Citation: | ZHAO Xinhua, ZHANG Min, WANG Yuming, HE Jiansen, NING Hao, QIN Gang. Interplanetary Physics in Mainland China[J]. Chinese Journal of Space Science, 2018, 38(5): 665-693. doi: 10.11728/cjss2018.05.665 |
[1] |
RUAN W Z, HE J S, ZHANG L, et al. Kinetic simulation of slow magnetosonic waves and quasi-periodic upflows in the solar corona[J]. Astrophys. J., 2016, 825:58
|
[2] |
YANG L P, FENG X S, HE J S, et al. A self-consistent numerical study of the global solar wind driven by the unified nonlinear Alfven wave[J]. Solar. Phys., 2016, 291(3):953-963
|
[3] |
PEI Z, HE J, WANG X, et al. Influence of intermittency on the anisotropy of magnetic structure functions of solar wind turbulence[J]. J. Geophys. Res.:Space Phys., 2016, 121(2):911-924
|
[4] |
YANG L, HE J, TU C, et al. Multiscale pressurebalanced structures in three-dimensional magnetohydrodynamic turbulence[J]. Astrophys. J., 2017, 836:69-77
|
[5] |
YANG L, HE J, TU C, et al. Influence of intermittency on the quasi-perpendicular scaling in three-dimensional magnetohydrodynamic turbulence[J]. Astrophys. J., 2017, 846:49
|
[6] |
YANG L, ZHANG L, HE J, et al. Formation and properties of tangential discontinuities in three-dimensional compressive MHD turbulence[J]. Astrophys. J., 2017, 851(2):121
|
[7] |
WANG X, TU C Y, HE J S, et al. Reexamination of data analysis for -2 spectral index at small theta-VB angle[R]//Proceedings of the 14th Solar Wind Conference, 2016, 1720:040020
|
[8] |
WANG X, TU C Y, HE J S, et al. On the weakly anisotropic nature of the time-stationary turbulence in the solar wind[C]//Proceedings of the 14th Solar Wind Conference, 2016, 1720:040019
|
[9] |
TU C Y, WANG X, HE J S, et al. The nature of the slow solar wind turbulence[R]//Proceedings of the 14th Solar Wind Conference, 2016, 1720:040017
|
[10] |
WANG X, TU C Y, HE J S, et al. Ion-scale spectral break in the normal plasma beta range in the solar wind turbulence[J]. J. Geophys. Res.:Space Phys., 2018, 123:68
|
[11] |
WANG X, TU C Y, HE J S, et al. Possible noise nature of Elsässer variable z- in highly Alfvénic solar wind fluctuations[J]. J. Geophys. Res.:Space Phys., 2018, 123:57
|
[12] |
YANG Z C, SHEN F, ZHANG J, et al. Correlation between the magnetic field and plasma parameters at 1 AU[J]. Solar Phys., 2018, 293:24
|
[13] |
YANG L P, ZHANG L, HE J S, et al. Disappearance of anisotropic intermittency in large-amplitude MHD turbulence and its comparison with small-amplitude MHD turbulence[J]. Astrophys. J., 2018, 855:69
|
[14] |
ZHANG Q H, WANG Y M, LIU R, et al. Damped large amplitude oscillations in a solar prominence and a bundle of coronal loops[J]. Res. Astron. Astrophys., 2016, 16:167
|
[15] |
WANG W S, LIU R, WANG Y M. Tornado-like evolution of a kink-unstable solar prominence[J]. Astrophys. J., 2017, 834:38
|
[16] |
LIU J J, WANG Y M, ERDELYI R, et al. On the magnetic and energy characteristics of recurrent homologous jets from an emerging flux[J]. Astrophys. J., 2016, 833:150
|
[17] |
LIU J J, FANG F, WANG Y M, et al. On the observation and simulation of solar coronal twin jets[J]. Astrophys. J., 2016, 817:126
|
[18] |
WANG B, CHEN Y, FU J, et al. Dynamics of a prominence-horn structure during its evaporation in the solar corona[J]. Astrophys J., 2016, 827(2):L33
|
[19] |
