Radio-astronomy, Radiometry and Infra-red Techniques

1961 ◽  
Vol 14 (1) ◽  
pp. 14-21 ◽  
Author(s):  
C. M. Cade

The year 1932 was one which had no great apparent significance for navigators, and yet it saw the commencement of two new lines of research which today, after an interval of more than a quarter-of-a-century, promise important contributions to the safety of navigators both at sea and in the air.The two lines of research were superficially quite unrelated, but fundamentally they relied upon the same principle—the detection of radiant energy emitted by objects solely as a result of their temperature. The first of these small beginnings was the discovery by K. G. Jansky that radio waves could be detected from extra-terrestrial sources: the second was the commencement by the U.S. Signal Corps Engineering Laboratories of an intensive study of infra-red devices with the object of obtaining night vision without illumination of the field of view.From Jansky's discovery has sprung the whole science of radio astronomy, which has revolutionized our ideas about the universe, and brought in its wake, as one practical benefit, the radio sextant. From the work of the U.S. Signal Corps there resulted a number of very useful infra-red components, including the pneumatic detector, better known as the Golay cell.

Although nearly all the major advances in radio astronomy have taken place during the last fifteen years the basic discoveries were made 30 years ago. At that time Jansky realized that the residual noise in his receiving equipment had a daily sidereal variation and must be the result of radio waves reaching the earth from outer space, and Appleton in the U. K. with Breit and Tuve in America through their studies of the ionosphere laid the foundation of the radio echo techniques of radio astronomy. The radio emission from outer space can be received on earth in the wavelength range from a few millimetres to 10 or 20 metres. The short wave end is limited by absorption in the atmosphere and the long wave end by the ionosphere, and this upper limit tends to vary in sympathy with ionospheric conditions throughout the sunspot cycle. These hindrances will soon be overcome when suitable equipment can be carried in earth satellites; then it should be possible to determine the true wavelength range of these extraterrestrial emissions.


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.


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.


1988 ◽  
Author(s):  
Kathy Roe Coker ◽  
Carol E. Rios
Keyword(s):  

Author(s):  
Geoff Cottrell

The atmosphere influences much of what can be seen through a telescope. Most of the atmosphere lies within 16 km from the Earth’s surface. Further out, the air becomes thinner until it merges with outer space. In the ionosphere—a layer 75–1000 km high—neutral atoms are ionized by solar radiation and high-energy cosmic ray particles arriving from distant parts of the Universe. ‘Windows in the sky’ explains electromagnetic radiation and the electromagnetic spectrum from gamma rays through to visible light and radio waves. Electromagnetic waves are transverse waves that can be polarized. The atmosphere acts as a filter and blocks cosmic electromagnetic radiation. Atmospheric turbulence distorts starlight resulting in ‘twinkling’ stars.


Author(s):  
Arthur M. Diamond

Cognitively diverse project entrepreneurs are the ones most likely to succeed at making a ding in the universe. Project entrepreneurs are more effective because they are more likely to persevere at achieving their project and at undertaking new breakthrough innovations. Cyrus Field, Marconi, Walt Disney, Sam Walton, and Steve Jobs were project entrepreneurs. Innovative entrepreneurs are likely to either know less theory, or to take theory less seriously, which allows them to try what theory says is impossible. For instance, the physics of Marconi’s day said that his radio waves should go straight into space rather than curve with the earth to cross the Atlantic. Conversely, innovative entrepreneurs often have more tacit knowledge. Innovative entrepreneurs pursue serendipitous observations or slow hunches, often through trial-and-error experiments, and may benefit from cognitive diversity, such as dyslexia and Asperger’s syndrome. What inventors and entrepreneurs know is the subject matter of the epistemology of innovation.


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