Computer Science
Scientific paper
Jun 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13..121w&link_type=abstract
Advances in Space Research (ISSN 0273-1177), vol. 13, no. 6, p. 121-130.
Computer Science
151
Gas Temperature, Helium, Interstellar Gas, Neutral Gases, Ulysses Mission, Velocity Measurement, Backscattering, Solar Wind
Scientific paper
A new technique to directly detect low energy neutral helium has been developed and successfully used in space for the first time. It makes possible the in situ measurement of the local angular distribution of the flow of interstellar neutral helium in the inner heliosphere. Based on the transformation of a velocity distribution, using Liouville's theorem, a straightforward model has been developed to determine, from these measurements, the flow parameters of the interstellar helium at infinity. From 12 measurements at radial distances between 1 and 5 AU, average values of the flow parameters were determined, namely: v(infinity) = 26 +/- 1 km/s, downstream direction: lambda(infinity) = 72 +/- 2.4 deg, beta(infinity) = -2.5 +/- 2.7 deg, temperature T(infinity) = 6700 +/- 1500 K. These values are in agreement with results found by completely different methods, although in detail there are significant differences.
Banaszkiewicz Marek
Fahr Hans
Rosenbauer Helmut
Witte Malte
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