The properties (density, bulk velocity relative to the solar system, and temperature) of the local interstellar gas, represented by neutral helium penetrating the heliosphere, will be measured in-situ for the first time by the ULYSSES GAS instrument. By employing the solar gravitational field as a natural velocity analyser, the bulk velocity relative to the solar system and the temperature of the E as can be derived from the angular distributions of the particles measured in at least two widely separated points in the heliosphere. The gas density can be determined if a composition corresponding to cosmic abundances is assumed. The neutral particles are detected via the secondary electrons or ions which are emitted upon particle impact fr... ...Show More
urn:nasa:pds:context:instrument:gas.uly
1.0