Modeling of the outer heliosphere with the realistic solar cycle

被引：56

作者：

Izmodenov, Vladislav V. ^{[1
,2
,3
]}

Malama, Yuri G. ^{[2
,3
]}

Ruderman, Michael S. ^{[4
]}

机构：

[1] Moscow MV Lomonosov State Univ, Dept Aeromech & Gas Dynam, Sch Mech & Math, Moscow 119899, Russia

[2] Russian Acad Sci, Space Res Inst, IKI, Moscow 117997, Russia

[3] Russian Acad Sci, Inst Problems Mech, Moscow 119526, Russia

[4] Univ Sheffield, Dept Appl Math, Sheffield S3 7RH, S Yorkshire, England

来源：

ADVANCES IN SPACE RESEARCH | 2008年 / 41卷 / 02期

基金：

俄罗斯基础研究基金会;

关键词：

heliospheric termination shock; heliospheric interface; solar wind; solar cycle; interstellar H atoms;

D O I：

10.1016/j.asr.2007.06.033

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

Time-dependent kinetic-continuum model of the solar wind interaction with the two-component local interstellar cloud (LIC) has been developed recently [Izmodenov, V., Malama, Y.G., Ruderman, M.S. Solar cycle influence on the interaction of the solar wind with local interstellar cloud. Astron. Astrophys. 429, 1069-1080, 2005a.]. Here, we adopted this model to the realistic solar cycle, when the solar wind parameters at the Earth's orbit are taken from space data. This paper focuses on the results related to the termination shock (TS) excursion with the solar cycle that may help to understand Voyager I data obtained at and after the crossing of the termination shock and to predict the time of the TS crossing by Voyager 2. (C) 2007 COSPAR. Published by Elsevier Ltd. All rights reserved.

引用

页码：318 / 324

页数：7

共 26 条

[1] Model Representations of the Interaction Between the Solar Wind and the Supersonic Interstellar Medium Flow. Prediction and Interpretation of Experimental Data [J].

Baranov, V. B. ;

Izmodenov, V. V. .

FLUID DYNAMICS, 2006, 41 (05) :689-707

[2]

Bzowski M, 2001, COSPAR COLL, V11, P69

[3] Voyager 1 in the foreshock, termination shock, and heliosheath [J].

Decker, RB ;

Krimigis, SM ;

Roelof, EC ;

Hill, ME ;

Armstrong, TP ;

Gloeckler, G ;

Hamilton, DC ;

Lanzerotti, LJ .

SCIENCE, 2005, 309 (5743) :2020-2024

[4] Composition of the local interstellar medium as diagnosed with pickup ions [J].

Gloeckler, G ;

Geiss, J .

TO THE EDGE OF THE SOLAR SYSTEM AND BEYOND, 2004, 34 (01) :53-60

[5] Observations of the helium focusing cone with pickup ions [J].

Gloeckler, G ;

Möbius, E ;

Geiss, J ;

Bzowski, M ;

Chalov, S ;

Fahr, H ;

McMullin, DR ;

Noda, H ;

Oka, M ;

Rucinski, D ;

Skoug, R ;

Terasawa, T ;

von Steiger, R ;

Yamazaki, A ;

Zurbuchen, T .

ASTRONOMY & ASTROPHYSICS, 2004, 426 (03) :845-854

[6] Solar cycle influence on the interaction of the solar wind with Local Interstellar Cloud [J].

Izmodenov, V ;

Malama, Y ;

Ruderman, MS .

ASTRONOMY & ASTROPHYSICS, 2005, 429 (03) :1069-U17

[7] Direction of the interstellar H atom inflow in the heliosphere: Role of the interstellar magnetic field [J].

Izmodenov, V ;

Alexashov, D ;

Myasnikov, A .

ASTRONOMY & ASTROPHYSICS, 2005, 437 (03) :L35-L38

[8] Variations of interstellar H atom parameters in the outer heliosphere: solar cycle effects [J].

Izmodenov, V ;

Malama, YG .

TO THE EDGE OF THE SOLAR SYSTEM AND BEYOND, 2004, 34 (01) :74-78

[9] When will Voyager 1 and 2 cross the termination shock? [J].

Izmodenov, V ;

Gloeckler, G ;

Malama, Y .

GEOPHYSICAL RESEARCH LETTERS, 2003, 30 (07) :3-1

[10] Effects of interstellar and solar wind ionized helium on the interaction of the solar wind with the local interstellar medium [J].

Izmodenov, V ;

Malama, YG ;

Gloeckler, G ;

Geiss, J .

ASTROPHYSICAL JOURNAL, 2003, 594 (01) :L59-L62

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