A Computational Review of The Solar Wind in Oblate Spheroidal Coordinates Perspective

The solar as theoretical is known not perfectly round. Many types of research have been trying to approach the states and properties of the solar. Complexities of these issues are very interesting to study and observe. In this paper presented the review of a solar wind that blows from its surface ba...

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Bibliographic Details
Published in:Journal of physics. Conference series 2017-03, Vol.820 (1), p.12019
Main Authors: Wibowo, F W, Wihayati
Format: Article
Language:English
Subjects:
Charged particles
Physics
Solar wind
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Summary:The solar as theoretical is known not perfectly round. Many types of research have been trying to approach the states and properties of the solar. Complexities of these issues are very interesting to study and observe. In this paper presented the review of a solar wind that blows from its surface based on Parker's model of solar wind that approached using continuity and momentum equations in the fluid. But in this case, the solar wind also approached in oblate spheroidal coordinates. This paper didn't describe the effect of the magnetic field and only calculated in the radial direction. The solar wind equation in oblate spheroidal coordinates has been observed in around the pole and equator. These approached equations have been solved computationally using parameters of G, M*, a and cs.
ISSN:1742-6588
1742-6596
DOI:10.1088/1742-6596/820/1/012019