ZHENG R, ZHANG Q, CHEN Y, et al. Interaction of two filaments in a long filament channel associated with twin coronal mass ejections[J]. Astrophys J., 2017, 8366(2):160
|
[20] |
SONG H Q, CHEN Y, LI B, et al. The origin of solar filament plasma inferred from in situ observations of elemental abundances[J]. Astrophys. J. Lett., 2017, 836(1):L11
|
[21] |
ZHENG R, CHEN Y, WANG B, et al. Interchange reconnection associated with a confined filament eruption:implications for the source of transient cold-dense plasma in Solar winds[J]. Astrophys. J., 2017, 840(1):3
|
[22] |
WANG Y M, ZHOU Z J, ZHANG J, et al. Thermodynamic spectrum of solar flares based on SDO/EVE observations:techniques and first results[J]. Astrophys. J. Supp., 2016, 223:4
|
[23] |
GOU T Y, LIU R, WANG Y M, et al. Stereoscopic observation of slipping reconnection in a double candle-flameshaped flare[J]. Astrophys. J. Lett., 2016, 821:L28
|
[24] |
LIU R, CHEN J, WANG Y M, et al. Investigating energetic X-shaped flares on the outskirts of a solar active region[J]. Sci. Rep., 2016, 6:34021
|
[25] |
WU Z, CHEN Y, HUANG G, et al. Microwave imaging of a hot flux rope structure during the pre-impulsive stage of an eruptive M7.7 solar flare[J]. Astrophys. J., 2016, 820(2):L29
|
[26] |
ZHENG R, CHEN Y, WANG B. Slipping magnetic reconnections with multiple flare ribbons during an X-class solar flare[J]. Astrophys. J., 2016, 823(2):136
|
[27] |
CHEN Y, WU Z, LIU W, et al. Double-coronal X-ray and microwave sources associated with a magnetic breakout solar eruption[J]. Astrophys. J., 2017, 843(1):8
|
[28] |
SONG Q, WANG J S, FENG X S, et al. Dark post-flare loops observed by the solar dynamics observatory[J]. Astrophys. J., 2016, 821:83
|
[29] |
JIANG C W, WU S T, YURCHYSHYN V, et al. How did a major confined flare occur in super solar active region 12192[J]. Astrophys. J., 2016, 828:62
|
[30] |
FENG SW, CHEN Y, SONG HQ, et al. An imaging study of a complex solar coronal radio eruption[J]. Astrophys. J., 2016, 827(1):L9
|
[31] |
KOVAL A, STANISLAVSKY A, CHEN Y, et al. A decameter stationary type iv burst in imaging observations on 2014 September 6[J]. Astrophys J., 2016, 826(2):125
|
[32] |
KONG X, CHEN Y, FENG S, et al. Observation of a metric type N solar radio burst[J]. Astrophys. J., 2016, 830(1):37
|
[33] |
VASANTH V, CHEN Y, FENG S, et al. An eruptive hot-channel structure observed at metric wavelength as a moving type-IV solar radio burst[J]. Astrophys. J., 2016, 830(1):L2
|
[34] |
LI C Y, CHEN Y, WANG B, et al. EUV and magnetic activities associated with type-I solar radio bursts[J]. Solar Phys., 2017, 292(6):82
|
[35] |
KOVAL A, CHEN Y, STANISLAVSKY A, et al. Traveling ionospheric disturbances as huge natural lenses:solar radio emission focusing effect[J]. J. Geophys. Res. Sp. Phys., 2017, 122:9092-9101
|
[36] |
LÜ M S, CHEN Y, LI CY, et al. Sources of the multilane type Ⅱ solar radio burst on 5 November 2014[J]. Solar Phys., 2017, 2922(12):194
|
[37] |
KONG X, CHEN Y, GUO F. The acceleration of electrons at a spherical coronal shock in a streamer-like coronal field[R]. AIP Conf. Proc., 2016, 1720:070003
|
[38] |
KONG X, CHEN Y, GUO F, et al. Electron acceleration at a coronal shock propagating through a largescale streamer-like magnetic field[J]. Astrophys J., 2016, 821(1):32
|
[39] |
