Citation: | ZHAO Xinhua, HE Jiansen, SHEN Chenglong, FENG Shiwei, JIANG Chaowei, LI Huichao, QIN Gang, LUO Xi. A Brief Review of Interplanetary Physics Research Progress in Mainland China during 2020–2022. Chinese Journal of Space Science, 2022, 42(4): 612-627 doi: 10.11728/cjss2022.04.yg19 |
[1] |
LI L P, PETER H, CHITTA L P, et al. Magnetic reconnection between loops accelerated by a nearby filament eruption[J]. The Astrophysical Journal, 2021, 908(2): 213 doi: 10.3847/1538-4357/abd47e
|
[2] |
HOU Z Y, TIAN H, CHEN H C, et al. Formation of solar quiescent coronal loops through magnetic reconnection in an emerging active region[J]. The Astrophysical Journal, 2021, 915(1): 39 doi: 10.3847/1538-4357/abff60
|
[3] |
CHEN H D, ZHANG J, DE PONTIEU B, et al. Coronal mini-jets in an activated solar tornado-like prominence[J]. The Astrophysical Journal, 2020, 899(1): 19 doi: 10.3847/1538-4357/ab9cad
|
[4] |
HOU Z Y, TIAN H, BERGHMANS D, et al. Coronal microjets in quiet-sun regions observed with the extreme ultraviolet imager on board the solar orbiter[J]. The Astrophysical Journal Letters, 2021, 918(1): L20 doi: 10.3847/2041-8213/ac1f30
|
[5] |
CHEN Y J, PRZYBYLSKI D, PETER H, et al. Transient small-scale brightenings in the quiet solar corona: a model for campfires observed with Solar Orbiter[J]. Astronomy & Astrophysics, 2021, 656: L7
|
[6] |
YANG Z H, BETHGE C, TIAN H, et al. Global maps of the magnetic field in the solar corona[J]. Science, 2020, 369(6504): 694-697 doi: 10.1126/science.abb4462
|
[7] |
YANG Z H, TIAN H, TOMCZYK S, et al. Mapping the magnetic field in the solar corona through magnetoseismology[J]. Science China Technological Sciences, 2020, 63(11): 2357-2368 doi: 10.1007/s11431-020-1706-9
|
[8] |
ZHU R, TAN B L, SU Y N, et al. Microwave diagnostics of magnetic field strengths in solar flaring loops[J]. Science China Technological Sciences, 2021, 64(1): 169-178 doi: 10.1007/s11431-020-1620-7
|
[9] |
CHEN Y J, LI W X, TIAN H, et al. Forward modeling of solar coronal magnetic-field measurements based on a magnetic-field-induced transition in Fe X[J]. The Astrophysical Journal, 2021, 920(2): 116 doi: 10.3847/1538-4357/ac1792
|
[10] |
ZHOU G P, GAO G N, WANG J X, et al. Magnetic reconnection invoked by sweeping of the CME-driven fast-mode shock[J]. The Astrophysical Journal, 2020, 905(2): 150 doi: 10.3847/1538-4357/abc5b2
|
[11] |
ZHOU X P, SHEN Y D, SU J T, et al. CME-driven and flare-ignited fast magnetosonic waves detected in a solar eruption[J]. Solar Physics, 2021, 296(11): 169 doi: 10.1007/s11207-021-01913-2
|
[12] |
ZHOU X P, SHEN Y D, TANG Z H, et al. Total reflection of a flare-driven quasi-periodic extreme ultraviolet wave train at a coronal hole boundary[J]. Astronomy & Astrophysics, 2022, 659: A164
|
[13] |
DUAN Y D, SHEN Y D, ZHOU X P, et al. Homologous accelerated electron beams, a quasiperiodic fast-propagating wave, and a coronal mass ejection observed in one fan-spine jet[J]. The Astrophysical Journal Letters, 2022, 926(2): L39 doi: 10.3847/2041-8213/ac4df2
|
[14] |
HOU Z Y, TIAN H, WANG J S, et al. Three-dimensional propagation of the global extreme-ultraviolet Wave associated with a solar eruption on 2021 October 28[J]. The Astrophysical Journal, 2022, 928(2): 98 doi: 10.3847/1538-4357/ac590d
|
[15] |
ZHANG Q M, DAI J, XU Z, et al. Transverse coronal loop oscillations excited by homologous circular-ribbon flares[J]. Astronomy & Astrophysics, 2020, 638: A32
|
[16] |
ZHANG Q M. Simultaneous transverse oscillations of a coronal loop and a filament excited by a circular-ribbon flare[J]. Astronomy & Astrophysics, 2020, 642: A159
|
[17] |
ZHANG Q M, CHEN J L, LI S T, et al. Transverse coronal-loop oscillations induced by the non-radial eruption of a magnetic flux rope[J]. Solar Physics, 2022, 297(2): 18 doi: 10.1007/s11207-022-01952-3
|
[18] |
XUE J C, SU Y, LI H, et al. Thermodynamical evolution of supra-arcade downflows[J]. The Astrophysical Journal, 2020, 898(1): 88 doi: 10.3847/1538-4357/ab9a3d
|
[19] |
