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The behavior of electrons at the heliospheric shock transition

Astrophysics and Space Science, no. 10 (2019): 1-5

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Abstract

The jump of the temperature of thermal protons and the compression at the solar wind termination shock, measured by the Voyager 2 spacecraft during its crossing of the shock, can be explained if one assumes that the downstream temperature of electrons essentially higher than that of the thermal protons. The upstream temperature of the ele...More

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