MICROSTRUCTURE OF THE HELIOSPHERIC TERMINATION SHOCK: IMPLICATIONS FOR ENERGETIC NEUTRAL ATOM OBSERVATIONS

By Gary Zank, J. Heerikhuisen, N. Pogorelov, R. Burrows, David John McComas. 2010

157 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/c28b15c427d32d2c169c623eb616d1e5dc6e51ac

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In Astronomy and Astrophysics

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Citations in the corpus

• Introduction to special section on Origins and Properties of Kappa Distributions: Statistical Background and Properties of Kappa Distributions in Space Plasmas (2015, background): “…and magnetospheres of planetary moons such as Io [e.g., Moncuquet et al., 2002] and Enceladus [e.g., Jurac et al., 2002]; (iii) the outer heliosphere and the inner heliosheath, [e.g., Decker and Krimigis, 2003; Decker et al., 2005; Heerikhuisen et al., 2008; Zank et al., 2010; LIVADIOTIS ©2015.”
• THE VECTOR DIRECTION OF THE INTERSTELLAR MAGNETIC FIELD OUTSIDE THE HELIOSPHERE (2010, background): “1995) even before the interaction with the termination shock introduces further modifications (Zank et al. 2010).”