LI Z F, CHENG X, DING M D, et al. Thermodynamic evolution of solar flare supra-arcade downflows[J]. The Astrophysical Journal, 2021, 915(2): 124 doi: 10.3847/1538-4357/ac043e
|
[20] |
SAMANTA T, TIAN H, CHEN B, et al. Plasma heating induced by tadpole-like downflows in the flaring solar corona[J]. The Innovation, 2021, 2(1): 100083 doi: 10.1016/j.xinn.2021.100083
|
[21] |
LI L P, PETER H, CHITTA L P, et al. Relation of coronal rain originating from coronal condensations to interchange magnetic reconnection[J]. The Astrophysical Journal, 2020, 905(1): 26 doi: 10.3847/1538-4357/abc68c
|
[22] |
LI L P, PETER H, CHITTA L P, et al. On-disk solar coronal condensations facilitated by magnetic reconnection between open and closed magnetic structures[J]. The Astrophysical Journal, 2021, 910(2): 82 doi: 10.3847/1538-4357/abe537
|
[23] |
LI L P, PETER H, CHITTA L P, et al. Revisiting the formation mechanism for coronal rain from previous studies[J]. Research in Astronomy and Astrophysics, 2021, 21(10): 255 doi: 10.1088/1674-4527/21/10/255
|
[24] |
LI L P, PETER H, CHITTA L P, et al. Formation of a solar filament by magnetic reconnection and coronal condensation[J]. The Astrophysical Journal Letters, 2021, 919: L21 doi: 10.3847/2041-8213/ac257f
|
[25] |
YANG B, YANG J Y, BI Y, et al. Formation of a solar filament by magnetic reconnection, associated chromospheric evaporation, and subsequent coronal condensation[J]. The Astrophysical Journal Letters, 2021, 921(2): L33 doi: 10.3847/2041-8213/ac31b6
|
[26] |
CHEN H C, TIAN H, LI L P, et al. Coronal condensation as the source of transition-region supersonic downflows above a sunspot[J]. Astronomy & Astrophysics, 2022, 659: A107
|
[27] |
DUAN D, HE J S, WU H H, et al. Magnetic energy transfer and distribution between protons and electrons for alfvénic waves at kinetic scales in wavenumber space[J]. The Astrophysical Journal, 2020, 896(1): 47 doi: 10.3847/1538-4357/ab8ad2
|
[28] |
DUAN D, HE J S, BOWEN T A, et al. Anisotropy of solar wind turbulence in the inner heliosphere at kinetic scales: PSP observations[J]. The Astrophysical Journal Letters, 2021, 915(1): L8 doi: 10.3847/2041-8213/ac07ac
|
[29] |
ZHANG J, HUANG S Y, HE J S, et al. Three-dimensional anisotropy and scaling properties of solar wind turbulence at kinetic scales in the inner heliosphere: Parker solar probe observations[J]. The Astrophysical Journal Letters, 2022, 924(2): L21 doi: 10.3847/2041-8213/ac4027
|
[30] |
HUANG S Y, ZHANG J, SAHRAOUI F, et al. Kinetic scale slow solar wind turbulence in the inner heliosphere: coexistence of kinetic alfvén waves and alfvén ion cyclotron waves[J]. The Astrophysical Journal Letters, 2020, 897(1): L3 doi: 10.3847/2041-8213/ab9abb
|
[31] |
ZHU X Y, HE J S, VERSCHAREN D, et al. Wave composition, propagation, and polarization of magnetohydrodynamic turbulence within 0.3 au as observed by parker solar probe[J]. The Astrophysical Journal Letters, 2020, 901(1): L3 doi: 10.3847/2041-8213/abb23e
|
[32] |
ZHAO G Q, LIN Y, WANG X Y, et al. Two correlations with enhancement near the proton gyroradius scale in solar wind turbulence: parker solar probe (PSP) and wind observations[J]. The Astrophysical Journal, 2022, 924(2): 92 doi: 10.3847/1538-4357/ac3747
|
[33] |
WU H H, TU C Y, WANG X, et al. Energy supply for heating the slow solar wind observed by parker solar probe between 0.17 and 0.7 au[J]. The Astrophysical Journal Letters, 2020, 904(1): L8 doi: 10.3847/2041-8213/abc5b6
|
[34] |
WU H H, TU C Y, HE J S, et al. Consistency of von Karman decay rate with the energy supply rate and heating rate observed by parker solar probe[J]. The Astrophysical Journal, 2022, 926(2): 116 doi: 10.3847/1538-4357/ac4413
|
[35] |
HE J S, ZHU X Y, YANG L P, et al. Solar origin of compressive alfvénic spikes/kinks as observed by parker solar probe[J]. The Astrophysical Journal Letters, 2021, 913(1): L14 doi: 10.3847/2041-8213/abf83d
|
[36] |
WU H H, TU C Y, WANG X, et al. Large amplitude switchback turbulence: possible magnetic velocity alignment structures[J]. The Astrophysical Journal, 2021, 911(2): 73 doi: 10.3847/1538-4357/abec6c
