Simulating the Interaction of a Non-magnetized Planet with the Stellar Wind Produced by a Sun-like Star Using the FLASH Code-Reference-Cited by-同舟云学术

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Simulating the Interaction of a Non-magnetized Planet with the Stellar Wind Produced by a Sun-like Star Using the FLASH Code

Published:2019-07-10 Issue:5 Volume:49 Page:678-692
ISSN:0103-9733
Container-title:Brazilian Journal of Physics
language:en
Short-container-title:Braz J Phys

Author:

Evangelista Edgard F. D.^ORCID,Miranda Oswaldo D.,Mendes Odim,Domingues Margarete O.

Funder

Conselho Nacional de Desenvolvimento Científico e Tecnológico

Financiadora de Estudos e Projetos

Fundação de Amparo à Pesquisa do Estado de São Paulo

Publisher

Springer Science and Business Media LLC

Subject

General Physics and Astronomy

Link

http://link.springer.com/content/pdf/10.1007/s13538-019-00689-y.pdf

Reference33 articles.

1. T. Takahashi, H. Ueki, A. Kunimatsu, H. Fujii, in . ACM SIGGRAPH 2002 conference abstracts and applications. https://doi.org/10.1145/1242073.1242279 (ACM, New York, 2002), p. 266

2. N. Takashi, T. J. R. Hughes, . Comput. Method. Appl. M. 95, 115–138 (1992). https://doi.org/10.1016/0045-7825(92)90085-X

3. K. G. Powell, P. L. Roe, T. J. Linde, T. I. Gombosi, D. L. De Zeeuw, . J. Comp. Phys. 154, 284–309 (1999). https://doi.org/10.1006/jcph.1999.6299

4. D. G. E. Grigoriadis, I. E. Sarris, S. C. Kassinos, . Comput. Fluids. 39, 345–258 (2010). https://doi.org/10.1016/j.compfluid.2009.09.012

5. C. P. Johnstone, et al., . Astron. Astrophys. 577, A122 (2015). https://doi.org/10.1051/0004-6361/201425134

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