Astronomy and Astrophysics, volume 437, issue 3, pages L35-L38
Direction of the interstellar H atom inflow in the heliosphere: Role of the interstellar magnetic field
Publication type: Journal Article
Publication date: 2005-06-30
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
Recently Lallement et al. (2005, Science, 307, 1447) reported that the direction of the flow of interstellar neutral hydrogen in the heliosphere is deflected by ~4° from the direction of the pristine local interstellar gas flow. The most probable physical phenomenon responsible for such a deviation is the interstellar magnetic field inclined to the direction of the interstellar gas flow. In this case the flow of the interstellar charged component is asymmetric and distorted in the region of the solar wind interaction with the local interstellar medium, which is called the heliospheric interface. The interstellar H atoms pass through the heliospheric interface and interact with the plasma component by charge exchange. Some imprints of the asymmetry of the heliospheric plasma interface should be seen in the distribution of the interstellar H atom component. In this letter we explore this scenario quantitatively and demonstrate that our new self-consistent 3D kinetic-MHD model of the solar wind interaction with the magnetized interstellar plasma is able to produce the measured deviation in the case of a rather strong interstellar magnetic field of ~2.5 μ G inclined by ~45° to the direction of interstellar flow.
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Izmodenov V. et al. Direction of the interstellar H atom inflow in the heliosphere: Role of the interstellar magnetic field // Astronomy and Astrophysics. 2005. Vol. 437. No. 3. p. L35-L38.
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Izmodenov V., Alexashov D., Myasnikov A. Direction of the interstellar H atom inflow in the heliosphere: Role of the interstellar magnetic field // Astronomy and Astrophysics. 2005. Vol. 437. No. 3. p. L35-L38.
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TY - JOUR
DO - 10.1051/0004-6361:200500132
UR - https://doi.org/10.1051%2F0004-6361%3A200500132
TI - Direction of the interstellar H atom inflow in the heliosphere: Role of the interstellar magnetic field
T2 - Astronomy and Astrophysics
AU - Izmodenov, Vlad
AU - Alexashov, Dmitry
AU - Myasnikov, A.
PY - 2005
DA - 2005/06/30 00:00:00
PB - EDP Sciences
SP - L35-L38
IS - 3
VL - 437
SN - 0004-6361
SN - 1432-0746
SN - 2329-1273
SN - 2329-1265
ER -
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@article{2005_Izmodenov,
author = {Vlad Izmodenov and Dmitry Alexashov and A. Myasnikov},
title = {Direction of the interstellar H atom inflow in the heliosphere: Role of the interstellar magnetic field},
journal = {Astronomy and Astrophysics},
year = {2005},
volume = {437},
publisher = {EDP Sciences},
month = {jun},
url = {https://doi.org/10.1051%2F0004-6361%3A200500132},
number = {3},
pages = {L35--L38},
doi = {10.1051/0004-6361:200500132}
}
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MLA
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Izmodenov, Vlad, et al. “Direction of the interstellar H atom inflow in the heliosphere: Role of the interstellar magnetic field.” Astronomy and Astrophysics, vol. 437, no. 3, Jun. 2005, pp. L35-L38. https://doi.org/10.1051%2F0004-6361%3A200500132.