|
[37] |
WU H H, TU C Y, WANG X, et al. Magnetic and velocity fluctuations in the near-sun region from 0.1-0.3 au observed by parker solar probe[J]. The Astrophysical Journal, 2021, 922(2): 92 doi: 10.3847/1538-4357/ac3331
|
[38] |
SHI C, ZHAO J S, HUANG J, et al. Parker solar probe observations of alfvénic waves and ion-cyclotron waves in a small-scale flux rope[J]. The Astrophysical Journal Letters, 2021, 908(1): L19 doi: 10.3847/2041-8213/abdd28
|
[39] |
LIU Y Y, FU H S, CAO J B, et al. Characteristics of interplanetary discontinuities in the inner heliosphere revealed by parker solar probe[J]. The Astrophysical Journal, 2021, 916(2): 65 doi: 10.3847/1538-4357/ac06a1
|
[40] |
YU L, HUANG S Y, YUAN Z G, et al. Characteristics of magnetic holes in the solar wind revealed by parker solar probe[J]. The Astrophysical Journal, 2021, 908(1): 56 doi: 10.3847/1538-4357/abb9a8
|
[41] |
SHI C, ZHAO J S, MALASPINA D M, et al. Multiband electrostatic waves below and above the electron cyclotron frequency in the near-sun solar wind[J]. The Astrophysical Journal Letters, 2022, 926(1): L3 doi: 10.3847/2041-8213/ac4d37
|
[42] |
CHEN L, MA B, WU D J, et al. An interplanetary type IIIb radio burst observed by parker solar probe and its emission mechanism[J]. The Astrophysical Journal Letters, 2021, 915(1): L22 doi: 10.3847/2041-8213/ac0b43
|
[43] |
HUANG S Y, WANG Q Y, SAHRAOUI F, et al. Analysis of turbulence properties in the mercury plasma environment using MESSENGER observations[J]. The Astrophysical Journal, 2020, 891(2): 159 doi: 10.3847/1538-4357/ab7349
|
[44] |
WU H H, TU C Y, WANG X, et al. Energy supply by low-frequency break sweeping for heating the fast solar wind from 0.3 to 4.8 au[J]. The Astrophysical Journal, 2021, 912: 84 doi: 10.3847/1538-4357/abf099
|
[45] |
WU H H, TU C Y, HE J S, et al. The yaglom scaling of the third-order structure functions in the inner heliosphere observed by Helios 1 and 2[J]. The Astrophysical Journal, 2022, 927(1): 113 doi: 10.3847/1538-4357/ac4fcc
|
[46] |
LIU D, RONG Z J, GAO J W, et al. Statistical properties of solar wind upstream of mars: maven observations[J]. The Astrophysical Journal, 2021, 911(2): 113 doi: 10.3847/1538-4357/abed50
|
[47] |
YAO S T, SHI Q Q, ZONG Q G, et al. Low-frequency whistler waves modulate electrons and generate higher-frequency whistler waves in the solar wind[J]. The Astrophysical Journal, 2021, 923(2): 216 doi: 10.3847/1538-4357/ac2e97
|
[48] |
WU H H, TU C Y, WANG X, et al. Isotropic scaling features measured locally in the solar wind turbulence with stationary background field[J]. The Astrophysical Journal, 2020, 892(2): 138 doi: 10.3847/1538-4357/ab7b72
|
[49] |
WANG X, TU C Y, HE J S. Fluctuation amplitudes of magnetic-field directional turnings and magnetic-velocity alignment structures in the solar wind[J]. The Astrophysical Journal, 2020, 903(1): 72 doi: 10.3847/1538-4357/abb883
|
[50] |
ZHAO G Q, FENG H Q, WU D J, et al. Dependence of ion temperatures on alpha–proton differential flow vector and heating mechanisms in the solar wind[J]. The Astrophysical Journal Letters, 2020, 889(1): L14 doi: 10.3847/2041-8213/ab6b29
|
[51] |
ZHAO G Q, LIN Y, WANG X Y, et al. Magnetic helicity signature and its role in regulating magnetic energy spectra and proton temperatures in the solar wind[J]. The Astrophysical Journal, 2021, 906: 123 doi: 10.3847/1538-4357/abca3b
|
[52] |
ZHAO G Q, FENG H Q, WU D J, et al. On mechanisms of proton perpendicular heating in the solar wind: test results based on wind observations[J]. Research in Astronomy and Astrophysics, 2022, 22(1): 015009 doi: 10.1088/1674-4527/ac3413
|
[53] |
HE J S, ZHU X Y, VERSCHAREN D, et al. Spectra of diffusion, dispersion, and dissipation for kinetic alfvénic and compressive turbulence: Comparison between kinetic theory and measurements from mms[J]. The Astrophysical Journal, 2020, 898(1): 43 doi: 10.3847/1538-4357/ab9174
|
[54] |
