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Effects of Dispersion of the Dust Velocity in the LISM on the Interstellar Dust Distribution inside the Heliosphere

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Abstract

Interstellar dust (ISD) penetrates into the heliosphere due to the relative motion of the Sun and the local interstellar medium (LISM). Inside the heliosphere and at the boundaries, where solar wind interacts with the LISM, distribution of ISD is modified due to the action of the electromagnetic forces, the solar gravitation and the radiation pressure. These forces make the distribution of the ISD particles in the heliosphere inhomogeneous. In previous work we demonstrated the existence of singularities in the ISD density distribution at 0.03–10 AU north and south with respect to the heliospheric current sheet. In this paper we show that dispersion in the ISD velocity distribution strongly affects the singularities. Even small values of dispersion have the drastic impact on the density distribution and smooth the high density layers discovered previously.

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ACKNOWLEDGMENTS

Authors are grateful to the Government of Russian Federation and the Ministry of Science and Higher Education for the support by grant 075-15-2020-780 (no. 13.1902.21.0039). We thank D.B. Alexashov, I.I. Baliukin, and A. Granovskiy for useful discussions and for the help with the preparation of the manuscript. This work is supported by grant 18-1-1-22-1 of ‘‘Basis’’ Foundation.

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Correspondence to E. A. Godenko.

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Godenko, E.A., Izmodenov, V.V. Effects of Dispersion of the Dust Velocity in the LISM on the Interstellar Dust Distribution inside the Heliosphere. Astron. Lett. 47, 50–60 (2021). https://doi.org/10.1134/S1063773721010047

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  • DOI: https://doi.org/10.1134/S1063773721010047

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