Defying race ideology in the South

2020 ◽  
pp. 121-134
Author(s):  
Christie M. Kleinmann
Keyword(s):  
2018 ◽  
Vol 34 ◽  
pp. 207-226
Author(s):  
Alan I. Abramowitz

The southern party system has undergone a dramatic transformation since the 1960s, a transformation that has affected both the electoral bases of the parties and their leadership. This transformation has involved two related trends-a shift in the racial composition of the Democratic Party at the mass and elite levels and an ideological realignment that has produced a much wider gap between the ideological orientations and policy preferences of Democratic and Republican leaders and voters. In the South, to an even greater extent than in the rest of the nation, the Democratic Party has become increasingly dependent on the support of nonwhite voters. Meanwhile, despite the growing size of the nonwhite electorate in the South, the Republican base has remained overwhelmingly white. The growing dependence of the Democratic Party in the South on African-American and more recently Hispanic votes has contributed to the party's increasing liberalism because African-American and Hispanic voters tend to strongly support activist government. And this trend has also contributed to the growing conservatism of the Republican base as conservative whites have continued to flee the Democratic Party for the GOP. As a result, the two-party system in the South now consists of a Democratic Party dominated by nonwhites and white liberals and a Republican Party dominated by white conservatives.


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.


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

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