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- W1514157465 abstract "By analogy with the case of planetary magnetospheres it is argued that magnetic field reconnection processes may play an important role for the plasma mixing at the heliopause /1/. Views of the front side heliopause and different areas, where reconnection can take place, are provided for various assumed orientations of the magnetic field of the LISM. Within these reconnection patches the lines of constant angle between the magnetic field of the unperturbed solar wind (standard Parker's spiral field) and the (uniform) LISM field, both projected onto the heliopause surface, are computed. Low frequency (2-3 kHz) interplanetary radio emissions detected by Voyager mission and implications of possible observations of the heliospheric boundary are discussed." @default.
- W1514157465 created "2016-06-24" @default.
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- W1514157465 date "1990-01-01" @default.
- W1514157465 modified "2023-10-18" @default.
- W1514157465 title "Reconnection Pattern at the Heliopause" @default.
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- W1514157465 doi "https://doi.org/10.1016/b978-0-08-040780-7.50069-5" @default.
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