Cumulative Distribution Functions as Hysteresis Models

被引：0
作者：
DE Campos, M. F. [1 ]
DE Castro, J. A. [1 ]
机构：
[1] Fed Fluminense Univ UFF, Ave Trabalhadores 420, BR-27255125 Volta Redond, RJ, Brazil
来源：
ACTA PHYSICA POLONICA A | 2024年 / 146卷 / 01期
关键词：
hysteresis; Stoner Wohlfarth; magnetic Barkhausen noise (MBN);
D O I：
10.12693/APhysPolA.146.20
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The cumulative distribution functions can be used as the basis for hysteresis models. Here it is described how, using only 3 parameters, including one representing the shape, hysteresis curves can be constructed using symmetric distribution functions. The model is useful in the interpretation of magnetic Barkhausen noise data. The model also has a clear physical meaning because it represents the distribution of coercivity inside the sample. An isotropic Stoner-Wohlfarth hysteresis was partially modelled by a three-parameter cumulative distribution function of Gaussian hysteresis for the 1st and 3rd quadrants. Asymmetric distributions will provide better hysteresis adjustment, but these are four-parameter models.
引用
收藏
页码：20 / 25
页数：120
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