Logo
Unionpedia
Communication
Get it on Google Play
New! Download Unionpedia on your Android™ device!
Install
Faster access than browser!
 

Very-long-baseline interferometry

Index Very-long-baseline interferometry

Very-long-baseline interferometry (VLBI) is a type of astronomical interferometry used in radio astronomy. [1]

52 relations: Astrometry, Astronomical interferometer, Astronomical radio source, Atomic clock, Australia, Canada, Closure phase, Coaxial cable, Earth orientation parameters, Europe, European VLBI Network, Event Horizon Telescope, GÉANT, Geodesy, Gravity, HALCA, Hard disk drive, Huygens (spacecraft), Hydrogen maser, Interferometry, International Association of Geodesy, International Astronomical Union, International Celestial Reference Frame, Japan, Joint Institute for VLBI in Europe, Magnetic tape data storage, Maser, Messier 87, Mexico, Milky Way, Minute and second of arc, Moon, Optical fiber, Plate tectonics, Quasar, Radio astronomy, Radio telescope, Roger Clifton Jennison, Russia, Salyut 6, Solar System, South Korea, Speed of gravity, Spektr-R, Sun, Supermassive black hole, Titan (moon), Transmission line, United States, Very Long Baseline Array, ..., Very-long-baseline interferometry, Waveguide. Expand index (2 more) »

Astrometry

Astrometry is the branch of astronomy that involves precise measurements of the positions and movements of stars and other celestial bodies.

New!!: Very-long-baseline interferometry and Astrometry · See more »

Astronomical interferometer

An astronomical interferometer is an array of separate telescopes, mirror segments, or radio telescope antennas that work together as a single telescope to provide higher resolution images of astronomical objects such as stars, nebulas and galaxies by means of interferometry.

New!!: Very-long-baseline interferometry and Astronomical interferometer · See more »

Astronomical radio source

Astronomical radio sources are objects in outer space that emit strong radio waves.

New!!: Very-long-baseline interferometry and Astronomical radio source · See more »

Atomic clock

An atomic clock is a clock device that uses an electron transition frequency in the microwave, optical, or ultraviolet region of the electromagnetic spectrum of atoms as a frequency standard for its timekeeping element.

New!!: Very-long-baseline interferometry and Atomic clock · See more »

Australia

Australia, officially the Commonwealth of Australia, is a sovereign country comprising the mainland of the Australian continent, the island of Tasmania and numerous smaller islands.

New!!: Very-long-baseline interferometry and Australia · See more »

Canada

Canada is a country located in the northern part of North America.

New!!: Very-long-baseline interferometry and Canada · See more »

Closure phase

The closure phase is an observable quantity in imaging astronomical interferometry, which allowed the use of interferometry with very long baselines.

New!!: Very-long-baseline interferometry and Closure phase · See more »

Coaxial cable

Cross-sectional view of a coaxial cable Coaxial cable, or coax (pronounced), is a type of electrical cable that has an inner conductor surrounded by a tubular insulating layer, surrounded by a tubular conducting shield.

New!!: Very-long-baseline interferometry and Coaxial cable · See more »

Earth orientation parameters

In geodesy, earth orientation parameters (EOP) are a collection of parameters that describe irregularities in the rotation of the Earth.

New!!: Very-long-baseline interferometry and Earth orientation parameters · See more »

Europe

Europe is a continent located entirely in the Northern Hemisphere and mostly in the Eastern Hemisphere.

New!!: Very-long-baseline interferometry and Europe · See more »

European VLBI Network

The European very-long-baseline interferometry (VLBI) Network was formed in 1980 by a consortium of five of the major radio astronomy institutes in Europe (the European Consortium for VLBI).

New!!: Very-long-baseline interferometry and European VLBI Network · See more »

Event Horizon Telescope

The Event Horizon Telescope (EHT) is a project to create a large telescope array consisting of a global network of radio telescopes and combining data from several very-long-baseline interferometry (VLBI) stations around the Earth.

New!!: Very-long-baseline interferometry and Event Horizon Telescope · See more »

GÉANT

GÉANT is the pan-European data network for the research and education community.

New!!: Very-long-baseline interferometry and GÉANT · See more »

Geodesy

Geodesy, also known as geodetics, is the earth science of accurately measuring and understanding three of Earth's fundamental properties: its geometric shape, orientation in space, and gravitational field.

