7. The radio sky

Author(s):  
Geoff Cottrell

‘The radio sky’ considers radio telescopes that can see much longer wavelengths. Cosmic radio waves were first discovered in 1932 by Karl Jansky, with the first radio telescope built in 1937. Technology for radar systems advanced during World War II and then after the war scientists, such as Bernard Lovell and Martin Ryle, made use of the advances in electronics, radio technology, and digital computers, to found radio astronomy. Single-dish antennas—including the Lovell Telescope at Jodrell Bank Observatory—continue to play important roles. To improve angular resolution two antennas need to be operated as an interferometer. These are described along with the discovery of quasars, supermassive black holes, pulsars, and neutron stars.

Bernard Lovell, Astronomer by chance . London: Macmillan, 1991. Pp. 380, £18.99. ISBN 0-333-55195-8 In his Story of Jodrell Bank and Out of the zenith Sir Bernard Lovell has already told us in impressive detail how he fostered the new science of radio astronomy and, against fearful odds, built the 250 foot radio telescope now called the Lovell telescope. In his forthcoming Echoes of war we are promised an account of the development of the H 2 S radar system on which he worked during World War II. For those of us who are not prepared to plough through these specialized books I recommend Astronomer by chance ; not only does it cover the interesting stories of Jodrell Bank and the development of H 2 S but it tells us more about the man behind them.


Author(s):  
B. Lovell

The cavity magnetron was invented in Birmingham University and developed by the GEC for centimetric radar in World War II. Its existence was kept secret, and its deployment was delayed, in the belief that as soon as it was used the enemy would be able to adopt the technique both in radar and in countermeasures. The H 2 S radar using the cavity magnetron was first used in January 1943, and a Stirling bomber with H 2 S crashed a few nights later near Rotterdam. The radar equipment was recovered almost intact by Telefunken engineers. The author of a German report on the equipment, Otto Hachenberg, subsequently became a colleague of the present author in radio astronomy. He died in 2001 and his report of May 1943 was discovered among his papers. It reveals that the principle of the cavity magnetron was already well known in Germany, based on work published in Leningrad in 1936. The most serious effect of the delay in deployment of the magnetron in centimetric radar was in the anti–U–boat campaign, in which the new centimetric radar became the main contributor to the successful end of the Battle of the Atlantic.


Author(s):  
Sherry Johnson

The Caribbean’s most emblematic weather symbol is the hurricane, a large rotating storm that can bring destructive winds, coastal and inland flooding, and torrential rain. A hurricane begins as a tropical depression, an area of low atmospheric pressure that produces clouds and thunderstorms. Hurricane season in the Caribbean runs from June 1 through November 30, although there have been infrequent storms that formed outside these dates. Hurricanes are classified according to their maximum wind speed, and when a tropical system reaches the wind speed of a tropical storm (35 mph), it is given a name. Lists of names, which are rotated periodically, are specific to certain regions. If a named storm is responsible for causing a significant number of deaths or property damage, the name is retired and replaced with another. Most deaths in a storm came from drowning, from storm surge along the coast or from flooding or mudslides in the interior. Storm-related deaths also occur when structures collapse or when victims are struck by flying debris. One important and underestimated cause of death after the passage of a storm is disease. Even if the destruction is not immediate, the passage of a hurricane can leave significant ecological damage along the coast and in the interior. Hurricanes can have a devastating effect on a community that takes a direct hit. Repeated hurricane strikes can leave a sense of helplessness and hopelessness, “hurricane fatigue.” Conversely, survivors of a disaster are often left with a feeling of confidence that, since they have endured the effects of at least one deadly hurricane, they can do so again. Until the last half of the 18th century, meteorology remained primitive, but the Age of Enlightenment brought scientific and ideological advances. Major beneficiaries were royal navies whose navigation manuals and nautical charts became increasingly more accurate. In 1821, William C. Redfield established the circular nature of storms and their counterclockwise rotation, while other scientists showed how wind currents within the storms moved upward. Once the coiled structure of hurricanes were established by mid-century, the term “cyclone” was applied, based upon the Greek word for the coils of a snake. After the mid-19th century, scientists moved from information gathering to attempts to predict hurricane strikes. Technology, in the form of the telegraph, was a key component in creating a forecasting system aided by organizations such as the Colegio de Belén, in Havana, Cuba. Later in the century, governments worldwide created official observation networks in which weather reports were radiotelegraphed from ships at sea to stations on land. The 20th century experienced advances, such as the use of kites and balloons, and the introduction of weather reconnaissance aircraft during World War II. In April 1960, the first satellite was launched to observe weather patterns, and by the early 1980s, ocean buoys and sophisticated radar systems made forecasts increasingly more accurate.