KONG X, GUO F, GIACALONE J, et al. The acceleration of high-energy protons at coronal shocks:the effect of large-scale streamer-like magnetic field structures[J]. Astrophys. J., 2017, 851(1):38
|
[40] |
WANG W S, LIU R, WANG Y M, et al. Buildup of a highly twisted magnetic flux rope during a solar eruption[J]. Nat. Comm., 2017, 8:1330
|
[41] |
WANG Y M, ZHUANG B, HU Q, et al. On the twists of interplanetary magnetic flux ropes observed at 1 AU[J]. J. Geophys. Res., 2016, 121:9316-9339
|
[42] |
LIU R, KLIEM B, TITOV V S, et al. Structure, stability, and evolution of magnetic flux ropes from the perspective of magnetic twist[J]. Astrophys. J., 2016, 818:148
|
[43] |
ZHANG Q H, WANG Y M, HU Y Q, et al. Influence of photospheric magnetic conditions on the catastrophic behaviors of flux ropes in active regions[J]. Astrophys. J., 2017, 835:11
|
[44] |
ZHANG Q H, WANG Y M, HU Y Q, et al. Downward catastrophe of solar magnetic flux ropes[J]. Astrophys. J., 2016, 825:109
|
[45] |
LIU C X, FENG X S, NAKAMURA R, et al. Doublepeaked core field of flux ropes during magnetic reconnection[J]. J. Geophys. Res. Space Phys., 2017, 122:6374-6384
|
[46] |
YANG L P, PETER H, HE J S, et al. Formation of cool and warm jets by magnetic flux emerging from the solar chromosphere to transition region[J]. Astrophys. J., 2018, 852:16
|
[47] |
TIAN C, CHEN Y. Numerical simulations of KelvinHelmholtz instability:a two-dimensional parametric study[J]. Astrophys J., 2016, 824:60
|
[48] |
DU Q F, CHEN L, ZHAO Y-C, et al. A solar radio dynamic spectrograph with flexible temporal-spectral resolution[J]. Res Astron Astrophys., 2017, 17:98
|
[49] |
FAN S T, HE J S, YAN L M, et al. Turbulence and heating in the flank and wake regions of a coronal mass ejection[J]. Solar Phys., 2018, 293(1):6
|
[50] |
MAO S, HE J, ZHANG L, et al. Numerical study of erosion, heating, and acceleration of the magnetic cloud as impacted by fast shock[J]. Astrophys. J., 2017, 842:109
|
[51] |
LIU L J, WANG Y M, WANG J X, et al. Why is a flare-rich active region CME-poor[J]. Astrophys. J., 2016, 826:119
|
[52] |
LIU L J, WANG Y M, LIU R, et al. The causes of quasihomologous CMEs[J]. Astrophys. J., 2017, 844:141
|
[53] |
SHEN F, WANG Y M, SHEN C L, et al. Turn on the super-elastic collision nature of coronal mass ejections through low approaching speed[J]. Sci. Rep., 2016, 6:19576
|
[54] |
SHEN F, WANG Y M, SHEN C L, et al. On the collision nature of two coronal mass ejections:a review[J]. Solar Phys., 2017, 292:104
|
[55] |
GUO J P, WEI F S, FENG X S, et al. Prolonged multiple excitation of large-scale Traveling Atmospheric Disturbances (TADs) by successive and interacting coronal mass ejections[J]. J. Geophys. Res., 2016, 121:2662-2668
|
[56] |
WANG Y M, ZHANG Q H, LIU J J, et al. On the propagation of a geoeffective coronal mass ejection during March 1517, 2015[J]. J. Geophys. Res., 2016, 121:7423-7434
|
[57] |
ZHAO A K, WANG Y M, CHI Y T, et al. Main cause of the poloidal plasma motion inside a magnetic cloud inferred from multiple-spacecraft observations[J]. Solar Phys., 2017, 292:58
|
[58] |
ZHAO A K, WANG Y M, LIU J J, et al. The role of viscosity in causing the plasma poloidal motion in magnetic clouds[J]. Astrophys. J.,2017, 845:109
|
[59] |
ZHANG B, WANG Y M, SHEN C L, et al. The significance of the influence of the CME deflection in interplanetary space on the CME arrival at the earth[J]. Astrophys. J., 2017, 845:117
