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...Cannes Resolutions in 1922. This statement is as true today as when it was first uttered, and it applies with equal force to the Soviet Republic of Russia as it did to the Republic of France. But our State Department of today pursues a policy in direct contradiction, and in basing recognition upon the economic character of the government by prescribing that it shall be capitalistic, it is taking a ground which is untenable. It is assuming an attitude which is hardly justifiable...

Author: NO WRITER ATTRIBUTED | Title: ATTACKS U. S. RUSSIAN POLICY | 6/23/1922 | See Source »

...such an extent that Cleveland was elected to the slogan: "No North, no South, no East, no Cornwallis-West!" Propaganda, a very vague term, is quickly laid at the door of the foreign envoy, and public opinion like a Frankenstein turns without warning upon anyone who has tried to direct...

Author: NO WRITER ATTRIBUTED | Title: OBSERVING THE MIDDLE COURSE | 6/16/1922 | See Source »

...paying his taxes. All in all, from start to finish, it appears that a vindictive society is out to "get" any attempts to break away from its ranks. The deserter is labelled A. W. O. L. and his efforts, instead of meeting with appreciation, find only derision or direct and vigorous disapproval...

Author: NO WRITER ATTRIBUTED | Title: MACADAMIZING ADAM | 6/12/1922 | See Source »

What is even more interesting to us we are accustomed to accept with a shrug of the shoulders what "has always been that way" is the fact that tennis was a gambling game and was played extensively about the Mediterranean. (A direct offspring is still played in Cuba and Mexico as Jaialai). None of the modern equipment was necessary. The players knocked a ball with their hands over a mound of earth, or some such obstacle, and settled their debts on the spot. It is barely possible that desperate matches are played on the Jarvis courts for sodas...

Author: NO WRITER ATTRIBUTED | Title: 1, 2, 3! | 6/9/1922 | See Source »

...greatest problems that confronts astronomers at the present time is an accurate knowledge of the distances of stars. From the earliest times, the relative positions of stars or their apparent directions in space have been observed and measured with increasing accuracy. Before anything definite could be learned, however, as to the actual structure of the sidereal universe in which the earth plays its ultra-microscopic part, the actual distance to many of the brighter stars had to be measured. When Copernicus promulgated the heliocentric theory in 1543 through the publication of his epoch-making book. 'De Revolution-ibus Orbium Coelestium...

Author: By H. T. Stetson, | Title: ASTRONOMY NOW SOLVING STAR DISTANCE PROBLEMS BY RECENTLY DEVELOPED METHOD WITH GREAT FUTURE | 6/9/1922 | See Source »

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