Detection of the local interstellar cloud from high-resolution spectroscopy of nearby stars: Inferences on the heliospheric interface

Author:

Bertin P.,Lallement R.,Ferlet R.,Vidal-Madjar A.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference29 articles.

1. The Influence of the interface between the heliosphere and the local interstellar medium on the penetration of the H atoms to the solar system;Baranov;Astrophys. J.,1991

2. Characteristics of the local interstellar hydrogen determined from Prognoz 5 and 6 interplanetary Lyman-alpha line profiles measurements with a hydrogen absorption cell;Bertaux;Astron. Astrophys.,1985

3. High resolution observations of interstellar NaI and Call towards the Scorpio-Centaurus association;Crawford;Astron. Astrophys.,1991

4. The local interstellar medium;Crutcher;Astrophys. J.,1982

5. Characteristics of interstellar helium observed with Prognoz 6 58.4 nm photometers;Dalaudier;Astron. Astrophys.,1984

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