One-Dimentional Numerical MHD Simulation of the Shock Events in the Outer Heliosphere

GUO Xiaocheng1,2, ZHOU Yucheng1,2, WANG Chi1,2, LI Hui1,2

PDF(850 KB)
PDF(850 KB)
Journal of Deep Space Exploration ›› 2020, Vol. 7 ›› Issue (6) : 560-566,604. DOI: 10.15982/j.issn.2096-9287.2020.20200059
Topic:Exploring the Solar System Boundary
Topic:Exploring the Solar System Boundary

One-Dimentional Numerical MHD Simulation of the Shock Events in the Outer Heliosphere

  • GUO Xiaocheng1,2, ZHOU Yucheng1,2, WANG Chi1,2, LI Hui1,2
Author information +
History +

Abstract

Voyager 1 occasionally detected the sudden jumps of the interstellar magnetic field strength since its heliopause crossing in August,2012. These events are believed to be the interstellar shocks,and associated with the product of the interaction between the large-scale solar wind structures and the heliopause. In this paper, this possibility is examined by means of a two-fluid magnetohydrodynamics(MHD)simulation consisting of the solar wind plasma and the interstellar neutrals. Three different solar wind observations from OMNI,STEREO A and B at a heliocentric distance of 1 au during the year 2010-2017 are used as input to the simulation,and the evolution of solar wind in the outer heliosphere is investigated after the charge-exchange between solar wind and interstellar neutrals.The numerical results are compared with the observation from the two Voyagers,showing that the shock events in the interstellar medium observed by Voyager 1 have direct linkage with the pressure pulses in the inner heliosheath detected by Voyager 2.

Keywords

outer heliosphere / shock events / solar wind / numerical MHD simulation

Cite this article

Download citation ▾
GUO Xiaocheng, ZHOU Yucheng, WANG Chi, LI Hui. One-Dimentional Numerical MHD Simulation of the Shock Events in the Outer Heliosphere. Journal of Deep Space Exploration, 2020, 7(6): 560‒566,604 https://doi.org/10.15982/j.issn.2096-9287.2020.20200059

