An oblique pulsar magnetosphere with a plasma conductivity
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/461/1/1068/13486766/stw1379.pdf
Reference41 articles.
1. Dissipation, energy transfer, and spin-down luminosity in 2.5D PIC simulations of the pulsar magnetosphere
2. Blandford R. D. Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology. Gilfanov M. Sunyaev R. Churazov E. , editors. Springer-Verlag; Berlin; 2002. p. 381.
3. Two Comments on Filtering (Artificial Viscosity) for Chebyshev and Legendre Spectral and Spectral Element Methods: Preserving Boundary Conditions and Interpretation of the Filter as a Diffusion
4. TESTING DISSIPATIVE MAGNETOSPHERE MODEL LIGHT CURVES AND SPECTRA WITHFERMIPULSARS
5. Canuto C. Hussaini M. Quarteroni A. Zang T. Spectral Methods: Fundamentals in Single Domains. Springer-Verlag; Berlin; 2006.
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