U.S. Army Special Forces Unconventional Warfare Doctrine: Engine of Change or Relic of the Past?

2000 ◽  
Author(s):  
Robert E. Kelley
Author(s):  
Martin Bayer

For centuries, military uniforms had been colourful to differentiate friend from foe on the battlefield, but also as a distinguishing feature towards civil society. With technological progress and the advent of both aviation and improved photography a century ago, camouflage became a necessity. Artists and zoologists played a huge role in developing camouflage patterns. Today, most nations have a distinct national camouflage, and often, specific services or special forces have their very own uniforms as a sign of distinction. Nevertheless, many patterns can be traced back to the 1930s and 1940s. While fooling an observer is at the heart of military camouflage, it remains to be ambivalent, with its roles ranging from a desired cloak of invisibility to an indicator of power and prowess. In the past decades, camouflage has become synonymous with the military, and simultaneously, a global icon on its own, a political statement and an aspect of fashion.


1963 ◽  
Vol 15 (4) ◽  
pp. 636-646 ◽  
Author(s):  
Andrew C. Janos

The importance and political implications of the subject of unconventional warfare are well known and need not be elaborated upon here. At the present time, the three branches of the American military services are expanding their “special” forces, preparing for the eventuality of conflicts of smaller scope than conventional warfare. On the Soviet side, the theory of peaceful coexistence—i.e., the thesis that capitalism should be eliminated by popular movements rather than by foreign armies—was reasserted at the January conference of the S.E.D. in Berlin, by no lesser authority than Nikita Khrushchev himself.


1967 ◽  
Vol 31 ◽  
pp. 405
Author(s):  
F. J. Kerr

A continuum survey of the galactic-centre region has been carried out at Parkes at 20 cm wavelength over the areal11= 355° to 5°,b11= -3° to +3° (Kerr and Sinclair 1966, 1967). This is a larger region than has been covered in such surveys in the past. The observations were done as declination scans.


1962 ◽  
Vol 14 ◽  
pp. 133-148 ◽  
Author(s):  
Harold C. Urey

During the last 10 years, the writer has presented evidence indicating that the Moon was captured by the Earth and that the large collisions with its surface occurred within a surprisingly short period of time. These observations have been a continuous preoccupation during the past years and some explanation that seemed physically possible and reasonably probable has been sought.


1961 ◽  
Vol 2 (2) ◽  
pp. 73-105 ◽  
Author(s):  
John R. W. Small

It is generally accepted that history is an element of culture and the historian a member of society, thus, in Croce's aphorism, that the only true history is contemporary history. It follows from this that when there occur great changes in the contemporary scene, there must also be great changes in historiography, that the vision not merely of the present but also of the past must change.


1962 ◽  
Vol 11 (02) ◽  
pp. 137-143
Author(s):  
M. Schwarzschild

It is perhaps one of the most important characteristics of the past decade in astronomy that the evolution of some major classes of astronomical objects has become accessible to detailed research. The theory of the evolution of individual stars has developed into a substantial body of quantitative investigations. The evolution of galaxies, particularly of our own, has clearly become a subject for serious research. Even the history of the solar system, this close-by intriguing puzzle, may soon make the transition from being a subject of speculation to being a subject of detailed study in view of the fast flow of new data obtained with new techniques, including space-craft.


1979 ◽  
Vol 46 ◽  
pp. 96-101
Author(s):  
J.A. Graham

During the past several years, a systematic search for novae in the Magellanic Clouds has been carried out at Cerro Tololo Inter-American Observatory. The Curtis Schmidt telescope, on loan to CTIO from the University of Michigan is used to obtain plates every two weeks during the observing season. An objective prism is used on the telescope. This provides additional low-dispersion spectroscopic information when a nova is discovered. The plates cover an area of 5°x5°. One plate is sufficient to cover the Small Magellanic Cloud and four are taken of the Large Magellanic Cloud with an overlap so that the central bar is included on each plate. The methods used in the search have been described by Graham and Araya (1971). In the CTIO survey, 8 novae have been discovered in the Large Cloud but none in the Small Cloud. The survey was not carried out in 1974 or 1976. During 1974, one nova was discovered in the Small Cloud by MacConnell and Sanduleak (1974).


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