HOU C P, HE J S, ZHU X Y, et al. Contribution of magnetic reconnection events to energy dissipation in space plasma turbulence[J]. The Astrophysical Journal, 2021, 908(2): 237 doi: 10.3847/1538-4357/abd6f3
|
[55] |
LUO Q W, HE J S, CUI J, et al. Energy conversion between ions and electrons through ion cyclotron waves and embedded ion-scale rotational discontinuity in collisionless space plasmas[J]. The Astrophysical Journal Letters, 2020, 904(2): L16 doi: 10.3847/2041-8213/abc75a
|
[56] |
WANG T Y, HE J S, ALEXANDROVA O, et al. Observational quantification of three-dimensional anisotropies and scalings of space plasma turbulence at kinetic scales[J]. The Astrophysical Journal, 2020, 898(1): 91 doi: 10.3847/1538-4357/ab99ca
|
[57] |
ZHU X Y, HE J S, WANG Y, et al. Difference of intermittency between electric field and magnetic field fluctuations from ion scale down to sub-electron scale in the magnetosheath turbulence[J]. The Astrophysical Journal, 2020, 893(2): 124 doi: 10.3847/1538-4357/ab7815
|
[58] |
YANG Z W, LIU Y D, MATSUKIYO S, et al. PIC simulations of microinstabilities and waves at near-sun solar wind perpendicular shocks: predictions for parker solar probe and solar orbiter[J]. The Astrophysical Journal Letters, 2020, 900(2): L24 doi: 10.3847/2041-8213/abaf59
|
[59] |
LIU Y C M, QI Z H, HUANG J, et al. Unusually low density regions in the compressed slow wind: solar wind transients of small coronal hole origin[J]. Astronomy & Astrophysics, 2020, 635: A49
|
[60] |
CHEN C, LIU Y D, HU H D. Macro magnetic holes caused by ripples in Heliospheric current sheet from coordinated imaging and parker solar probe observations[J]. The Astrophysical Journal, 2021, 921(1): 15 doi: 10.3847/1538-4357/ac1b2b
|
[61] |
LIU Y D, CHEN C, STEVENS M L, et al. Determination of solar wind angular momentum and Alfvén radius from Parker Solar Probe observations[J]. The Astrophysical Journal Letters, 2021, 908(2): L41 doi: 10.3847/2041-8213/abe38e
|
[62] |
QI Z H, LIU Y, LIU R Y. The small coronal hole solar wind and Alfvén wave within the slow solar wind[J]. Chinese Journal of Geophysics, 2021, 64(11): 3837-3845
|
[63] |
LIU R Y, LIU Y C M, HUANG J, et al. Density compressions at magnetic switchbacks associated with fast plasma: a superposed epoch analysis[J]. Journal of Geophysical Research: Space Physics, 2022, 127(5): e2022JA030382
|
[64] |
MENG M M, LIU Y D, CHEN C, et al. Analysis of the distribution, rotation and scale characteristics of solar wind switchbacks: comparison between the first and second encounters of parker solar probe[J]. Research in Astronomy and Astrophysics, 2022, 22(3): 035018 doi: 10.1088/1674-4527/ac49e4
|
[65] |
LI X L, WANG Y M, LIU R, et al. Reconstructing solar wind inhomogeneous structures from stereoscopic observations in white light: Solar wind transients in 3-D[J]. Journal of Geophysical Research: Space Physics, 2020, 125(7): e2019JA027513 doi: 10.1029/2019JA027513
|
[66] |
LYU S Y, WANG Y M, LI X L, et al. Three-dimensional reconstruction of coronal mass ejections by the correlation-aided reconstruction technique through different stereoscopic angles of the solar terrestrial relations observatory twin spacecraft[J]. The Astrophysical Journal, 2021, 909(2): 182 doi: 10.3847/1538-4357/abd9c9
|
[67] |
LI X L, WANG Y M, GUO J N, et al. Radial velocity map of solar wind transients in the field of view of STEREO/HI1 on 3 and 4 April 2010[J]. Astronomy & Astrophysics, 2021, 649: A58
|
[68] |
SHEN C L, CHI Y T, XU M J, et al. Origin of extremely intense southward component of magnetic field (Bs) in ICMEs[J]. Frontiers in Physics, 2021, 9: 762488 doi: 10.3389/fphy.2021.762488
|
[69] |
LIU Y D, CHEN C, ZHAO X W. Characteristics and importance of “ICME-in-sheath” phenomenon and upper limit for geomagnetic storm activity[J]. The Astrophysical Journal Letters, 2020, 897(1): L11 doi: 10.3847/2041-8213/ab9d25
|
[70] |
SONG H Q, ZHANG J, CHENG X, et al. Do all interplanetary coronal mass ejections have a magnetic flux rope structure near 1 AU[J]. The Astrophysical Journal Letters, 2020, 901(2): L21 doi: 10.3847/2041-8213/abb6ec