References

[1] PARKER E N. The stellar wind regions[J]. The Astrophysical Journal,1961,134:20-27
[2] BURLAGA L F,NESS N F,ACU?A M H,et al. Magnetic fields at the solar wind termination shock[J]. Nature,2008,454(7200):75-77
[3] KRIMIGIS S M,DECKER R B,ROELOF E C,et al. Search for the exit:Voyager 1 at heliosphere’s border with the galaxy[J]. Science,2013,341(6242):144-147
[4] SARABHAI V. Some consequences of nonuniformity of solar wind velocity[J]. Journal of Geophysical Research,1963,68(5):1555-1557
[5] GOPALSWAMY N. Properties of interplanetary coronal mass ejections[J]. Space Science Reviews,2006,124:145-168
[6] WHANG Y C,BURLAGA L F. Evolution and interaction of interplanetary shocks[J]. Journal of Geophysical Research,1985,90(A11):10765-10778
[7] BURLAGA L F,NESS N F,BELCHER J W. Radial evolution of corotating merged interaction regions and flows between ~14 AU and ~43 AU[J]. Journal of Geophysical Research Space Physics,1997,102(A3):4661-4672
[8] WANG C,RICHARDSON J D. Development of a strong shock in the outer heliosphere[J]. Geophysical Research Letters,2002,29(8):1181-1188
[9] BURLAGA L F,NESS N F. Observations of the interstellar magnetic field in the outer heliosheath:Voyager 1[J]. The Astrophysical Journal,2016,829(2):1-10
[10] GURNETT D A,KURTH W S,STONE E C,et al. Precursors to interstellar shocks of solar origin[J]. The Astrophysical Journal,2015,809(2):1-10
[11] LIU Y D,RICHARDSON J D,WANG C,et al. Propagation of the 2012 march coronal mass ejections from the Sun to heliopause[J]. The Astrophysical Journal Letters,2014,788(2):1-6
[12] FERMO R L,POGORELOV N V,BURLAGA L F. Transient shocks beyond the heliopause[C]//14th Annual International Astrophysics Conference:Linear and Nonlinear Particle Energization Throughout the Heliosphere and Beyond. Tampa,Florida,USA:IOP,2015.
[13] KIM T K,POGORELOV N V,BURLAGA L F. Modelling shocks detected by Voyager 1 in the local interstellar medium[J]. The Astrophysical Journal Letters,2017,843(2):1-7
[14] POGORELOV N V,SUESS S T,BOROVIKOV S N,et al. Three-dimensional features of the outer heliosphere due to coupling between the interstellar and interplanetary magnetic fields. IV. Solar cycle model based on Ulysses observations[J]. The Astrophysical Journal,2013,772(2):1-17
[15] RICHARDSON J D,WANG C,LIU Y D,et al. Pressure pulses at Voyager 2:drivers of interstellar transients?[J]. The Astrophysical Journal,2017,834(2):1-6
[16] PAULS H L,ZANK G P,WILLIAMS L L. Interaction of the solar wind with the local interstellar medium[J]. Journal of Geophysical Research,1995,100(A11):21595-21604
[17] GUO X C,FLORINSKI V,WANG C. A global MHD simulation of outer heliosphere including anomalous cosmic-rays[J]. The Astrophysical Journal,2019,879(2):1-10
[18] FLORINSKI V,GUO X,BALSARA D S,et al. Magnetohydrodynamic modeling of solar system processes on geodesic grids[J]. The Astrophysical Journal Supplement Serisa,2013,205(2):1-12
[19] GUO X C. An extended HLLC Riemann solver for the magneto-hydrodynamics including strong internal magnetic field[J]. Journal of Computional Physics,2015,290:352-363
[20] AXFORD W 1. The interaction of the solar wind with the interstellar medium[C]//In Solar Wind:Proceedings of the Second International Conference. [S.l.]:NASA,1972.
[21] WANG C,RICHARDSON J D. Energy partition between solar wind protons and pickup ions in the distant heliosphere:a three-fluid approach[J]. Journal of Geophysical Research,2001,106(A12):29401-29408
[22] GUO X C,FLORINSKI V. Galactic cosmic-ray intensity modulation by corotating interaction region stream interfaces at 1 AU[J]. The Astrophysical Journal,2016,826(1):1-13
[23] RICHARDSON J D,BELCHER J W,GARCIA-GALINDO P,et al. Voyager 2 plasma observations of the heliopause and interstellar medium[J]. Nature,2019(3):1019-1023
[24] GURNETT D A,KURTH W S. Plasma densities near and beyond the heliopause from the Voyager 1 and 2 plasma wave instruments[J]. Nature Astronomy,2019,3(11):1024-1028
[25] BALE S D,REINER M J,BOUGERET J L,et al. The source region of an interplanetary type II radio burst[J]. Geophysical Research Letters,1999,26(11):1573-1576
[26] GAZIS P R. Solar wind stream structure at large heliocentric distances:pioneer observations[J]. Journal of Geophysical Research,1987,92(A3):2231-2242
[27] SZABO A,SMITH C W,SKOUG R M. The transition of interplanetary shocks through the magnetosheath[C]//AIP Conference Proceedings. Melville,NY:AIP,2003.
[28] JIAN L K,RUSSELL C,LUHMANN J G,et al. STEREO observations of interplanetary coronal mass ejections in 2007–2016[J]. The Astrophysical Journal,2018,855(2):1-19
[29] STONE E C,CUMMINGS A C,MCDONALD F B,et al. Voyager 1 observes low-energy galactic cosmic rays in a region depleted of heliospheric ions[J]. Science,2013,341(6142):150-153
[30] CUMMINGS A C,STONE E C,HEIKKILA B C,et al. Galactic cosmic rays in the local interstellar medium:Voyager 1 observations and model results[J]. The Astrophysical Journal,2016,831(1):1-21
[31] BURLAGA L F,NESS N F. Observations of the interstellar magnetic field in the outer heliosheath:Voyager 1[J]. The Astrophysical Journal,2013,829(2):1-10
PDF(850 KB)

Accesses

Citations

Detail

Sections
Recommended

/