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Mauritius Radio Telescope
The Mauritius Radio Telescope (MRT) is a synthesis radio telescope in Mauritius that is used to make images of the sky at a frequency of 151.5 MHz. The MRT was primarily designed to make a survey with a point source sensitivity of 150 mJy. Its resolution is about 4 arc min.Astrophysical results of the Mauritius radio telescope ''IOP Conf. Series: Materials Science and Engineering'', 44 (2013). R. Somanah, N. Issur and N. Oozeer. Structure The MRT is a T-shaped array consisting of a 2048m-long East-West arm with 1024 fixed helical antennas arranged in 32 groups and an 880m-long North-South arm with 15 movable trolleys, each containing four antenn ...[...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Radio Telescope
A radio telescope is a specialized antenna and radio receiver used to detect radio waves from astronomical radio sources in the sky. Radio telescopes are the main observing instrument used in radio astronomy, which studies the radio frequency portion of the electromagnetic spectrum emitted by astronomical objects, just as optical telescopes are the main observing instrument used in traditional optical astronomy which studies the light wave portion of the spectrum coming from astronomical objects. Unlike optical telescopes, radio telescopes can be used in the daytime as well as at night. Since astronomical radio sources such as planets, stars, nebulas and galaxies are very far away, the radio waves coming from them are extremely weak, so radio telescopes require very large antennas to collect enough radio energy to study them, and extremely sensitive receiving equipment. Radio telescopes are typically large parabolic ("dish") antennas similar to those employed in tracking an ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Southern Celestial Hemisphere
The southern celestial hemisphere, also called the Southern Sky, is the southern half of the celestial sphere; that is, it lies south of the celestial equator. This arbitrary sphere, on which seemingly fixed stars form constellations, appears to rotate westward around a polar axis due to Earth's rotation. At any given time, the entire Southern Sky is visible from the geographic South Pole, while less of this hemisphere is visible the further north the observer is located. The northern counterpart is the northern celestial hemisphere. Astronomy In the context of astronomical discussions or writing about celestial mapping, it may also simply then be referred to as the Southern Hemisphere. For the purpose of celestial mapping, the sky is considered by astronomers as the inside of a sphere divided in two halves by the celestial equator. The Southern Sky or Southern Hemisphere is, therefore, that half of the celestial sphere that is south of the celestial equator. Even if ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Raman Research Institute
The Raman Research Institute (RRI) is an institute for scientific research located in Bangalore, India. It was founded by Nobel laureate C. V. Raman in 1948. Although it began as an institute privately owned by Sir C. V. Raman, it is now funded by the government of India. History Before Raman considered founding a research institute, he had approached the former Maharaja of Mysore seeking land to build office and conference premises for the Indian Academy of Sciences (IAS). The Maharaja acceded to Raman's request and a plot of land in the Malleshwaram suburb of Bangalore was allotted to the Indian Academy of Sciences in 1934. However, the Academy (then headed by Raman) made no use of the land for seven years. According to the terms of the deal with the Maharaja, the land could be to another use by the government of Mysore if it still remained unused at the end of 1941. Raman, as President of the IAS, held an extraordinary meeting of the academy in 1941, and proposed that a ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Indian Institute Of Astrophysics
The Indian Institute of Astrophysics (IIA), with its headquarters in Bengaluru,is an autonomous Research Institute wholly financed by the department of Science and Technology, Government of India. IIA conducts research primarily in the areas of astronomy, astrophysics and related fields. The institute has a network of laboratories and observatories in India, including Kodaikanal (the Kodaikanal Solar Observatory), Kavalur (the Vainu Bappu Observatory), Gauribidanur (the Gauribidanur Radio Observatory), Hanle (the Indian Astronomical Observatory) and Hosakote. IIA contributed to Astrosat, India's first dedicated multi-wavelength space observatory. The Astrosat project is a collaborative effort of many different research institutions from India. The institute led the development of Ultra-Violet Imaging Telescope (UVIT). Areas of research Researchers at IIA work on a diverse set of topics related to Astronomy and Astrophysics. However, the research can be broadly classified und ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
University Of Mauritius
The University of Mauritius (UoM) (french: Université de Maurice) is the national university of Mauritius. It is the oldest and largest university in the country in terms of student enrollment and curriculum offered. The public university's main campus is located at Réduit, Moka. History The University of Mauritius was officially established by the University of Mauritius Ordinance in December 1965, incorporating the existing School of Agriculture. In 1971, the University of Mauritius Act further defined the objects, powers, functions and structure of the university. On 24 March 1972, Her Majesty Queen Elizabeth II, accompanied by His Royal Highness the Duke of Edinburgh, inaugurated the University of Mauritius. The first chancellor of the university of Mauritius was Her Royal Highness the Princess Alexandra, the Honourable Lady Ogilvy. Organisation Faculty of Agriculture The Faculty of Agriculture is the oldest faculty of the university. It was founded in 1914 as th ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Steep Spectrum Radio Source