Author(s):  
John W. Moffat

Civita criticized Einstein’s papers on gravitational waves: their energy momentum is frame dependent and therefore does not fit the covariance of Einstein’s gravity theory. Infeld and Rosen did not believe gravitational waves existed, and Einstein changed his mind on their existence repeatedly. Others did believe in them, such as Fock and Feynman. Weber constructed his “Weber bar” to detect gravitational waves, but when he claimed success, he was criticized. He then proposed using a Michelson-Morley type of interferometer with lasers to detect gravitational waves, as did Weiss. Merging black holes and neutron stars were proposed as detectable sources of gravitational waves. Taylor and Hulse, using the large Arecibo radio telescope, indirectly detected gravitational waves from inspiraling neutron stars. Primordial gravitational waves, still emanating from the Big Bang, were claimed to have been detected by BICEP2, but the waves were eventually shown to be a result of foreground dust.


Author(s):  
S.Ya. Braude ◽  
V.M. Kontorovich

The book tells about the achievements of modern radio astronomy. Data on radio galaxies, quasars, pulsars, space masers, and other space objects emitting radio waves are presented in a popular form. The ways of evolution of stars, supernovae and radio eruptions of their remains, the formation of white dwarfs and neutron stars, the phenomena in the centers of galaxies and the fusion of galaxies responsible for the formation of radio galaxies and quasars are considered. The radio radiation of the Sun and planets is discussed. A modern view of the evolution of the universe, the origin of the relic radiation left over from the Great Eruption, and its anisotropy is presented. A separate chapter is devoted to the description of radio telescopes.


Polar Record ◽  
1959 ◽  
Vol 9 (61) ◽  
pp. 320-330 ◽  
Author(s):  
Angus C. Hamilton

A geodetic survey by shoran trilateration, to approximately second-order accuracy, of the islands of the Canadian Arctic archipelago was completed in 1957. This was the culmination of a programme started in the south-central section of the country in 1949.Shoran (short-range aid to navigation) was developed during World War II as a navigational aid for precise tactical bombing. It consists of two radar transponders at known points on the ground and another radar unit in an aircraft capable of measuring the time required for radio waves to travel from the aircraft to each ground station and to return. These times are converted to distances by an intricate electro-mechanical system and the distances are shown on counters, reading to 0·001 mile. For the military application the distance between transponders was known and the position of the aircraft could be plotted from the mileage-counter distances; for geodetic application the mileage-counter distances are used to measure the distance between the two transponders.


2016 ◽  
Vol 62 ◽  
pp. 323-344
Author(s):  
Rodney D. Davies ◽  
Sir Francis Graham-Smith ◽  
Andrew G. Lyne

Bernard Lovell is remembered for the iconic radio telescope at Jodrell Bank that bears his name, and for the research group at the University of Manchester that has become the Jodrell Bank Centre for Astrophysics. His enthusiasm and warm personality inspired several generations of radio astronomers, many of whom now lead their own research groups. Lovell also played a key role in the development of airborne radar during World War II.


Unity Journal ◽  
2021 ◽  
Vol 2 ◽  
pp. 243-250
Author(s):  
Sirjana Pun

After the independent invention of radar in the early 1930s, the development of radar went rapidly during World War II (1939-1945) when both Axis and Allied forces relied on the system to get an edge over the other. Ever since the war, radar technology has substantially increased in its innovation and capability throughout the years. This paper examines the progress of radar technology following World War II (1939-1945) with an aim to provide a landscape of the prevalent radar system during the war which was mono-pulse tracking radar systems and moving-target indication (MTI) system. After a thorough background study of the past radar system, the paper highlights application of the newer developed Phased Array Radar System which was formulated out through the implementation of the improved capabilities of both prevalent systems. Moreover, the paper provides a brief overview of the modular system and formulates a time frame relating to the development of radar research. Thus, the paper, later on, foresees the prominent future where phased array systems could be expanded to civilian and non-civilian technological research by providing thorough research and comparative analysis. Phased array systems are found to a prominent possible cheaper alternative for the civilian and non-civilian system. It shows prominence to be an effective useful tool for radar systems.


2004 ◽  
Vol 21 (1) ◽  
pp. 23-71 ◽  
Author(s):  
Wayne Orchiston

AbstractOwen Bruce Slee is one of the pioneers of Australian radio astronomy. During World War II he independently discovered solar radio emission, and, after joining the CSIRO Division of Radiophysics, used a succession of increasingly more sophisticated radio telescopes to examine an amazing variety of celestial objects and phenomena. These ranged from the solar corona and other targets in our solar system, to different types of stars and the ISM in our Galaxy, and beyond to distant galaxies and clusters of galaxies. Although long retired, Slee continues to carry out research, with emphasis on active stars and clusters of galaxies. A quiet and unassuming man, Slee has spent more than half a century making an important, wide-ranging contribution to astronomy, and his work deserves to be more widely known.


2002 ◽  
Vol 10 (2) ◽  
pp. 285-300 ◽  
Author(s):  
FRANCIS GRAHAM - SMITH

The special value of radio astronomy lies in the probing of extreme conditions in the universe, including the highest energies and the lowest temperatures. Radio waves can penetrate clouds of gas and dust to reveal objects in the universe and, in particular, in our Galaxy that cannot be seen by visible light. To achieve the highest resolution, radio telescopes in widely separate parts of our globe combine their reception to produce a synthesized image. This is a splendid example of international collaboration. Among the images visualized are pulsars, derived from the remnants of supernovae explosions, and quasar sources powered by black holes.


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