New Analytical Solution of the Equilibrium Ampere's Law Using the Walker's Method: a Didactic Example

被引:0
|
作者
Laurindo Sousa, A. N. [1 ,2 ]
Ojeda-Gonzalez, A. [2 ]
Prestes, A. [2 ]
Klausner, V. [2 ]
Carita, L. A. [2 ,3 ]
机构
[1] Univ Estadual Maranhao UEMA, Dept Math, CESBA, BR-65800000 Balsas, MA, Brazil
[2] Univ Vale Paraiba UNIVAP, Lab Phys & Astron, IP&D, BR-12244000 Sao Jose Dos Campos, SP, Brazil
[3] Inst Fed Educ Ciencia & Tecnol Sao Paulo IFSP, Dept Math, Campus Sao Jose dos Campos Petrobras IFSP, BR-12223201 Sao Jose Dos Campos, SP, Brazil
关键词
Kinetic and MHD theory; Current sheet model; Grad-Shafranov equation; Plasma sheet; GRAD-SHAFRANOV RECONSTRUCTION; MAGNETIC-FLUX TRANSFER; CARRYING PLASMA SHEET; TEARING INSTABILITY; RECONNECTION; MAGNETOPAUSE; MODEL;
D O I
10.1007/s13538-017-0542-8
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
This work aims to demonstrate the analytical solution of the Grad-Shafranov (GS) equation or generalized Ampere's law, which is important in the studies of self-consistent 2.5-D solution for current sheet structures. A detailed mathematical development is presented to obtain the generating function as shown by Walker (RSPSA 91, 410, 1915). Therefore, we study the general solution of the GS equation in terms of the Walker's generating function in details without omitting any step. The Walker's generating function g(zeta) is written in a new way as the tangent of an unspecified function K(zeta). In this trend, the general solution of the GS equation is expressed as exp(- 2I<spacing diaeresis>) = 4|K (')(zeta)|(2)/cos(2)[K(zeta) - K(zeta (au))]. In order to investigate whether our proposal would simplify the mathematical effort to find new generating functions, we use Harris's solution as a test, in this case K(zeta) = arctan(exp(i zeta)). In summary, one of the article purposes is to present a review of the Harris's solution. In an attempt to find a simplified solution, we propose a new way to write the GS solution using g(zeta) = tan(K(zeta)). We also present a new analytical solution to the equilibrium Ampere's law using g(zeta) = cosh(b zeta), which includes a generalization of the Harris model and presents isolated magnetic islands.
引用
收藏
页码:67 / 73
页数:7
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