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The heliopause is the boundary separating the predominantly solar-wind plasma of the heliosphere from the surrounding interstellar plasma. It is set by the interaction of flows, magnetic fields and pressure, rather than by a fixed spherical surface. It differs from the termination shock, where the solar wind slows abruptly inside the heliosphere.

Voyager 1 supplied a direct test. Plasma-wave oscillations observed in 2013 indicated a much greater local electron density, supporting a retrospective crossing in August 2012. Because the characteristic plasma frequency depends on the square root of electron density, the observed oscillation frequency served as a density diagnostic.^[ref]

The heliosheath, usually meaning the inner heliosheath, is the region of shocked solar wind between the termination shock and the heliopause. Solar wind plasma entering it has been slowed and compressed, and its flow turns as it approaches the boundary with the interstellar medium. The termination shock and heliopause are different boundaries: crossing the shock does not yet mean leaving solar-wind material.

The Voyager 2 plasma experiment provided direct measurements around several shock crossings between 30 August and 1 September 2007. The observed thermal plasma was cooler than a simple picture of complete conversion of the incoming flow energy into thermal-ion heat would suggest. The researchers inferred that much of the energy instead went into pickup ions or other energetic particles.^[ref]

The instrument used four Faraday cups, three facing approximately into the flow. Currents recorded at different particle energies and viewing directions were fitted with moving Maxwell-Boltzmann velocity distributions to estimate proton temperatures. This measures a selected part of the particle population; it does not directly measure all the energetic ions that may carry the remaining energy.^[ref]

The heliosphere is the region of space dominated by the solar-wind plasma and its carried magnetic field as they interact with the interstellar medium. The solar wind slows at the termination shock and encounters the interstellar plasma at the heliopause.

This is a plasma-interaction boundary, not the outer reach of the Sun's gravity or light. Voyager observations combine particle, magnetic-field and plasma-wave measurements to diagnose the transition. An increased local electron density outside the heliopause supplied an important independent diagnostic, illustrating why a boundary cannot always be identified from one field direction alone.^[ref]

John D. Richardson studies space plasmas, including the solar wind and its interaction with the interstellar medium. MIT identifies him as a principal investigator of the Voyager plasma experiment and describes earlier work on plasma transport in planetary magnetospheres.^[ref]

His 2008 Voyager 2 study analyzed plasma measurements across the termination shock. The thermal ions were cooler than a simple picture of bulk-flow energy becoming thermal-ion heat would suggest. The result made the partition of energy among particle populations central to understanding the shock.^[ref]

The experiment illustrates how a remote boundary becomes a local measurement. Four Faraday cups sampled particle currents over energy-per-charge ranges; combining differently oriented detectors allowed the team to infer plasma density, flow and temperature. These inferred properties depend on the measured spectra and distribution model, rather than being direct readings of a thermometer.^[ref]

The termination shock is the transition where the expanding solar wind slows from supersonic flow into the slower, compressed and heated flow of the outer heliosphere. It forms because the outward flow encounters pressure from its surroundings. It is distinct from the farther-out heliopause, where solar-wind plasma meets the interstellar plasma.

A shock wave converts organized flow kinetic energy into thermal and nonthermal particle energy. A spacecraft can therefore identify a crossing through changes in the magnetic field, plasma and energetic-particle populations, rather than through a visible solid boundary. Voyager 1 crossed the termination shock on 16 December 2004 near 94 astronomical units from the Sun. Its magnetic-field and particle instruments supplied evidence for entering the heliosheath.^[ref] The original particle report found enhanced low-energy protons but no local maximum of anomalous cosmic ray helium, illustrating why detecting a shock and explaining all particle acceleration are separate questions.^[ref]