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Science 21 May 1993:
Vol. 260. no. 5111, pp. 1095 - 1098
DOI: 10.1126/science.260.5111.1095
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Articles

Deceleration of Interstellar Hydrogen at the Heliospheric Interface

Rosine Lallement 1, Jean-Loup Bertaux 1, and John T. Clarke 2

1 Service d'aéronomie du CNRS BP 3, F91371 Verrières-le-buisson, France
2 Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI 48109

High-resolution spectra of nearby stars show absorption lines due to material in the local interstellar cloud. This cloud is deduced to be moving at 26 kilometers per second with respect to the sun, and in the same direction as the "interstellar wind" flowing through the solar system. Measurements by the Ulysses spacecraft show that neutral helium is drifting through the solar system at the same velocity, but neutral hydrogen appears to be moving at only 20 kilometers per second, a result confirmed by new measurements of the hydrogen emission line taken by the High-Resolution Spectrograph on the Hubble Space Telescope. These results indicate that neutral hydrogen atoms from the local interstellar cloud are preferentially decelerated at the heliospheric interface, most likely by charge-exchange with interstellar protons, while neutral helium is unaffected by the plasma. The magnitude of the observed deceleration implies an interstellar plasma density of 0.06 to 0.10 per cubic centimeter, which in turn implies that the heliospheric shock should be less than 100 astronomical units from the sun.

Submitted on January 19, 1993
Accepted on March 30, 1993


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
Deflection of the Interstellar Neutral Hydrogen Flow Across the Heliospheric Interface.
R. Lallement, E. Quemerais, J. L. Bertaux, S. Ferron, D. Koutroumpa, and R. Pellinen (2005)
Science 307, 1447-1449
   Abstract »    Full Text »    PDF »
Morphology and Ionization of the Interstellar Cloud Surrounding the Solar System.
P. C. Frisch (1994)
Science 265, 1423-1427
   Abstract »    PDF »
Radio Emission from the Heliopause Triggered by an Interplanetary Shock.
D. A. Gurnett, W. S. Kurth, S. C. Allendorf, and R. L. Poynter (1993)
Science 262, 199-203
   Abstract »    PDF »


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Science. ISSN 0036-8075 (print), 1095-9203 (online)