VLA Very Large Array - vertaling naar Engels
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VLA Very Large Array - vertaling naar Engels

RADIO ASTRONOMY OBSERVATORY LOCATED ON THE PLAINS OF SAN AGUSTIN
Very Large Array Radio Telescope; EVLA; Expanded Very Large Array; JVLA; Y27; Karl G. Jansky Very Large Array
  • The Bracewell Radio Sundial on the VLA walking tour, seen from the south. Named for [[Ronald N. Bracewell]], this sundial marks on the ground positions of the shadow of the central sphere (the [[gnomon]]) at different times of day and times of year. The shadow on Dec 22, 2017 falls very near the [[winter solstice]] line and the 1:00 PM (solar time) mark.  The other two lines of markers north of the gnomon are for the [[equinox]]es and the [[summer solstice]].  Additional lines of markers south of the gnomon mark positions of "shadows" of the radio sources [[Cygnus A]] and [[Cassiopeia A]]. The posts at the back of the sundial were recovered from Bracewell's radio telescope array at [[Stanford University]], abandoned in 1980, where they had been signed by visitors with chisels at his invitation.
  • website=National Radio Astronomy Observatory}}</ref>

VLA Very Large Array      
VLA Very Large Array noun радиотелескоп с очень большой антенной системой
ULSI         
PROCESS OF CREATING AN INTEGRATED CIRCUIT BY COMBINING THOUSANDS OF TRANSISTORS INTO A SINGLE CHIP; BEGAN IN THE 1970S WHEN COMPLEX SEMICONDUCTOR AND COMMUNICATION TECHNOLOGIES WERE BEING DEVELOPED
VLSI; Very-Large-Scale Integration; Very Large-Scale Integration; Very Large-scale Integration; Very large-scale integration; ULSI; Structured VLSI design; Deep Submicron; Deep Submicrometre; Very Large System Integration; Analog VLSI; Analog vlsi; Vlsi; VLSI circuit; Very large scale integration; Very-large-scale integration; VLSI device; History of VLSI; VLSI design

общая лексика

Ultra Large Scale Integration

ультрабольшая интеграция, УБИС

микросхема с очень высокой плотностью размещения элементов. К таким схемам можно отнести современные процессоры, в которых число транзисторов на кристалле составляет от 10 млн. до 1 млрд

VLSI         
PROCESS OF CREATING AN INTEGRATED CIRCUIT BY COMBINING THOUSANDS OF TRANSISTORS INTO A SINGLE CHIP; BEGAN IN THE 1970S WHEN COMPLEX SEMICONDUCTOR AND COMMUNICATION TECHNOLOGIES WERE BEING DEVELOPED
VLSI; Very-Large-Scale Integration; Very Large-Scale Integration; Very Large-scale Integration; Very large-scale integration; ULSI; Structured VLSI design; Deep Submicron; Deep Submicrometre; Very Large System Integration; Analog VLSI; Analog vlsi; Vlsi; VLSI circuit; Very large scale integration; Very-large-scale integration; VLSI device; History of VLSI; VLSI design

общая лексика

Very Large-Scale Integration

сверхбольшая степень интеграции, сверхбольшая интегральная микросхема, СБИС

микросхема, содержащая на кристалле от 100 000 до 10 млн. транзисторов или логических вентилей

(Very Large Scale Integration) сверхбольшая степень интеграции (СБИС)

Смотрите также

GSI; integrated circuit; LSI; MSI; SSI; ULSI

существительное

общая лексика

очень широкомасштабная интеграция

синоним

Very Large Scale Integration

Definitie

Very Large Scale Integration
<hardware> (VLSI) A term describing semiconductor {integrated circuits} composed of hundreds of thousands of logic elements or memory cells. (1995-01-11)

Wikipedia

Very Large Array

The Karl G. Jansky Very Large Array (VLA) is a centimeter-wavelength radio astronomy observatory in the southwestern United States. It lies in central New Mexico on the Plains of San Agustin, between the towns of Magdalena and Datil, ~50 miles (80 km) west of Socorro. The VLA comprises twenty-eight 25-meter radio telescopes (twenty-seven of which are operational while one is always rotating through maintenance) deployed in a Y-shaped array and all the equipment, instrumentation, and computing power to function as an interferometer. Each of the massive telescopes is mounted on double parallel railroad tracks, so the radius and density of the array can be transformed to adjust the balance between its angular resolution and its surface brightness sensitivity. Astronomers using the VLA have made key observations of black holes and protoplanetary disks around young stars, discovered magnetic filaments and traced complex gas motions at the Milky Way's center, probed the Universe's cosmological parameters, and provided new knowledge about the physical mechanisms that produce radio emission.

The VLA stands at an elevation of 6,970 feet (2,120 m) above sea level. It is a component of the National Radio Astronomy Observatory (NRAO). The NRAO is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.

Vertaling van &#39VLA Very Large Array&#39 naar Russisch