University of Dayton Chautauqua Course

 

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Chautauqua Course DAY-6

 

Interferometry in Radio Astronomy, the VLA and the VLBA

 

DAVID G.  FINLEY and STAFF, National Radio Astronomy Observatory

 

July 9-11, 2008 in and near Socorro, NM --- Apply to the Dayton Center --- To apply for this course now - click here

 

Note:     This course is cosponsored by and offered at the National Radio Astronomy Observatory in Socorro, New Mexico.  Applications should be sent to the DAY Field Center.  Limited on-site lodging will be available to early applicants.  This course, along with the course The Radio Universe and the Green Bank Telescope (DAY-5), form a two‑session pair.  Applications from individuals applying for both and received by the end of February will receive priority consideration.  Single course applications are also welcome for both.

 

Multiple radio telescopes used in concert can form a synthetic antenna providing the resolving power of a much larger dish. These techniques of interferometry are the focus of this course.  Twenty‑seven identical reflector antennas operating together on the Plains of San Agustin in New Mexico form the Very Large Array (VLA). They are interconnected, and each can be moved to different observing stations over an area of about 20 by 20 miles. The 25 meter (82‑foot) antennas are precise, yet strong enough to stand the snow and wind at the 7000‑foot elevation of the site.  They are moved every few months to different locations in the Y‑shaped layout. They are controlled by a central observing station to which they return data. The VLA is an extremely versatile research instrument and a valuable tool for investigations ranging from planetary and other solar‑system observations, to studies of stellar life cycles, galactic structure and evolution, and cosmological studies of the far‑distant universe.  Dedicated in 1980, the VLA now is undergoing a major expansion, aimed at replacing older technologies with equipment at the current state of the art.  This project, resulting in an Expanded VLA (EVLA), will increase the scientific capabilities of the instrument tenfold.

 

The Very Long Baseline Array (VLBA) is composed of ten identical 25‑meter reflector antennas located at independent sites geographically distributed across the United States, from Hawaii to the Virgin Islands. Each antenna independently records data, which is then synthesized into output with the resolution of an 8000‑kilometer (5000 miles) single radio telescope. The VLBA's extremely high resolution makes it a premier tool for researchers studying the details of stars and other objects within the Milky Way, as well as distant galaxies, quasars and gravitational‑lens systems. In addition, the VLBA provides important data on Earth's plate‑tectonic movements.

 

The course will be held at the NRAO Array Operations Center in Socorro, NM.  It will feature lectures by research astronomers on areas of current research in which the VLA and the VLBA play world-leading roles.  Techniques for radio astronomy interferometry will be described.  Participants will tour control rooms and central computer processing facilities at the Operations Center.  On the second day of the course, participants will take an in-depth tour of the VLA.  Current and future observing programs with the VLA, EVLA, and VLBA will be discussed, along with the scientific contributions expected from the Atacama Large Millimeter Array (ALMA), an international millimeter-wavelength interferometer under construction in Chile's high Atacama  Desert.

 

For college teachers of:  all disciplines.  Prerequisites: the Chautauqua course, The Radio Universe and the Green Bank Telescope, or equivalent elementary knowledge of radio astronomy.

 


 

Costs for 2008

Application fee: $100 [$50 if received by February 29, 2008]

Course fee: $295 [Due in March 2008]

Optional on-site lodging: $25 per person per night in a single

 


 

David G. Finley is Public Information Officer for the National Radio Astronomy Observatory in Socorro, NM.  A former science editor and writer for The Miami Herald, he taught astronomy and geology at Florida International University in Miami.  Author of one book and co-editor of another, his articles on astronomy and other topics have appeared in numerous publications, including Astronomy and Air & Space.  He has lectured extensively at observatories, museums, universities, national parks, aboard cruise ships and to clubs and organizations.  The staff includes other scientists, electronics engineers and programmers.

 

 

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University of Dayton Chautauqua Course