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Neutral component of the outerstellar medium in the vicinity of the Sun

Published online by Cambridge University Press:  04 August 2017

Vladimir G. Kurt
Affiliation:
Space Research Institute USSR Academy of Sciences Moscow, USSR
Jean-Loup Bertaux
Affiliation:
Service Aeronomie, Verierre, France

Extract

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Optical observations of the solar radiation resonance scattering in the hydrogen and helium lines (λ1216Å and 584Å) provide a unique opportunity for determining numerous parameters of the local interstellar medium closest to the Sun (LISM). The distance exceeds 10 to 102 AU where the interstellar medium is no longer perturbed by the gravity field, and the hard and corpuscular radiation of the Sun.

Type
Stellar Coronae: Chromospheres of Cool Stars
Copyright
Copyright © Reidel 1987 

References

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