The Abundance of Atomic 1H, 4He and 3He in the Local Interstellar Cloud from Pickup Ion Observations with SWICS on Ulysses

Abstract

Pickup ions measured deep inside the heliosphere open a new way to determine the absolute atomic density of a number of elements and isotopes in the local interstellar cloud (LIC). We derive the atomic abundance of hydrogen and the two isotopes of helium from the velocity and spatial distributions of interstellar pickup protons and ionized helium measured with the Solar Wind Ion Composition Spectrometer (SWICS) on the Ulysses spacecraft between ~2 and ~5 AU. The atomic hydrogen density near the termination shock derived from interstellar pickup ion measurements is 0.115±0.025 cm-3, and the atomic H/He ratio from these observations is found to be 7.7 ± 1.3 in the outer heliosphere. Comparing this value with the standard universal H/He ratio of ~10 we conclude that filtration of hydrogen is small and that the ionization fraction of hydrogen in the LIC is low.KeywordsSolar WindTermination ShockPhase Space DensitySolar Wind ProtonOuter HeliosphereThese keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.