Metric Tensor Approach in Solar Wind for Rapidly Rotating Stellar

5th International Conference on Science & Engineering in Mathematics, Chemistry and Physics 2017

数学;化学;物理学

Wihayati^1 ; Wibowo, F.W.^2

Astrophysics and Mathematics Group, Sekip Utara Bulaksumur, Yogyakarta

55281, Indonesia^1

Department of Informatics Engineering, STMIK AMIKOM Yogyakarta, Jl. Ring Road Utara, Condong Catur, Depok, Sleman, Yogyakarta

55283, Indonesia^2

关键词: Co-ordinate system;    Metric tensor;    Oblate shape;    Oblateness;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/820/1/012034/pdf
DOI  :  10.1088/1742-6596/820/1/012034

来源: IOP

【 摘 要 】

Many researchers have observed the phenomena associated with the solar wind. One of which became a reference in this field is Parker's solar wind. The development of ideas initiated by Parker led to many cases related to Parker's solar wind. This paper aims at finding the metric tensor of the solar wind by using the idea of Parker's solar wind in rapidly rotating stellar. By the discovery of the metric tensor can be used to find the distance and characteristics of the coordinate system in approaching oblateness because a rapidly rotating stellar has an oblate shape at the poles.