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Voyager 1 in the Foreshock, Termination Shock, and Heliosheath
Science, 2005Voyager 1 (V1) began measuring precursor energetic ions and electrons from the heliospheric termination shock (TS) in July 2002. During the ensuing 2.5 years, average particle intensities rose as V1 penetrated deeper into the energetic particle foreshock of the TS.
R B, Decker +7 more
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Structure and properties of the termination shock
AIP Conference Proceedings, 2004Conventionally, the heliospheric termination shock (HTS) is regarded as a sharp MHD discontinuity. More recent models suggest that the back‐reaction of energetic cosmic rays accelerated at the HTS will create a broad shock with an extended precursor. Here we suggest that a combination of upstream solar wind disturbances interacting with the HTS, the ...
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Observations of the Termination Shock and Heliosheath
2010Voyagers 1 and 2 have both crossed the solar wind termination shock and are now in the heliosheath, the region of shocked solar wind plasma before the heliopause. This paper reviews observations of the termination foreshock, the termination shock (TS), and the heliosheath.
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Heat shock induces premature transcript termination and reconfigures the human transcriptome
Molecular Cell, 2022Richard Mitter +2 more
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Properties of the termination shock observed by Voyager 2
Geophysical Research Letters, 2008Hui Li, Chi Wang, J D Richardson
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An energetic‐particle‐mediated termination shock observed by Voyager 2
Geophysical Research Letters, 2009V Florinski, R B Decker, J A Le Roux
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