4.8 Article

Structures and Spectral Variations of the Outer Heliosphere in IBEX Energetic Neutral Atom Maps

Journal

SCIENCE
Volume 326, Issue 5955, Pages 964-966

Publisher

AMER ASSOC ADVANCEMENT SCIENCE
DOI: 10.1126/science.1180927

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Funding

  1. NASA Explorer Program
  2. U. S. Department of Energy

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The Interstellar Boundary Explorer ( IBEX) has obtained all-sky images of energetic neutral atoms emitted from the heliosheath, located between the solar wind termination shock and the local interstellar medium (LISM). These flux maps reveal distinct nonthermal (0.2 to 6 kilo-electron volts) heliosheath proton populations with spectral signatures ordered predominantly by ecliptic latitude. The maps show a globally distributed population of termination-shock-heated protons and a superimposed ribbonlike feature that forms a circular arc in the sky centered on ecliptic coordinate (longitude lambda, latitude beta) = (221 degrees, 39 degrees), probably near the direction of the LISM magnetic field. Over the IBEX energy range, the ribbon's nonthermal ion pressure multiplied by its radial thickness is in the range of 70 to 100 picodynes per square centimeter AU ( AU, astronomical unit), which is significantly larger than the 30 to 60 picodynes per square centimeter AU of the globally distributed population.

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