New!!: Very-long-baseline interferometry and Geodesy · See more »

Gravity

Gravity, or gravitation, is a natural phenomenon by which all things with mass or energy—including planets, stars, galaxies, and even light—are brought toward (or gravitate toward) one another.

New!!: Very-long-baseline interferometry and Gravity · See more »

HALCA

HALCA (Highly Advanced Laboratory for Communications and Astronomy), also known for its project name VSOP (VLBI Space Observatory Programme), or the code name MUSES-B (for the second of the Mu Space Engineering Spacecraft series), is a Japanese 8 meter diameter radio telescope satellite which was used for Very Long Baseline Interferometry (VLBI).

New!!: Very-long-baseline interferometry and HALCA · See more »

Hard disk drive

A hard disk drive (HDD), hard disk, hard drive or fixed disk is an electromechanical data storage device that uses magnetic storage to store and retrieve digital information using one or more rigid rapidly rotating disks (platters) coated with magnetic material.

New!!: Very-long-baseline interferometry and Hard disk drive · See more »

Huygens (spacecraft)

Huygens was an atmospheric entry probe that landed successfully on Saturn's moon Titan in 2005.

New!!: Very-long-baseline interferometry and Huygens (spacecraft) · See more »

Hydrogen maser

A hydrogen maser, also known as hydrogen frequency standard, is a specific type of maser that uses the intrinsic properties of the hydrogen atom to serve as a precision frequency reference.

New!!: Very-long-baseline interferometry and Hydrogen maser · See more »

Interferometry

Interferometry is a family of techniques in which waves, usually electromagnetic waves, are superimposed causing the phenomenon of interference in order to extract information.

New!!: Very-long-baseline interferometry and Interferometry · See more »

International Association of Geodesy

The International Association of Geodesy is a constituent Association of the International Union of Geodesy and Geophysics.

New!!: Very-long-baseline interferometry and International Association of Geodesy · See more »

International Astronomical Union

The International Astronomical Union (IAU; Union astronomique internationale, UAI) is an international association of professional astronomers, at the PhD level and beyond, active in professional research and education in astronomy.

New!!: Very-long-baseline interferometry and International Astronomical Union · See more »

International Celestial Reference Frame

In astrometry, an International Celestial Reference Frame (ICRF) is a realization of the International Celestial Reference System (ICRS) using reference celestial sources observed at radio wavelengths.

New!!: Very-long-baseline interferometry and International Celestial Reference Frame · See more »

Japan

Japan (日本; Nippon or Nihon; formally 日本国 or Nihon-koku, lit. "State of Japan") is a sovereign island country in East Asia.

New!!: Very-long-baseline interferometry and Japan · See more »

Joint Institute for VLBI in Europe

The Joint Institute for VLBI ERIC (JIVE) was formed in 1993 by the European Consortium for VLBI and is the central facility of the European VLBI Network (EVN).

New!!: Very-long-baseline interferometry and Joint Institute for VLBI in Europe · See more »

Magnetic tape data storage

Magnetic tape data storage is a system for storing digital information on magnetic tape using digital recording.

New!!: Very-long-baseline interferometry and Magnetic tape data storage · See more »

Maser

A maser (an acronym for "microwave amplification by stimulated emission of radiation") is a device that produces coherent electromagnetic waves through amplification by stimulated emission.

New!!: Very-long-baseline interferometry and Maser · See more »

Messier 87

Messier 87 (also known as Virgo A or NGC 4486, generally abbreviated to M87) is a supergiant elliptical galaxy in the constellation Virgo.

New!!: Very-long-baseline interferometry and Messier 87 · See more »

Mexico

Mexico (México; Mēxihco), officially called the United Mexican States (Estados Unidos Mexicanos) is a federal republic in the southern portion of North America.

New!!: Very-long-baseline interferometry and Mexico · See more »

Milky Way

The Milky Way is the galaxy that contains our Solar System.

New!!: Very-long-baseline interferometry and Milky Way · See more »

Minute and second of arc

A minute of arc, arcminute (arcmin), arc minute, or minute arc is a unit of angular measurement equal to of one degree.

New!!: Very-long-baseline interferometry and Minute and second of arc · See more »

Moon

The Moon is an astronomical body that orbits planet Earth and is Earth's only permanent natural satellite.

