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Modeling for performance analysis of electromagnetic zero-sequence suppressor
(2010-12-30)
The purpose of this work is to present a frequency domain model to demonstrate the operation of an electromagnetic arrangement for controlling the injection of zero-sequence currents in the electrical system. Considering ...
ConvolutionTR: comprehensive study of SNPs within tandem repeats.
(In: INTERNATIONAL PLANT & ANIMAL GENOME, 20., 2012, San Diego. Abstract... Jersey City: Scherago International, 2012., 2012)
Dynamic sequence evolution of a sex-Associated b chromosome in lake Malawi cichlid fish
(2017-01-01)
B chromosomes are extra chromosomes found in many species of plants, animals, and fungi. B chromosomes often manipulate common cellular processes to increase their frequency, sometimes to the detriment of organismal fitness. ...
Single nucleotide variations in the buffalo kappa-casein gene (CSN3)
(2013-12-01)
Caseins are the major milk proteins associated with lactation performance, milk composition and cheese yield efficiency, representing around 80% of the total amount of proteins found in milk. Among the caseins, kappa-casein ...
Experimental analysis of an electromagnetic zero-sequence suppressor
(2012-11-01)
The intent of this paper is to present contributions focused on the analysis and development of harmonic attenuator devices. Among these, highlights here the so-called electromagnetic zero-sequence suppressor. This arrangement ...
Sequencing And Identification Of Different Salmonella Species In Cocoa Beans Treated With Gamma Irradiation
(Elsevier Science BVAmsterdam, 2016)
Kinematic distances of pre-main-sequence stars in the Lupus star-forming region
(International Astronomical UnionBeijing, 2012)
To reliably determine the main physical parameters (masses and ages) of young stars, we must know their distances. While the average distance to nearby star-forming regions (<300 pc) is often known, the distances to ...
Kinematic distances of pre-main-sequence stars in the Lupus star-forming region
(International Astronomical UnionBeijing, 2012)
To reliably determine the main physical parameters (masses and ages) of young stars, we must know their distances. While the average distance to nearby star-forming regions (<300 pc) is often known, the distances to ...