Density correlations between solar wind and pick-up ions with New Horizons/SWAP near 11 AU

Details Density correlations between solar wind and pick-up ions with New Horizons/SWAP near 11 AU Density correlations between solar wind and pick-up ions with New Horizons/SWAP near 11 AU

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aps..tsffm2007r&link_type=abstract

American Physical Society, Joint Fall 2010 Meeting of the Texas Sections of the APS, AAPT, Zone 13 of SPS and the National Socie

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Scientific paper

The Solar Wind Around Pluto (SWAP) instrument aboard the New Horizons spacecraft measured ion energy spectra of the solar wind and pick-up ions between 11 and 12 AU in late 2008. We report on detailed fitting of these spectra using an empirical model that includes major solar wind ions (H+, He2+, and O6+) as well as pick-up ions (from the interstellar and inner sources). We find a correlation between the densities of the solar wind H+ ions and all other populations. The two strongest correlations are with the interstellar pick-up ions and the inner source pick-up ions. These results could have implications for transport of pick-up ions through the heliosphere.

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