Open Access
Astrophysical Journal, Supplement Series, volume 220, issue 2, pages 32
THREE-DIMENSIONAL KINETIC-MHD MODEL OF THE GLOBAL HELIOSPHERE WITH THE HELIOPAUSE-SURFACE FITTING
Izmodenov Vlad
1, 2
,
Publication type: Journal Article
Publication date: 2015-10-20
Quartile SCImago
Q1
Quartile WOS
Q1
Impact factor: 8.7
ISSN: 00670049, 15384365
Space and Planetary Science
Astronomy and Astrophysics
Abstract
This paper provides a detailed description of the latest version of our model of the solar wind (SW) interaction with the local interstellar medium (LISM). This model has already been applied to the analysis of Lyman-alpha absorption spectra toward nearby stars and for analyses of Solar and Heliospheric Observatory/SWAN data. Katushkina et al. (this issue) used the model results to analyze IBEX-Lo data. At the same time, the details of this model have not yet been published. This is a three-dimensional (3D) kinetic-magnetohydrodynamical (MHD) model that takes into account SW and interstellar plasmas (including $\alpha$ particles in SW and helium ions in LISM), the solar and interstellar magnetic fields, and the interstellar hydrogen atoms. The latitudinal dependence of SW and the actual flow direction of the interstellar gas with respect to the Sun are also taken into account in the model. It was very essential that our numerical code had been developed in such a way that any numerical diffusion or reconnection across the heliopause had not been allowed in the model. The heliospheric current sheet is a rotational discontinuity in the ideal MHD and can be treated kinematically. In the paper, we focus in particular on the effects of the heliospheric magnetic field and on the heliolatitudinal dependence of SW.
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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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Izmodenov V., Alexashov D. THREE-DIMENSIONAL KINETIC-MHD MODEL OF THE GLOBAL HELIOSPHERE WITH THE HELIOPAUSE-SURFACE FITTING // Astrophysical Journal, Supplement Series. 2015. Vol. 220. No. 2. p. 32.
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Izmodenov V., Alexashov D. THREE-DIMENSIONAL KINETIC-MHD MODEL OF THE GLOBAL HELIOSPHERE WITH THE HELIOPAUSE-SURFACE FITTING // Astrophysical Journal, Supplement Series. 2015. Vol. 220. No. 2. p. 32.
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TY - JOUR
DO - 10.1088/0067-0049/220/2/32
UR - https://doi.org/10.1088%2F0067-0049%2F220%2F2%2F32
TI - THREE-DIMENSIONAL KINETIC-MHD MODEL OF THE GLOBAL HELIOSPHERE WITH THE HELIOPAUSE-SURFACE FITTING
T2 - Astrophysical Journal, Supplement Series
AU - Izmodenov, Vlad
AU - Alexashov, Dmitry
PY - 2015
DA - 2015/10/20 00:00:00
PB - American Astronomical Society
SP - 32
IS - 2
VL - 220
SN - 0067-0049
SN - 1538-4365
ER -
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@article{2015_Izmodenov,
author = {Vlad Izmodenov and Dmitry Alexashov},
title = {THREE-DIMENSIONAL KINETIC-MHD MODEL OF THE GLOBAL HELIOSPHERE WITH THE HELIOPAUSE-SURFACE FITTING},
journal = {Astrophysical Journal, Supplement Series},
year = {2015},
volume = {220},
publisher = {American Astronomical Society},
month = {oct},
url = {https://doi.org/10.1088%2F0067-0049%2F220%2F2%2F32},
number = {2},
pages = {32},
doi = {10.1088/0067-0049/220/2/32}
}
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MLA
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Izmodenov, Vlad, et al. “THREE-DIMENSIONAL KINETIC-MHD MODEL OF THE GLOBAL HELIOSPHERE WITH THE HELIOPAUSE-SURFACE FITTING.” Astrophysical Journal, Supplement Series, vol. 220, no. 2, Oct. 2015, p. 32. https://doi.org/10.1088%2F0067-0049%2F220%2F2%2F32.