Steep may refer to: Arts and entertainment * ''Steep'' (2007 film), a film about extreme skiing * ''Steep'' (video game), a 2016 video game Places England * Steep, Hampshire, a village in central Hampshire, England * Steep Hill, a popular tourist street in the historic city of Lincoln, Lincolnshire, England * Steep Holm, an English island lying in the Bristol Channel Other places * Steep Island, Australia * Steep Island, Hong Kong * Steep Point, westernmost point of the Australian mainland * Mount Steep, Antarctica Science, technology, and mathematics * Slope, an elementary mathematical concept * Grade (slope), in civil engineering People with the surname * Frederick Steep (1874–1956), Canadian amateur football (soccer) player Other uses * Steeping, a cooking technique employing soaking * STEEP analysis, a variant of the PEST analysis In business analysis, PEST analysis ("political, economic, socio-cultural and technological") describes a framework of macro-enviro ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Supernova Remnant
A supernova remnant (SNR) is the structure resulting from the explosion of a star in a supernova. The supernova remnant is bounded by an expanding shock wave, and consists of ejected material expanding from the explosion, and the interstellar material it sweeps up and shocks along the way. There are two common routes to a supernova: either a massive star may run out of fuel, ceasing to generate fusion energy in its core, and collapsing inward under the force of its own gravity to form a neutron star or a black hole; or a white dwarf star may accrete material from a companion star until it reaches a critical mass and undergoes a thermonuclear explosion. In either case, the resulting supernova explosion expels much or all of the stellar material with velocities as much as 10% the speed of light (or approximately 30,000 km/s). These speeds are highly supersonic, so a strong shock wave forms ahead of the ejecta. That heats the upstream plasma up to temperatures well above mi ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Extra-galactic Radio Source
An astronomical radio source is an object in outer space that emits strong radio waves. Radio emission comes from a wide variety of sources. Such objects are among the most extreme and energetic physical processes in the universe. History In 1932, American physicist and radio engineer Karl Jansky detected radio waves coming from an unknown source in the center of our galaxy. Jansky was studying the origins of radio frequency interference for Bell Laboratories. He found "...a steady hiss type static of unknown origin", which eventually he concluded had an extraterrestrial origin. This was the first time that radio waves were detected from outer space. The first radio sky survey was conducted by Grote Reber and was completed in 1941. In the 1970s, some stars in our galaxy were found to be radio emitters, one of the strongest being the unique binary MWC 349. Sources: solar system The Sun As the nearest star, the Sun is the brightest radiation source in most frequencies, down to t ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Solar Radio Emission
Solar radio emission refers to radio waves that are naturally produced by the Sun, primarily from the lower and upper layers of the atmosphere called the chromosphere and Stellar corona, corona, respectively. The Sun produces radio emissions through four known mechanisms, each of which operates primarily by converting the energy of moving electrons into radiation. The four emission mechanisms are thermal bremsstrahlung (free-free) emission, gyromagnetic emission, plasma emission, and electron-cyclotron maser emission. The first two are ''incoherent'' mechanisms, which means that they are the summation of radiation generated independently by many individual particles. These mechanisms are primarily responsible for the persistent "background" emissions that slowly vary as structures in the atmosphere evolve. The latter two processes are ''coherent'' mechanisms, which refers to special cases where radiation is efficiently produced at a particular set of frequencies. Coherent mechanisms ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Galactic Plane
The galactic plane is the plane on which the majority of a disk-shaped galaxy's mass lies. The directions perpendicular to the galactic plane point to the galactic poles. In actual usage, the terms ''galactic plane'' and ''galactic poles'' usually refer specifically to the plane and poles of the Milky Way, in which Planet Earth is located. Some galaxies are irregular and do not have any well-defined disk. Even in the case of a barred spiral galaxy like the Milky Way, defining the galactic plane is slightly imprecise and arbitrary since the stars are not perfectly coplanar. In 1959, the IAU defined the position of the Milky Way's north galactic pole as exactly RA = , Dec = in the then-used B1950 epoch; in the currently-used J2000 epoch, after precession is taken into account, its position is RA , Dec . This position is in Coma Berenices, near the bright star Arcturus; likewise, the south galactic pole lies in the constellation Sculptor. The "zero of longitude" of galactic coor ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Pulsars
A pulsar (from ''pulsating radio source'') is a highly magnetized rotating neutron star that emits beams of electromagnetic radiation out of its magnetic poles. This radiation can be observed only when a beam of emission is pointing toward Earth (similar to the way a lighthouse can be seen only when the light is pointed in the direction of an observer), and is responsible for the pulsed appearance of emission. Neutron stars are very dense and have short, regular rotational periods. This produces a very precise interval between pulses that ranges from milliseconds to seconds for an individual pulsar. Pulsars are one of the candidates for the source of ultra-high-energy cosmic rays. (See also centrifugal mechanism of acceleration.) The periods of pulsars make them very useful tools for astronomers. Observations of a pulsar in a binary neutron star system were used to indirectly confirm the existence of gravitational radiation. The first extrasolar planets were discovered aroun ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
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