|
[71] |
ZHAO Y, FENG H Q, LIU Q, et al. The flux of flux ropes embedded within magnetic clouds near 5 AU[J]. Journal of Geophysical Research: Space Physics, 2021, 126(8): e2020JA028594 doi: 10.1029/2020JA028594
|
[72] |
SONG H Q, LI L P, SUN Y Y, et al. Solar cycle dependence of ICME composition[J]. Solar Physics, 2021, 296(7): 111 doi: 10.1007/s11207-021-01852-y
|
[73] |
HUANG J, LIU Y, FENG H Q, et al. A statistical study of the plasma and composition distribution inside magnetic clouds: 1998-2011[J]. The Astrophysical Journal, 2020, 893(2): 136 doi: 10.3847/1538-4357/ab7a28
|
[74] |
SONG H Q, CHENG X, LI L P, et al. Comparison of helium abundance between ICMEs and solar wind near 1 AU[J]. The Astrophysical Journal, 2022, 925(2): 137 doi: 10.3847/1538-4357/ac3bbf
|
[75] |
WANG C, XU M J, SHEN C L, et al. Interplanetary shock candidates observed at Venus’s orbit[J]. The Astrophysical Journal, 2021, 912(2): 85 doi: 10.3847/1538-4357/abee7b
|
[76] |
ZHAO D, GUO J P, HUANG H, et al. Interplanetary coronal mass ejections from MAVEN orbital observations at mars[J]. The Astrophysical Journal, 2021, 923(1): 4 doi: 10.3847/1538-4357/ac294b
|
[77] |
HUANG H, GUO J P, MAZELLE C, et al. Properties of interplanetary fast shocks close to the Martian environment[J]. The Astrophysical Journal, 2021, 914(1): 14 doi: 10.3847/1538-4357/abf82b
|
[78] |
CHI Y T, SCOTT C, SHEN C L, et al. Using the “ghost front” to predict the arrival time and speed of CMEs at Venus and Earth[J]. The Astrophysical Journal, 2020, 899(2): 143 doi: 10.3847/1538-4357/aba95a
|
[79] |
XU M J, SHEN C L, WANG C, et al. Multipoint analysis of the interaction between a shock and an ICME-like structure around 2011 March 22[J]. The Astrophysical Journal Letters, 2022, 930(1): L11 doi: 10.3847/2041-8213/ac6879
|
[80] |
XU M J, SHEN C L, HU Q, et al. Whether small flux ropes and magnetic clouds have the same origin: a statistical study of small flux ropes in different types of solar wind[J]. The Astrophysical Journal, 2020, 904(2): 122 doi: 10.3847/1538-4357/abbe21
|
[81] |
FENG H Q, ZHAO Y, WANG J M, et al. Observations of magnetic flux ropes opened or disconnected from the Sun by magnetic reconnection in interplanetary space[J]. Frontiers in Physics, 2021, 9: 679780 doi: 10.3389/fphy.2021.679780
|
[82] |
NING H, CHEN Y, NI S L, et al. Harmonic maser emissions from electrons with loss-cone distribution in solar active regions[J]. The Astrophysical Journal Letters, 2021, 920: L40 doi: 10.3847/2041-8213/ac2cc6
|
[83] |
NING H, CHEN Y, NI S L, et al. Harmonic electron-cyclotron maser emissions driven by energetic electrons of the horseshoe distribution with application to solar radio spikes[J]. Astronomy & Astrophysics, 2021, 651: A118
|
[84] |
LI C Y, CHEN Y, NI S L, et al. PIC simulation of double plasma resonance and zebra pattern of solar radio bursts[J]. The Astrophysical Journal Letters, 2021, 909(1): L5 doi: 10.3847/2041-8213/abe708
|
[85] |
NI S L, CHEN Y, LI C Y, et al. Plasma emission induced by electron cyclotron maser instability in solar plasmas with a large ratio of plasma frequency to gyrofrequency[J]. The Astrophysical Journal Letters, 2020, 891(1): L25 doi: 10.3847/2041-8213/ab7750
|
[86] |
LI T M, LI C, CHEN P F, et al. Particle-in-cell simulation of plasma emission in solar radio bursts[J]. Astronomy & Astrophysics, 2021, 653: A169
|
[87] |
FENG Shiwei, LÜ Maoshui. Recent observational studies on the fine structures of solar type II radio bursts[J]. Progress in Astronomy, 2021, 39(2): 129-143
|
[88] |
FENG Shiwei, ZHAO Fei. Observational study on the fine structures of solar type III radio bursts[J]. Scientia Sinica Technologica, 2021, 51(1): 35-45 doi: 10.1360/SST-2020-0066
|
[89] |
GAO G N, CAI Q W, GUO S J, et al. Decimetric type-U solar radio bursts and associated EUV phenomena on 2011 February 9[J]. The Astrophysical Journal, 2021, 923(2): 286
|
[90] |
WAN J L, TANG J F, TAN B L, et al. Statistical analysis of solar radio fiber bursts and relations with flares[J]. Astronomy & Astrophysics, 2021, 653: A38
