scholarly journals Association between Catalase Gene (CAT-262 C/T) Polymorphism and Preeclampsia in the South of Iran

2020 ◽  
Vol 28 (2) ◽  
pp. 11-20
Author(s):  
Marzieh Alipour ◽  
Sirous Naeimi ◽  
Mohammad Mahdi Moghanibashi ◽  
khalil Khasheivarnamkhasti ◽  
Zeynab Mahmmodian ◽  
...  
Keyword(s):  
2014 ◽  
Vol 2014 ◽  
pp. 1-4 ◽  
Author(s):  
A. Lourdhu Mary ◽  
K. Nithya ◽  
W. Isabel ◽  
T. Angeline

Catalase, an endogenous antioxidant enzyme, is responsible for regulating reactive species levels. Several epidemiologic studies have suggested that single nucleotide polymorphism in catalase gene may be associated with many diseases. The genotype of CAT (-21 A/T) point mutation in promoter region of catalase gene was determined by polymerase chain based restriction fragment length polymorphism analysis in the DNA of 100 healthy volunteers. The frequency of CAT (-21 A/T) gene polymorphism AA, AT, and TT genotypes was found to be 7, 23, and 70 percent, respectively. The mutant “T” allele frequency was found to be 0.82 among the south Indian (Tamil) population. Chi square analysis showed that the study population lies within the Hardy-Weinberg equilibrium. The wild type genotype (AA) was found to be very low (7%) and the mutant genotype (AT/TT) was found to be more prevalent (93%) among the south Indian population. This suggests that the high prevalence of mutant genotype may increase the susceptibility to oxidative stress associated diseases.


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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