Zero outward flow velocity for plasma in a heliosheath transition layer

Details Zero outward flow velocity for plasma in a heliosheath transition layer Zero outward flow velocity for plasma in a heliosheath transition layer

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011natur.474..359k&link_type=abstract

Nature, Volume 474, Issue 7351, pp. 359-361 (2011).

Astronomy and Astrophysics

Astronomy

9

Scientific paper

Voyager 1 has been in the reservoir of energetic ions and electrons that constitutes the heliosheath since it crossed the solar wind termination shock on 16 December 2004 at a distance from the Sun of 94 astronomical units (1AU = 1.5×108km). It is now ~22AU past the termination shock crossing. The bulk velocity of the plasma in the radial-transverse plane has been determined using measurements of the anisotropy of the convected energetic ion distribution. Here we report that the radial component of the velocity has been decreasing almost linearly over the past three years, from ~70kms-1 to ~0kms-1, where it has remained for the past eight months. It now seems that Voyager 1 has entered a finite transition layer of zero-radial-velocity plasma flow, indicating that the spacecraft may be close to the heliopause, the border between the heliosheath and the interstellar plasma. The existence of a flow transition layer in the heliosheath contradicts current predictions--generally assumed by conceptual models--of a sharp discontinuity at the heliopause.

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