|
[91] |
TANG J F, WU D J, WAN J L, et al. Evolvement of microwave spike bursts in a solar flare on 2006 December 13[J]. Research in Astronomy and Astrophysics, 2021, 21(6): 148 doi: 10.1088/1674-4527/21/6/148
|
[92] |
ZHANG M H, ZHANG Y, YAN Y H, et al. Observational results of MUSER during 2014-2019[J]. Research in Astronomy and Astrophysics, 2021, 21(11): 284 doi: 10.1088/1674-4527/21/11/284
|
[93] |
LU L, LI D, NING Z J, et al. Quasi-periodic pulsations detected in Ly α and nonthermal emissions during solar flares[J]. Solar Physics, 2021, 296(8): 130 doi: 10.1007/s11207-021-01876-4
|
[94] |
HONG Z X, LI D, ZHANG M H, et al. Multi-wavelength observations of quasi-periodic pulsations in a solar flare[J]. Solar Physics, 2021, 296(11): 171 doi: 10.1007/s11207-021-01922-1
|
[95] |
LÜ M S, CHEN Y, VASANTH V, et al. An observational revisit of stationary type IV solar radio bursts[J]. Solar Physics, 2021, 296(2): 38 doi: 10.1007/s11207-021-01769-6
|
[96] |
ZHANG P J, WANG C B, KONTAR E P. Parametric simulation studies on the wave propagation of solar radio emission: the source size, duration, and position[J]. The Astrophysical Journal, 2021, 909(2): 195 doi: 10.3847/1538-4357/abd8c5
|
[97] |
JIANG C W, FENG X S, LIU R, et al. A fundamental mechanism of solar eruption initiation[J]. Nature Astronomy, 2021, 5(11): 1126-1138 doi: 10.1038/s41550-021-01414-z
|
[98] |
BIAN X K, JIANG C W, FENG X S, et al. Numerical simulation of a fundamental mechanism of solar eruption with a range of magnetic flux distributions[J]. Astronomy & Astrophysics, 2022, 658: A174
|
[99] |
BIAN X K, JIANG C W, FENG X S, et al. Homologous coronal mass ejections caused by recurring formation and disruption of current sheet within a sheared magnetic arcade[J]. The Astrophysical Journal Letters, 2022, 925(1): L7 doi: 10.3847/2041-8213/ac4980
|
[100] |
JIANG C W, CHEN J, DUAN A Y, et al. Formation of magnetic flux rope during solar eruption. I. Evolution of toroidal flux and reconnection flux[J]. Frontiers in Physics, 2021, 9: 575 doi: 10.3389/fphy.2021.746576
|
[101] |
XING C, CHENG X, DING M D. Evolution of the toroidal flux of CME flux ropes during eruption[J]. The Innovation, 2020, 1(3): 100059 doi: 10.1016/j.xinn.2020.100059
|
[102] |
WANG J T, JIANG C W, YUAN D, et al. The causes of peripheral coronal loop contraction and disappearance revealed in a magnetohydrodynamic simulation of solar eruption[J]. The Astrophysical Journal, 2021, 911(1): 2 doi: 10.3847/1538-4357/abe637
|
[103] |
HUDSON H S. Global properties of solar flares[J]. Space Science Reviews, 2011, 158(1): 5-41 doi: 10.1007/s11214-010-9721-4
|
[104] |
ZHOU Z J, JIANG C W, LIU R, et al. The rotation of magnetic flux ropes formed during solar eruption[J]. The Astrophysical Journal Letters, 2022, 927(1): L14 doi: 10.3847/2041-8213/ac5740
|
[105] |
YE J, SHEN C, LIN J, et al. An efficient parallel semi-implicit solver for anisotropic thermal conduction in the solar corona[J]. Astronomy and Computing, 2020, 30: 100341 doi: 10.1016/j.ascom.2019.100341
|
[106] |
YE J, CAI Q W, SHEN C C, et al. The role of turbulence for heating plasmas in eruptive solar flares[J]. The Astrophysical Journal, 2020, 897(1): 64 doi: 10.3847/1538-4357/ab93b5
|
[107] |
YE J, CAI Q W, SHEN C C, et al. Coronal wave trains and plasma heating triggered by turbulence in the wake of a CME[J]. The Astrophysical Journal, 2021, 909(1): 45 doi: 10.3847/1538-4357/abdeb5
|
[108] |
XIE X Y, MEI Z X, SHEN C C, et al. Numerical experiments on dynamic evolution of a CME-flare current sheet[J]. Monthly Notices of the Royal Astronomical Society, 2022, 509(1): 406-420
|
[109] |
MEI Z X, KEPPENS R, CAI Q W, et al. The triple-layered leading edge of solar coronal mass ejections[J]. The Astrophysical Journal Letters, 2020, 898(1): L21 doi: 10.3847/2041-8213/aba2ce
|
[110] |
MEI Z X, KEPPENS R, CAI Q W, et al. 3 D numerical experiment for EUV waves caused by flux rope eruption[J]. Monthly Notices of the Royal Astronomical Society, 2020, 493(4): 4816-4829 doi: 10.1093/mnras/staa555
