Astronomy and Astrophysics, volume 445, issue 2, pages 693-701
Modeling of the heliospheric interface: multi-component nature of the heliospheric plasma
Publication type: Journal Article
Publication date: 2005-12-16
Journal:
Astronomy and Astrophysics
Quartile SCImago
Q1
Quartile WOS
Q1
Impact factor: 6.5
ISSN: 00046361, 14320746, 23291273, 23291265
Space and Planetary Science
Astronomy and Astrophysics
Abstract
We present a new model of the heliospheric interface - the region of the solar wind interaction with the local interstellar medium. This new model performs a multi-component treatment of charged particles in the heliosphere. All charged particles are divided into several co-moving types. The coldest type, with parameters typical of original solar wind protons, is considered in the framework of fluid approximation. The hot pickup proton components created from interstellar H atoms and heliospheric ENAs by charge exchange, electron impact ionization and photoionization are treated kinetically. The charged components are considered self-consistently with interstellar H atoms, which are described kinetically as well. To solve the kinetic equation for H atoms we use the Monte Carlo method with splitting of trajectories, which allows us 1) to reduce statistical uncertainties allowing correct interpretation of observational data; 2) to separate all H atoms in the heliosphere into several populations depending on the place of their birth and on the type of parent protons.
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- We do not take into account publications that without a DOI.
- Statistics recalculated only for publications connected to researchers, organizations and labs registered on the platform.
- Statistics recalculated weekly.
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Malama Y. G. et al. Modeling of the heliospheric interface: multi-component nature of the heliospheric plasma // Astronomy and Astrophysics. 2005. Vol. 445. No. 2. pp. 693-701.
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Malama Y. G., Izmodenov V., CHALOV S. R. Modeling of the heliospheric interface: multi-component nature of the heliospheric plasma // Astronomy and Astrophysics. 2005. Vol. 445. No. 2. pp. 693-701.
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TY - JOUR
DO - 10.1051/0004-6361:20053646
UR - https://doi.org/10.1051%2F0004-6361%3A20053646
TI - Modeling of the heliospheric interface: multi-component nature of the heliospheric plasma
T2 - Astronomy and Astrophysics
AU - Malama, Y. G.
AU - Izmodenov, Vlad
AU - CHALOV, Sergey R.
PY - 2005
DA - 2005/12/16 00:00:00
PB - EDP Sciences
SP - 693-701
IS - 2
VL - 445
SN - 0004-6361
SN - 1432-0746
SN - 2329-1273
SN - 2329-1265
ER -
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@article{2005_Malama,
author = {Y. G. Malama and Vlad Izmodenov and Sergey R. CHALOV},
title = {Modeling of the heliospheric interface: multi-component nature of the heliospheric plasma},
journal = {Astronomy and Astrophysics},
year = {2005},
volume = {445},
publisher = {EDP Sciences},
month = {dec},
url = {https://doi.org/10.1051%2F0004-6361%3A20053646},
number = {2},
pages = {693--701},
doi = {10.1051/0004-6361:20053646}
}
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MLA
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Malama, Y. G., et al. “Modeling of the heliospheric interface: multi-component nature of the heliospheric plasma.” Astronomy and Astrophysics, vol. 445, no. 2, Dec. 2005, pp. 693-701. https://doi.org/10.1051%2F0004-6361%3A20053646.
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