Not long ago I came across a piece in the Scientific American archives from the earliest days of very - long
baseline radio interferometry, the technique employed by the Event Horizon Telescope.
Not exact matches
The observatory includes three
radio telescopes for Very Long
Baseline Interferometry (VLBI), which receive
radio waves emitted by quasars.
Currently, the best measurements of those variables come from a system called very - long -
baseline interferometry (VLBI), which uses
radio dishes spaced across Earth to stare at quasars — brilliant beacons in the distant universe that occasionally flicker.
MRI is used to image tissues deep within the human body and tells us whether we might suffer from an illness, while atomic clocks are extremely precise timekeepers used for GPS, internet synchronization, and long
baseline interferometry in
radio - astronomy.
The four new telescopes will form part of the worldwide network of
radio telescopes known as VGOS (Very Long
Baseline Interferometry 2010 Global Observing System).
In particular, VLBI (very long
baseline interferometry) uses a global network of
radio telescopes spread across different continents to form a virtual Earth - sized telescope.
2000 V. Tudose (Netherlands Institute for
Radio Astronomy - ASTRON), Z. Paragi (Joint Institute for Very Long
Baseline Interferometry in Europe - JIVE), P. Soleri, D.M. Russell, D. Maitra (Amsterdam), F. Lewis (FT), R.P. Fender (Southampton), M.A. Garrett (ASTRON), R.E. Spencer, A. Rushton (Jodrell Bank)
These networks of
radio telescopes use sophisticated computer and communication technology called very long
baseline interferometry (VLBI) to function as single continent spanning telescopes - the greatest eyes - on - the - sky ever created.
This telescope observes as a space - based
radio telescope, but also can be used with other
radio telescopes on Earth for what is called Space Very Long
Baseline Interferometry.
However, by combining high - frequency
radio telescopes around the world, in a technique called very long
baseline interferometry, or VLBI, even such a tiny feature is in principle detectable.
Very long
baseline interferometry (VLBI) is a technique used by
radio astronomers to electronically link widely separated
radio telescopes together so they work as if they were a single instrument with extraordinarily sharp «vision,» or resolving power.
The technique of combining
radio waves, known as very long
baseline interferometry, is common enough in
radio astronomy.
Thanks to recent distance measurements with an international network of
radio telescopes, including the EVN (European Very Long
Baseline Interferometry Network) telescopes, the NSF's Green Bank Telescope and Arecibo Observatory, astronomers realized that VLA J2130 +12 is at a distance of 7,200 light years, showing that it is well within our own Milky Way galaxy and about five times closer than M15.
Another team, led by scientists from the Joint Institute for Very Long
Baseline Interferometry in Europe (JIVE), in Dwingeloo, The Netherlands, will use a world - wide network of
radio telescopes, including the NRAO telescopes, to track the probe's trajectory with unprecedented accuracy.
With the technique of very long
baseline interferometry, astronomers can hook up
radio telescopes, distant from one another in different countries and on continents, to mimic a single «virtual» telescope with an aperture as wide as Earth.
The Ministries of Ghana and South Africa announce the combination of «first light» science observations which confirm the successful conversion of the Ghana communications antenna from a redundant telecoms instrument into a functioning Very Long
Baseline Interferometry (VLBI)
radio telescope.
The satellite is part of an international collaboration led by ISAS and backed by Japan's National Astronomical Observatory; NASA's Jet Propulsion Laboratory (JPL), Pasadena, CA; the National Science Foundation's National
Radio Astronomy Observatory (NRAO), Socorro, NM; the Canadian Space Agency; the Australia Telescope National Facility; the European VLBI Network and the Joint Institute for Very Long
Baseline Interferometry in Europe.
Very long
baseline interferometry is a technique used by
radio astronomers to electronically link widely separated
radio telescopes together so they work as if they were a single instrument with extraordinarily sharp «vision,» or resolving power.
Although super small, this angular size can actually be resolved by astronomical observations using an interferometric technique at
radio wavelengths, called Very Long
Baseline Interferometry or VLBI (see here for details).