scholarly journals Slavic Swimming Championships in the Years 1927–1929

2021 ◽  
Vol 4 (1) ◽  
pp. 33-54
Author(s):  
Petra Tomšová
Keyword(s):  

In Czechoslovak swimming circles, swimming clubs were often criticized for having active sports contacts with many countries, especially Germany, Austria, Hungary, France, Sweden, England, but completely forgot about Slavic nations such as Poland and Yugoslavia. The reason could be found mainly in the fact that swimming in the Slavic countries developed only after the war. There were also financial reasons and greater distances between the states. After the successful European Championships in Budapest in 1926, when it turned out that the swimmers of the Slavic nations were able to compete in Europe, the International Secretary of ČSAPS, Eng. Hauptmann proposed to the South Slavic and Polish Swimming Associations to hold the swimmers’ championships of these nations. The proposal was adopted unanimously with great enthusiasm. This resulted in a convention, signed by the leading officials of the Yugoslavian, Polish and Czechoslovak Associations, in which all participating associations undertook to host the Slavic Championships in three consecutive years: in 1927 in Belgrade, Yugoslavia, in 1928 in Prague, Czechoslovakia, and 1929 in Warsaw, Poland. According to this convention, the Slavonic Championships were held with a full Olympic program according to the FINA regulations.

1962 ◽  
Vol 24 (2) ◽  
pp. 303-322 ◽  
Author(s):  
Bernard Cosman
Keyword(s):  

2000 ◽  
Vol 179 ◽  
pp. 201-204
Author(s):  
Vojtech Rušin ◽  
Milan Minarovjech ◽  
Milan Rybanský

AbstractLong-term cyclic variations in the distribution of prominences and intensities of green (530.3 nm) and red (637.4 nm) coronal emission lines over solar cycles 18–23 are presented. Polar prominence branches will reach the poles at different epochs in cycle 23: the north branch at the beginning in 2002 and the south branch a year later (2003), respectively. The local maxima of intensities in the green line show both poleward- and equatorward-migrating branches. The poleward branches will reach the poles around cycle maxima like prominences, while the equatorward branches show a duration of 18 years and will end in cycle minima (2007). The red corona shows mostly equatorward branches. The possibility that these branches begin to develop at high latitudes in the preceding cycles cannot be excluded.


Author(s):  
Hans M. Bolli ◽  
J. P. Beckmann ◽  
J. B. Saunders

2014 ◽  
Author(s):  
John Narborough ◽  
Abel Tasman ◽  
John Wood ◽  
Friderich Martens
Keyword(s):  

Sign in / Sign up

Export Citation Format

Share Document