New!!: Very-long-baseline interferometry and Moon · See more »

Optical fiber

An optical fiber or optical fibre is a flexible, transparent fiber made by drawing glass (silica) or plastic to a diameter slightly thicker than that of a human hair.

New!!: Very-long-baseline interferometry and Optical fiber · See more »

Plate tectonics

Plate tectonics (from the Late Latin tectonicus, from the τεκτονικός "pertaining to building") is a scientific theory describing the large-scale motion of seven large plates and the movements of a larger number of smaller plates of the Earth's lithosphere, since tectonic processes began on Earth between 3 and 3.5 billion years ago.

New!!: Very-long-baseline interferometry and Plate tectonics · See more »

Quasar

A quasar (also known as a QSO or quasi-stellar object) is an extremely luminous active galactic nucleus (AGN).

New!!: Very-long-baseline interferometry and Quasar · See more »

Radio astronomy

Radio astronomy is a subfield of astronomy that studies celestial objects at radio frequencies.

New!!: Very-long-baseline interferometry and Radio astronomy · See more »

Radio telescope

A radio telescope is a specialized antenna and radio receiver used to receive radio waves from astronomical radio sources in the sky in radio astronomy.

New!!: Very-long-baseline interferometry and Radio telescope · See more »

Roger Clifton Jennison

Roger Clifton Jennison (18 December 1922 – 29 December 2006) worked as a radio astronomer at Jodrell Bank under the guidance of Robert Hanbury Brown.

New!!: Very-long-baseline interferometry and Roger Clifton Jennison · See more »

Russia

Russia (rɐˈsʲijə), officially the Russian Federation (p), is a country in Eurasia. At, Russia is the largest country in the world by area, covering more than one-eighth of the Earth's inhabited land area, and the ninth most populous, with over 144 million people as of December 2017, excluding Crimea. About 77% of the population live in the western, European part of the country. Russia's capital Moscow is one of the largest cities in the world; other major cities include Saint Petersburg, Novosibirsk, Yekaterinburg and Nizhny Novgorod. Extending across the entirety of Northern Asia and much of Eastern Europe, Russia spans eleven time zones and incorporates a wide range of environments and landforms. From northwest to southeast, Russia shares land borders with Norway, Finland, Estonia, Latvia, Lithuania and Poland (both with Kaliningrad Oblast), Belarus, Ukraine, Georgia, Azerbaijan, Kazakhstan, China, Mongolia and North Korea. It shares maritime borders with Japan by the Sea of Okhotsk and the U.S. state of Alaska across the Bering Strait. The East Slavs emerged as a recognizable group in Europe between the 3rd and 8th centuries AD. Founded and ruled by a Varangian warrior elite and their descendants, the medieval state of Rus arose in the 9th century. In 988 it adopted Orthodox Christianity from the Byzantine Empire, beginning the synthesis of Byzantine and Slavic cultures that defined Russian culture for the next millennium. Rus' ultimately disintegrated into a number of smaller states; most of the Rus' lands were overrun by the Mongol invasion and became tributaries of the nomadic Golden Horde in the 13th century. The Grand Duchy of Moscow gradually reunified the surrounding Russian principalities, achieved independence from the Golden Horde. By the 18th century, the nation had greatly expanded through conquest, annexation, and exploration to become the Russian Empire, which was the third largest empire in history, stretching from Poland on the west to Alaska on the east. Following the Russian Revolution, the Russian Soviet Federative Socialist Republic became the largest and leading constituent of the Union of Soviet Socialist Republics, the world's first constitutionally socialist state. The Soviet Union played a decisive role in the Allied victory in World War II, and emerged as a recognized superpower and rival to the United States during the Cold War. The Soviet era saw some of the most significant technological achievements of the 20th century, including the world's first human-made satellite and the launching of the first humans in space. By the end of 1990, the Soviet Union had the world's second largest economy, largest standing military in the world and the largest stockpile of weapons of mass destruction. Following the dissolution of the Soviet Union in 1991, twelve independent republics emerged from the USSR: Russia, Ukraine, Belarus, Kazakhstan, Uzbekistan, Armenia, Azerbaijan, Georgia, Kyrgyzstan, Moldova, Tajikistan, Turkmenistan and the Baltic states regained independence: Estonia, Latvia, Lithuania; the Russian SFSR reconstituted itself as the Russian Federation and is recognized as the continuing legal personality and a successor of the Soviet Union. It is governed as a federal semi-presidential republic. The Russian economy ranks as the twelfth largest by nominal GDP and sixth largest by purchasing power parity in 2015. Russia's extensive mineral and energy resources are the largest such reserves in the world, making it one of the leading producers of oil and natural gas globally. The country is one of the five recognized nuclear weapons states and possesses the largest stockpile of weapons of mass destruction. Russia is a great power as well as a regional power and has been characterised as a potential superpower. It is a permanent member of the United Nations Security Council and an active global partner of ASEAN, as well as a member of the G20, the Shanghai Cooperation Organisation (SCO), the Council of Europe, the Asia-Pacific Economic Cooperation (APEC), the Organization for Security and Co-operation in Europe (OSCE), and the World Trade Organization (WTO), as well as being the leading member of the Commonwealth of Independent States (CIS), the Collective Security Treaty Organization (CSTO) and one of the five members of the Eurasian Economic Union (EEU), along with Armenia, Belarus, Kazakhstan and Kyrgyzstan.