|
[111] |
MEI Z X, CAI Q W, YE J, et al. Velocity distribution associated with EUV disturbances caused by eruptive MFR[J]. Frontiers in Astronomy and Space Science, 2021, 8: 771882 doi: 10.3389/fspas.2021.771882
|
[112] |
JIANG C W, BIAN X K, SUN T T, et al. MHD modeling of solar coronal magnetic evolution driven by photospheric flow[J]. Frontiers in Physics, 2021, 9: 646750 doi: 10.3389/fphy.2021.646750
|
[113] |
JIANG C W, TORIUMI S. Testing a data-driven active region evolution model with boundary data at different heights from a solar magnetic flux emergence simulation[J]. The Astrophysical Journal, 2020, 903(1): 11 doi: 10.3847/1538-4357/abb5ac
|
[114] |
TORIUMI S, TAKASAO S, CHEUNG M C M, et al. Comparative study of data-driven solar coronal field models using a flux emergence simulation as a ground-truth data set[J]. The Astrophysical Journal, 2020, 890(2): 103 doi: 10.3847/1538-4357/ab6b1f
|
[115] |
HE W, JIANG C W, ZOU P, et al. Data-driven MHD simulation of the formation and initiation of a large-scale preflare magnetic flux rope in AR 12371[J]. The Astrophysical Journal, 2020, 892(1): 9 doi: 10.3847/1538-4357/ab75ab
|
[116] |
ZHONG Z, GUO Y, DING M D. The role of non-axisymmetry of magnetic flux rope in constraining solar eruptions[J]. Nature Communications, 2021, 12(1): 2734 doi: 10.1038/s41467-021-23037-8
|
[117] |
GUO Y, ZHONG Z, DING M D, et al. Data-constrained magnetohydrodynamic simulation of a long-duration eruptive flare[J]. The Astrophysical Journal, 2021, 919(1): 39 doi: 10.3847/1538-4357/ac10c8
|
[118] |
YAN X L, XUE Z K, JIANG C W, et al. Fast plasmoid-mediated reconnection in a solar flare[J]. Nature Communication 2022, 13: 640
|
[119] |
FENG X S, WANG H P, XIANG C Q, et al. Magnetohydrodynamic modeling of the solar corona with an effective implicit strategy[J]. The Astrophysical Journal Supplement Series, 2021, 257(2): 34 doi: 10.3847/1538-4365/ac1f8b
|
[120] |
LI C X, FENG X S, LI H C, et al. Modified path-conservative HLLEM scheme for magnetohydrodynamic solar wind simulations[J]. The Astrophysical Journal Supplement Series, 2021, 253(1): 24 doi: 10.3847/1538-4365/abd5ab
|
[121] |
LI C X, FENG X S, WEI F S. An entropy-stable ideal EC-GLM-MHD model for the simulation of the three-dimensional ambient solar wind[J]. The Astrophysical Journal Supplement Series, 2021, 257(2): 24 doi: 10.3847/1538-4365/ac16d5
|
[122] |
LIU C, SHEN F, LIU Y S, et al. Numerical study of divergence cleaning and coronal heating/acceleration methods in the 3 D COIN-TVD MHD model[J]. Frontiers in Physics, 2021, 9: 705744 doi: 10.3389/fphy.2021.705744
|
[123] |
LI H C, FENG X S, WEI F S. Comparison of synoptic maps and PFSS solutions for the declining phase of solar cycle 24[J]. Journal of Geophysical Research: Space Physics, 2021, 126(3): e2020JA028870
|
[124] |
YANG Y, SHEN F. Three-dimensional MHD modeling of interplanetary solar wind using self-consistent boundary condition obtained from multiple observations and machine learning[J]. Universe, 2021, 7(10): 371 doi: 10.3390/universe7100371
|
[125] |
LI H C, FENG X S, WEI F S. Assessment of CESE-HLLD ambient solar wind model results using multipoint observation[J]. Journal of Space Weather and Space Climate, 2020, 10: 44 doi: 10.1051/swsc/2020048
|
[126] |
LI H C, FENG X S, ZUO P B, et al. Simulation of the interplanetary Bz using a data-driven heliospheric solar wind model[J]. The Astrophysical Journal, 2020, 900(1): 76 doi: 10.3847/1538-4357/aba61f
|
[127] |
SHEN F, LIU Y S, YANG Y. Numerical research on the effect of the initial parameters of a CME flux-rope model on simulation results. II. Different locations of observers[J]. The Astrophysical Journal, 2021, 915(1): 30 doi: 10.3847/1538-4357/ac004e
|
[128] |
SHEN F, LIU Y S, YANG Y. Numerical research on the effect of the initial parameters of a CME flux-rope model on simulation results[J]. The Astrophysical Journal Supplement Series, 2021, 253(1): 12 doi: 10.3847/1538-4365/abd4d2
