be held at Haystack Observatory on Friday, March 27, 2015, at 4:00 PM. To provide more information and...

haystack.edu

MIT Haystack Observatory: Haystack Observatory Site Map

http://www.haystack.edu/site/sitemap.html

250 KB PDF file). Info@haystack.mit.edu. Radio Arrays (MWA, SKA, MAPS, Deuterium). Small Radio Telescope (SRT). Mark 4 VLBI Correlator. International VLBI Service (IVS). Radio Arrays (MWA, SKA, MAPS, Deuterium). Very Long Baseline Interferometry (VLBI). Research Experiences for Undergraduates (REU). Research Experiences for Teachers (RET). Northeast Radio Observatory Corp. (NEROC).

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MIT Haystack Observatory: Astronomy Wideband VLBI

http://www.haystack.edu/ast/uvlbi/index.html

The technique of very long baseline interferometry. Haystack is at the forefront of a global effort to exploit modern electronics and storage system technologies to remove this VLBI bottleneck once and for all. By developing systems based on parallelized IO in arrays of commercial hard disk drives, and high-speed digital systems to efficiently process wide bandwidths into a form suitable for recording, engineers are rapidly expanding bandwidths, and rapidly decreasing costs. Ultimately, on-site recording...

haystack.edu

MIT Haystack Observatory: Geodesy Mark 4 Correlator

http://www.haystack.edu/geo/mark4/index.html

Mark 4 VLBI Correlator. The Haystack Mark4 Correlator. Mark 4 VLBI correlators are now placed at MIT Haystack Observatory, the U.S. Naval Observatory in Washington, D.C., JIVE in The Netherlands, and at the Max Planck Institute in Bonn, Germany. In addition, large connected-element correlators based on the Mark 4 correlator ASIC chip and board are in place at the Sub-Millimeter Array (SMA) at Mauna Kea, Hawaii, and at Westerbord, The Netherlands. Papers of particular interest about the Mark 4 correlator:.

haystack.edu

MIT Haystack Observatory: Geodesy Science

http://www.haystack.edu/geo/science/index.html

Mark 4 VLBI Correlator. Geodesy is a specialized application of several familiar facets of basic mathematical and physical concepts. In practice, geodesy uses the principles of mathematics, astronomy and physics, and applies them within the capabilities of modern engineering and technology. A thorough study of the science of geodesy is not a simple undertaking. At Haystack Observatory, the science of geodesy allows researchers to make precise measurements of the Earth's plate tectonic motions.

haystack.edu

MIT Haystack Observatory: Geodesy

http://www.haystack.edu/geo/index.html

Mark 4 VLBI Correlator. Geodesy and geophysics are concerned mostly with what is going on under our feet, so it may seem ironic that these two disciplines are advanced by looking up at the stars! VLBI techniques, which were originally developed for studying radio objects in the universe can, in effect, be turned upside down to do very precise studies of the Earth. Geodetic studies help aid in the use of GPS and other navigational equipment. Geodetic VLBI in Action. Measuring tectonic plate motions.

haystack.edu

MIT Haystack Observatory: Astronomy Science

http://www.haystack.edu/ast/science/index.html

A common theme to all this research is the exploitation of cutting-edge radio astronomy techniques, the development and refinement of which are a major focus of Haystack astronomers and engineers. Very long baseline interferometry (VLBI). And the Mileura Widefield Array. Such instruments exploit modern digital data handling to create hitherto unachievable flexibility and measurement precision, again opening up new scientific vistas. Info@haystack.mit.edu. Radio Arrays (MWA, SKA, MAPS, Deuterium).

atlas.haystack.mit.edu

MIT Haystack Observatory: Millstone Hill IS Radar Realtime Displays

http://atlas.haystack.mit.edu/isr

Millstone Hill IS Radar Realtime Displays. Millstone Hill IS Radar Realtime Displays. Millstone IS Radar Status. Info@haystack.mit.edu. Radio Arrays (MWA, SKA, MAPS, Deuterium). Small Radio Telescope (SRT). Mark 4 VLBI Correlator. International VLBI Service (IVS). Radio Arrays (MWA, SKA, MAPS, Deuterium). Very Long Baseline Interferometry (VLBI). Research Experiences for Undergraduates (REU). Research Experiences for Teachers (RET). Northeast Radio Observatory Corp. (NEROC).

atlas.haystack.mit.edu

MIT Haystack Observatory: Millstone Hill Operations

http://atlas.haystack.mit.edu//index.html

Millstone Hill Incoherent Scatter Radar. ISIS Software Radio Array. Info@haystack.mit.edu. Radio Arrays (MWA, SKA, MAPS, Deuterium). Small Radio Telescope (SRT). Mark 4 VLBI Correlator. International VLBI Service (IVS). Radio Arrays (MWA, SKA, MAPS, Deuterium). Very Long Baseline Interferometry (VLBI). Research Experiences for Undergraduates (REU). Research Experiences for Teachers (RET). Northeast Radio Observatory Corp. (NEROC).

atlas.haystack.mit.edu

MIT Haystack Observatory: Millstone Hill Radar MISA Antenna

http://atlas.haystack.mit.edu/isr/status/mhr_radar_status.html

Millstone Hill UHF Radar Status. There is likely a problem in reading out the experiment description. Updated at : Thu Mar 9 16:24:30 2017 UT www@haystack.mit.edu. Info@haystack.mit.edu. Radio Arrays (MWA, SKA, MAPS, Deuterium). Small Radio Telescope (SRT). Mark 4 VLBI Correlator. International VLBI Service (IVS). Radio Arrays (MWA, SKA, MAPS, Deuterium). Very Long Baseline Interferometry (VLBI). Research Experiences for Undergraduates (REU). Research Experiences for Teachers (RET).