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- W2005092503 abstract "Recent observations from the Voyager 1 spacecraft show that it is sampling the local interstellar medium (LISM). This is quite surprising because no realistic, steady-state model of the solar wind (SW) interaction with the LISM gives an inner heliosheath width as narrow as ∼30 AU. This includes models that assume a strong redistribution of the ion energy to the tails in the pickup ion distribution function. We show that the heliopause (HP), which separates the SW from the LISM, is not a smooth tangential discontinuity, but rather a surface subject to Rayleigh–Taylor-type instabilities which can result in LISM material penetration deep inside the SW. We also show that the HP flanks are always subject to a Kelvin–Helmholtz instability. The instabilities are considerably suppressed near the HP nose by the heliospheric magnetic field in steady-state models, but reveal themselves in the presence of solar cycle effects. We argue that Voyager 1 may be in one such instability region and is therefore observing plasma densities much higher than those in the pristine SW. These results may explain the early penetration of Voyager 1 into the LISM. They also show that there is a possibility that the spacecraft may start sampling the SW again before it finally leaves the heliosphere." @default.
- W2005092503 created "2016-06-24" @default.
- W2005092503 creator A5027629446 @default.
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- W2005092503 date "2014-02-18" @default.
- W2005092503 modified "2023-09-27" @default.
- W2005092503 title "<i>VOYAGER 1</i> NEAR THE HELIOPAUSE" @default.
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- W2005092503 doi "https://doi.org/10.1088/2041-8205/783/1/l16" @default.
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