Preliminary results of a study of mothers' opinions of children's radio programs.

1936 ◽  
Vol 20 (3) ◽  
pp. 416-419 ◽  
Author(s):  
H. P. Longstaff
1937 ◽  
Vol 21 (3) ◽  
pp. 265-279 ◽  
Author(s):  
H. P. Longstaff

1959 ◽  
Author(s):  
Marlene Sa'ad Nasrallah

1986 ◽  
Vol 41 (1) ◽  
pp. 27-29
Author(s):  
John Patrick

Making radio programs for children is very exciting. Writers, producers and actors can be bold and imaginative because the responses of the young audience are fresh and vital, hot yet deadened by a lengthy exposure to the format programs of adult commercial television. And the act of listening to good story programs on radio uses the imaginative resources of the listener to provide the visual element so that the experience becomes collaborative and intensely personal.


1936 ◽  
Vol 20 (2) ◽  
pp. 208-220 ◽  
Author(s):  
H. P. Longstaff

2016 ◽  
Vol 43 (1) ◽  
pp. 67-97
Author(s):  
Vladimir Somov ◽  
Daria Somova

This article examines the impact of children’s radio programs on the promotion of patriotism among young Soviet citizens during the 1930s. The authors employ archival materials, periodicals, and personal documents, and use a generational approach and methods of cognitive history to reach their conclusions. In addition, this article analyzes the content of children’s radio programs in the Soviet Union and their impact on the lives and mentality of young people in the prewar ussr.


1999 ◽  
Vol 173 ◽  
pp. 185-188
Author(s):  
Gy. Szabó ◽  
K. Sárneczky ◽  
L.L. Kiss

AbstractA widely used tool in studying quasi-monoperiodic processes is the O–C diagram. This paper deals with the application of this diagram in minor planet studies. The main difference between our approach and the classical O–C diagram is that we transform the epoch (=time) dependence into the geocentric longitude domain. We outline a rotation modelling using this modified O–C and illustrate the abilities with detailed error analysis. The primary assumption, that the monotonity and the shape of this diagram is (almost) independent of the geometry of the asteroids is discussed and tested. The monotonity enables an unambiguous distinction between the prograde and retrograde rotation, thus the four-fold (or in some cases the two-fold) ambiguities can be avoided. This turned out to be the main advantage of the O–C examination. As an extension to the theoretical work, we present some preliminary results on 1727 Mette based on new CCD observations.


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