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- W1635014169 abstract "Interstellar material around the Sun is typical for our neighborhood of the Galaxy. The physical properties and kinematics of the partially ionized interstellar material (ISM) near the Sun are typical of warm diffuse clouds in the solar vicinity. The direction of the interstellar magnetic field at the heliosphere, the polarization of light from nearby stars, and the kinematics of nearby clouds are naturally explained in terms of the S1 superbubble shell. The interstellar radiation field at the Sun appears to be harder than the field ionizing ambient diffuse gas, which may be a consequence of the low opacity of the tiny cloud surrounding the heliosphere." @default.
- W1635014169 created "2016-06-24" @default.
- W1635014169 creator A5064620659 @default.
- W1635014169 date "2008-01-01" @default.
- W1635014169 modified "2023-09-25" @default.
- W1635014169 title "Is the Sun Embedded in a Typical Interstellar Cloud?" @default.
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- W1635014169 doi "https://doi.org/10.1007/978-1-4419-0247-4_15" @default.
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