|
[60] |
CHI Y T, SHEN C L, WANG Y M, et al. Statistical study of the interplanetary coronal mass ejections from 1996 to 2015[J]. Solar Phys., 2016, 291:2419-2439
|
[61] |
CHEN Y, DU G, ZHAO D, et al. Imaging a magnetic-breakout solar eruption[J]. Astrophys J., 2016, 820(2):L37
|
[62] |
ZHENG R, CHEN Y, DU G, et al. Solar Jetcoronal hole collision and a closely related coronal mass ejection[J]. Astrophys J., 2016, 819(2):L18
|
[63] |
SONG H Q, ZHONG Z, CHEN Y, et al. A statistical study of the average iron charge state distributions inside magnetic clouds for solar cycle 23[J]. Astrophys. J. Suppl. Ser., 2016, 224(2):27
|
[64] |
SONG H Q, CHENG X, CHEN Y, et al. The three-part structure of a filament-unrelated solar coronal mass ejection[J]. Astrophys J., 2017, 848(1):21
|
[65] |
HU H D, LIU Y D, WANG R, et al. Sun-to-Earth characteristics of the 2012 July 12 coronal mass ejection and associated geo-effectiveness[J]. Astrophys. J., 2016, 829:97
|
[66] |
ZHU B, LIU Y D, LUHMANN J G, et al. Solar energetic particle event associated the 2012 July extreme solar storm[J]. Astrophys J., 2016, 827
|
[67] |
WANG R, LIU Y D, ZIMOVETS I, et al. Sympathetic solar filament eruptions[J]. Astrophys. J., 2016, 827:L12
|
[68] |
LIU Y D, HU H D, WANG C, et al. On Sun-to-Earth propagation of coronal mass ejecctions:Ⅱ slow events and comparison with others[J]. Astrophys. J. Supp., 2016, 222:23
|
[69] |
WANG R, LIU Y D, WIEGELMANN T, et al. Relationship between sunspot rotation and a major solar eruption on 12 July 2012[J]. Solar Phys., 2016, 291:11591171
|
[70] |
HU H D, LIU Y D, WANG R, et al. Multi-spacecraft observations of the coronal and interplanetary evolution of a solar eruption associated with two active regions[J]. Astrophys. J., 2016, 840:76
|
[71] |
LIU Y D, ZHAO X W, ZHU B. Propagation and interaction properties of successive coronal mass ejections in relation to a complex type Ⅱ radio burst[J]. Astrophys J., 2017, 849:112
|
[72] |
LIU Y D, HU H D, ZHU B, et al. Structure, propagation, and expansion of a CME-driven shock in the heliosphere:A review of the 2012 July 23 extreme storm[J]. Astrophys J., 2017, 834:158
|
[73] |
ZHAO X W, LIU Y D, HU H D, et al. Propagation characteristics of two coronal mass ejections from the sun far into interplanetary space[J]. Astrophys. J., 2017, 837:4
|
[74] |
LIU Y A, LIU Y D, HU H D, et al. Multi-spacecraft observations of the rotation and nonradial motion of a CME flux rope causing an intense geomagnetic storm[J]. Astrophys. J., 2018, 854:126
|
[75] |
ZHAO X H, LIU Y D, INHESTER B, et al. Comparison of CME/shock propagation models with heliospheric imaging and in situ observations[J]. Astrophys J., 2016, 830:48
|
[76] |
ZHAO X H, FENG X S, FENG H Q, et al. Correlation between angular widths of CMEs and characteristics of their source regions[J]. Astrophys. J., 2017, 849:79
|
[77] |
XIONG M, DAVIES J A, HARRISON R A, et al. Prospective out-of-ecliptic white-light imaging of coronal mass ejections traveling through the corona and heliosphere[J]. Astrophys. J., 2018, 852:111
|
[78] |
WU S T, ZHOU Y F, JIANG C W, et al. A dataconstrained three-dimensional magnetohydrodynamic simulation model for a coronal mass ejection initiation[J]. J. Geophys. Res.:Space Phys., 2016, 121:1009-1023
|
[79] |