New!!: Very-long-baseline interferometry and Russia · See more »

Salyut 6

Salyut 6 (Салют-6; lit. Salute 6), DOS-5, was a Soviet orbital space station, the eighth flown as part of the Salyut programme.

New!!: Very-long-baseline interferometry and Salyut 6 · See more »

Solar System

The Solar SystemCapitalization of the name varies.

New!!: Very-long-baseline interferometry and Solar System · See more »

South Korea

South Korea, officially the Republic of Korea (대한민국; Hanja: 大韓民國; Daehan Minguk,; lit. "The Great Country of the Han People"), is a country in East Asia, constituting the southern part of the Korean Peninsula and lying east to the Asian mainland.

New!!: Very-long-baseline interferometry and South Korea · See more »

Speed of gravity

In classical theories of gravitation, the changes in a gravitational field propagate.

New!!: Very-long-baseline interferometry and Speed of gravity · See more »

Spektr-R

Spektr-R (or RadioAstron) is a Russian scientific satellite with a radio telescope on board.

New!!: Very-long-baseline interferometry and Spektr-R · See more »

Sun

The Sun is the star at the center of the Solar System.

New!!: Very-long-baseline interferometry and Sun · See more »

Supermassive black hole

A supermassive black hole (SMBH or SBH) is the largest type of black hole, on the order of hundreds of thousands to billions of solar masses, and is found in the centre of almost all currently known massive galaxies.

New!!: Very-long-baseline interferometry and Supermassive black hole · See more »

Titan (moon)

Titan is the largest moon of Saturn.

New!!: Very-long-baseline interferometry and Titan (moon) · See more »

Transmission line

In communications and electronic engineering, a transmission line is a specialized cable or other structure designed to conduct alternating current of radio frequency, that is, currents with a frequency high enough that their wave nature must be taken into account.

New!!: Very-long-baseline interferometry and Transmission line · See more »

United States

The United States of America (USA), commonly known as the United States (U.S.) or America, is a federal republic composed of 50 states, a federal district, five major self-governing territories, and various possessions.

New!!: Very-long-baseline interferometry and United States · See more »

Very Long Baseline Array

The Very Long Baseline Array (VLBA) is a system of ten radio telescopes which are operated remotely from their Array Operations Center located in Socorro, New Mexico, as a part of the (LBO).

New!!: Very-long-baseline interferometry and Very Long Baseline Array · See more »

Very-long-baseline interferometry

Very-long-baseline interferometry (VLBI) is a type of astronomical interferometry used in radio astronomy.

New!!: Very-long-baseline interferometry and Very-long-baseline interferometry · See more »

Waveguide

A waveguide is a structure that guides waves, such as electromagnetic waves or sound, with minimal loss of energy by restricting expansion to one dimension or two.

New!!: Very-long-baseline interferometry and Waveguide · See more »

Redirects here:

E-VLBI, EVLBI, International VLBI Service for Geodesy and Astrometry, Long-baseline interferometry, VLBI, Very Long Baseline Interferometry, Very long baseline interferometry.

References

[1] https://en.wikipedia.org/wiki/Very-long-baseline_interferometry

OutgoingIncoming
Hey! We are on Facebook now! »