Reiserecht – Literarisch

Frisch, Max

doi:10.1515/rra.2003.11.6.241b

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2004

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“…The interplanetary magnetic field in the upstream region has the form of an Archimedean spiral according to the Parker model [8]. The interstellar magnetic field is uniform with the vector B is that either lies in the ecliptic plane (case I: φ 0 AE ) or deviates from the ecliptic by an angle φ 40 AE 60 AE (case II) as suggested by [9], [10].…”

Section: Introductionmentioning

confidence: 99%

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Questions about effects of interplanetary and interstellar magnetic fields on the heliospheric interface

Ratkiewicz¹,

Grygorczuk²,

Ben‐Jaffel³

2004

AIP Conference Proceedings

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In this paper we discuss configurations of the heliospheric interface shaped by the influence of both the uniform interstellar and the interplanetary (Parker model -Archimedean spiral) magnetic fields in the presence of the neutral particles. Magnetic fields strongly affect the structure and the shape of the heliospheric interface, which becomes asymmetric for any configuration of the interstellar magnetic field (ISMF), for the case where the interplanetary magnetic field (IMF) is included. In particular, the interstellar magnetic field lines may merge with interplanetary magnetic field lines of opposite direction at the heliopause. This may possibly cause a reconnection of the magnetic field lines at the heliopause.

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Section: Introductionmentioning

confidence: 99%

“…Parameters at the inner (SW) and outer (LISM) boundaries ([12],[9],[10]) AE , α=0 AE -90 AE , ∆α 10 AE…”

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confidence: 99%