JIANG C W, FENG X S, WU S T. Analyses of the photospheric magnetic dynamics in solar active region 11117 using an advanced CESE-MHD model[J]. Front. Astron. Space Sci., 2016, 3:16
|
[80] |
JIANG C W, WU S T, FENG X S, et al. Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption[J]. Nature Commun., 2016, 7:11522
|
[81] |
ZHANG J K, LI H C.Two upstream splitting schemes for generalized Lagrange multiplier magnetohydrodynamics[J]. Chin. J. Space Sci., 2017, 37(1):8-18
|
[82] |
LIU Q, LI H C. Improvement and application of LaxFriderichs scheme in MHD numerical simulation[J]. Chin. J. Space Sci., 2016, 36(6):857-865
|
[83] |
XIONG M, DAVIES J A, LI B, et al. Prospective Out-ofecliptic white-light Imaging of interplanetary corotating interaction regions at solar maximum[J]. Astrophys. J., 2017, 844:76
|
[84] |
YANG Y, FENG X S, JIANG C W. A high-order CESE scheme with a new divergence-free method for MHD numerical simulation[J]. J. Comput. Phys., 2017, 349:561-581
|
[85] |
FENG X S, LI C X, XIANG C Q, et al. Data-driven modeling of the solar corona by a new three-dimensional path-conservative Osher-Solomon MHD model[J]. Astrophys. J. Supp. Ser., 2017, 233:10
|
[86] |
ZHOU Y F, FENG X S. Numerical study of the propagation characteristics of coronal mass ejections in a structured ambient solar wind[J]. J. Geophys. Res.:Space Phys., 2017, 122:1451-1462
|
[87] |
HAYASHI K, FENG X S, XIONG M, et al. An MHD simulation of solar active region 11158 driven with a timedependent electric field determined from HMI Vector magnetic field measurement data[J]. Astrophys. J., 2018, 855:11
|
[88] |
WANG W, WANG L, KRUCKER S, et al. Simulation of Quiet-Sun Hard X-Rays Related to Solar Wind Superhalo Electrons[J]. Solar Phys., 2016, 291(5):1357-1367
|
[89] |
QIN G, SHALCHI A. Numerical test of different approximation used in the transport theory of energetic particles[J]. Astrophys. J., 2016, 823:23
|
[90] |
WANG J F, QIN G, MA Q M, et al. Perpendicular diffusion coefficient of comic rays:the presence of weak adiabatic focusing[J]. Astrophys. J., 2017, 845:112
|
[91] |
WANG J F, QIN G, MA Q M, et al. Magnetic field line random walk in two-dimensional dynamical turbulence[J]. Phys. Plasmas, 2017, 24:082901
|
[92] |
QI S Y, QIN G, WANG Y. Numerical simulations of solar energetic particle event timescales associated with ICMES[J]. Res. Astron. Astrophys., 2017, 809(4):11-22
|
[93] |
KONG F J, QIN G, ZHANG L H. Numerical simulations of particle acceleration at interplanetary quasiperpendicular shocks[J]. Astrophys. J., 2017, 845:43
|
[94] |
SHEN Z N, QIN G. A study of cosmic ray flux based on the noise in raw CCD data from solar images[J]. J. Geophys. Res.:Space Phys., 2016, 121:10712-10727
|
[95] |
WU S S, QIN G. Model of energy spectrum parameters of ground level enhancement events in solar cycle 23[J]. J. Geophys. Res.:Space Phys., 2018, 123(1):76
|
[96] |
QIN G, SHEN Z N. Modulation of galactic cosmic rays in the inner heliosphere, comparing with PAMELA measurements[J]. Astrophys. J., 2017, 846:56
|
[97] |
LUO X, POTGIETER M S, ZHANG M, et al. A numerical simulation of cosmic ray modulation near the heliopause Ⅱ. Some physical insights[J]. Astrophys. J., 2016, 826:182
|
[98] |
LUO X, POTGIETER M S, ZHANG M, et al. A numerical study of forbush decreases with a 3D cosmic-ray modulation model based on an SDE approach[J]. Astrophys. J., 2017, 839:53
|