|
[129] |
ZHANG M, FENG X S, SHEN F, et al. Numerical study of two injection methods for the 2007 November 15 coronal mass ejection in the inner heliosphere[J]. The Astrophysical Journal, 2021, 918(1): 35 doi: 10.3847/1538-4357/ac0b3f
|
[130] |
YANG L P, WANG H P, FENG X S, et al. Numerical MHD simulations of the 3 D morphology and kinematics of the 2017 September 10 CME-driven shock from the sun to earth[J]. The Astrophysical Journal, 2021, 918(1): 31 doi: 10.3847/1538-4357/ac0ef7
|
[131] |
LIU Z X, WANG L H, WIMMER-SCHWEINGRUBER R F, et al. Pan-spectrum fitting formula for suprathermal particles[J]. Journal of Geophysical Research: Space Physics, 2020, 125(12): e2020JA028702 doi: 10.1029/2020JA028702
|
[132] |
WANG W, WANG L H, KRUCKER S, et al. Solar energetic electron events associated with hard X-ray flares[J]. The Astrophysical Journal, 2021, 913(2): 89 doi: 10.3847/1538-4357/abefce
|
[133] |
WANG L H, ZONG Q G, SHI Q Q, et al. Solar energetic electrons entering the Earth’s cusp/lobe[J]. The Astrophysical Journal, 2021, 910(1): 12 doi: 10.3847/1538-4357/abdb2b
|
[134] |
KONG F J, QIN G. Suprathermal electron acceleration by a quasi-perpendicular shock: Simulations and observations[J]. The Astrophysical Journal, 2020, 896(1): 20 doi: 10.3847/1538-4357/ab8e32
|
[135] |
WANG Y, LYU D, XIAO B X, et al. Statistical survey of reservoir phenomenon in energetic proton events observed by multiple spacecraft[J]. The Astrophysical Journal, 2021, 909(2): 110 doi: 10.3847/1538-4357/abda39
|
[136] |
WANG Y, LYU D, QIN G, et al. The effects of magnetic boundary on the uniform distribution of energetic particle intensities observed by multiple spacecraft[J]. The Astrophysical Journal, 2021, 913(1): 66 doi: 10.3847/1538-4357/abf9a4
|
[137] |
WU S S, QIN G. Magnetic cloud and sheath in the ground-level enhancement event of 2000 July 14. I. Effects on the solar energetic particles[J]. The Astrophysical Journal, 2020, 904(2): 151 doi: 10.3847/1538-4357/abc0f2
|
[138] |
QIN G, WU S S. Magnetic cloud and sheath in the ground-level enhancement event of 2000 July 14. II. Effects on the forbush decrease[J]. The Astrophysical Journal, 2021, 908(2): 236 doi: 10.3847/1538-4357/abd77c
|
[139] |
WANG J F, QIN G. The invariance of the diffusion coefficient with iterative operations of the charged particle transport equation[J]. The Astrophysical Journal, 2020, 899(1): 39 doi: 10.3847/1538-4357/aba3c8
|
[140] |
WANG J F, QIN G. Study of momentum diffusion with the effect of adiabatic focusing[J]. The Astrophysical Journal Supplement Series, 2021, 257: 44 doi: 10.3847/1538-4365/ac1bb3
|
[141] |
LUO X, ZHANG M, FENG X S, et al. A numerical study of the effects of corotating interaction regions on cosmic-ray transport[J]. The Astrophysical Journal, 2020, 899(2): 90 doi: 10.3847/1538-4357/aba7b5
|
[142] |
SONG X J, LUO X, POTGIETER M S, et al. A numerical study of the solar modulation of galactic protons and helium from 2006 to 2017[J]. The Astrophysical Journal Supplement Series, 2021, 257(2): 48 doi: 10.3847/1538-4365/ac281c
|
[143] |
SHEN Z N, QIN G, ZUO P B, et al. A study of variations of galactic cosmic-ray intensity based on a hybrid data-processing method[J]. The Astrophysical Journal, 2020, 900(2): 143 doi: 10.3847/1538-4357/abac60
|
[144] |
SHEN Z N, QIN G, ZUO P B, et al. Numerical modeling of latitudinal gradients for galactic cosmic-ray protons during solar minima: comparing with Ulysses observations[J]. The Astrophysical Journal Supplement Series, 2021, 256(1): 18 doi: 10.3847/1538-4365/ac0a78
|
[145] |
SHEN Z N, YANG H, ZUO P B, et al. Solar modulation of galactic cosmic-ray protons based on a modified force-field approach[J]. The Astrophysical Journal, 2021, 921(2): 109 doi: 10.3847/1538-4357/ac1fe8
|
[146] |
ZHU B, LIU Y D, KWON R Y, et al. Shock properties and associated characteristics of solar energetic particles in the 2017 September 10 ground-level enhancement event[J]. The Astrophysical Journal, 2021, 921(1): 26 doi: 10.3847/1538-4357/ac106b
|