Possible physical properties of the flow in the vicinity of the heliopause

Author:

Baranov V.B.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference40 articles.

1. An axisymmetric magnetohydrodynamic model for the interaction of the solar wind with the local interstellar medium;Alexashov;Astron. Lett.,2000

2. Baranov, V.B. Possible effects of the interstellar magnetic field on the heliospheric structure and H-atom penetration to the solar system. In: Scherer, K., Fichtner, H., Fahr, H.-J., Marsch, E. (Eds.), The Outer Heliosphere: The Next Frontiers, COSPAR Colloquia Series, vol. II, Pergamon, pp. 99–108, 2000.

3. Baranov, V.B. Early concepts of the heliospheric interface: plasma. In: Izmodenov, V., Kallenbach, R. (Eds.), The Physics of the Heliospheric Boundaries, ISSI Scientific Report, No 5, ESA -ESTEC, Paris, pp. 27–44, 2006.

4. Kinetic-fluid perspective on modeling the heliospheric/interstellar medium interface;Baranov;Space Sci. Rev.,2008

5. Kinetic-hydrodynamic models of the solar wind interaction with the partially ionized supersonic flow of the local interstellar gas: predictions and interpretations of the experimental data;Baranov;Space Sci. Rev.,2009

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