Abstract The Interstellar Mapping and Acceleration Probe (IMAP) is a revolutionary mission
that simultaneously investigates two of the most important overarching issues in …

The GAS-instrument onboard the space probe Ulysses is designed to measure the local
angular distribution of the flow of interstellar neutral He-atoms within≈ 3 AU distance from …

A self‐consistent gasdynamic model of the solar wind interaction with the local interstellar
medium (LISM), which took into account the mutual influence of the plasma component …

Singly-ionized helium with a velocity distribution extending up to double the solar wind
velocity has been detected in interplanetary space. This distribution unambiguously …

Ultraviolet studies of the interstellar gas ADS Classic is now deprecated. It will be completely
retired in October 2019. This page will automatically redirect to the new ADS interface at that …

This review examines the details of the interaction of the solar wind flux with interstellar gas
streaming into the solar system. A survey of the general astronomical setting of the solar …

Neutral atom imaging of the interstellar gas flow in the inner heliosphere provides the most
detailed information on physical conditions of the surrounding interstellar medium (ISM) and …

Because of its high ionization potential and weak interaction with hydrogen, neutral
interstellar helium (NISHe) is almost unaffected at the heliospheric interface with the …

The Voyager ultraviolet spectrometers (UVS) have been making almost continuous
observations, in the 500‐Å to 1700‐Å wavelength range, of sources in the solar system and …

A coordinated effort to combine all three methods that are used to determine the physical
parameters of interstellar gas in the heliosphere has been undertaken. In order to arrive at a …