火星上游拾起离子激发质子回旋波的研究

[1] Langlais B, Purucker M, Mandea M. Crustal magnetic field of Mars[J]. Journal of GeophysicalResearch: Planets, 2004, 109(E2).
[2] Usui T, Bajo K i, Fujiya W, et al. The importance of Phobos sample return for understandingthe Mars-moon system[J]. Space Science Reviews, 2020, 216: 1-18.
[3] Jakosky B M, Lin R P, Grebowsky J M, et al. The Mars atmosphere and volatile evolution(MAVEN) mission[J]. Space Science Reviews, 2015, 195: 3-48.
[4] Chicarro A, Martin P, Trautner R. The Mars Express mission: an overview[J]. Mars Express:the scientific payload, 2004, 1240: 3-13.
[5] Zou Y, Zhu Y, Bai Y, et al. Scientific objectives and payloads of Tianwen-1, China’s first Marsexploration mission[J]. Advances in Space Research, 2021, 67(2): 812-823.
[6] Chassefiere E, Leblanc F. Mars atmospheric escape and evolution; interaction with the solarwind[J]. Planetary & Space Science, 2004, 52(11): 1039-1058.
[7] Jakosky B M, Slipski M, Benna M, et al. Mars’ atmospheric history derived from upperatmosphere measurements of 38Ar/36Ar[J]. Science, 2017, 355(6332): 1408-1410.
[8] Kurokawa H, Kurosawa K, Usui T. A lower limit of atmospheric pressure on early Mars inferredfrom nitrogen and argon isotopic compositions[J]. Icarus, 2017, 299: 443-459.
[9] Hunten D, McElroy M. Production and escape of hydrogen on Mars[J]. Journal of GeophysicalResearch, 1970, 75(31): 5989-6001.
[10] Cravens T E, Hamil O, Houston S, et al. Estimates of ionospheric transport and ion loss atMars[J]. Journal of Geophysical Research: Space Physics, 2017, 122(10): 10-626.
[11] Dong Y, Fang X, Brain D, et al. Seasonal variability of Martian ion escape through the plumeand tail from MAVEN observations[J]. Journal of Geophysical Research: Space Physics, 2017,122(4): 4009-4022.
[12] Johnson B C, Liemohn M W, Frnz M, et al. Influence of the interplanetary convective electricfield on the distribution of heavy pickup ions around Mars[J]. Journal of Geophysical ResearchSpace Physics, 2018, 123(1): 473-484.
[13] Ramstad R, Barabash S, Futaana Y, et al. Global Mars-solar wind coupling and ion escape[J].Journal of Geophysical Research Space Physics, 2017, 122.
[14] Russell C, Luhmann J, Schwingenschuh K, et al. Upstream waves at mars: Phobos observations[J]. Geophysical Research Letters, 1990, 17(6): 897-900.
[15] Wei H, Russell C. Proton cyclotron waves at Mars: Exosphere structure and evidence for a fastneutral disk[J]. Geophysical research letters, 2006, 33(23).
[16] Halekas J S, Ruhunusiri S, Vaisberg O L, et al. Properties of plasma waves observed upstreamfrom Mars[J]. Journal of Geophysical Research: Space Physics, 2020, 125(9): e2020JA028221.
[17] Lillis R J, Brain D A, Bougher S W, et al. Characterizing atmospheric escape from Mars todayand through time, with MAVEN[J]. Space Science Reviews, 2015, 195: 357-422.
[18] Bertucci C, Mazelle C, Acuña M H. Interaction of the solar wind with Mars from Mars GlobalSurveyor MAG/ER observations[J]. Journal of atmospheric and solar-terrestrial physics, 2005,67(17-18): 1797-1808.
[19] Bertucci C, Mazelle C, Crider D, et al. Magnetic field draping enhancement at the Martianmagnetic pileup boundary from Mars global surveyor observations[J]. Geophysical researchletters, 2003, 30(2).
[20] Zhang M, Luhmann J, Nagy A, et al. Oxygen ionization rates at Mars and Venus: Relativecontributions of impact ionization and charge exchange[J]. Journal of Geophysical Research:Planets, 1993, 98(E2): 3311-3318.
[21] Leblanc F, Johnson R. Sputtering of the Martian atmosphere by solar wind pick-up ions[J].Planetary and Space Science, 2001, 49(6): 645-656.
[22] Wei Y, Fraenz M, Dubinin E, et al. Ablation of Venusian oxygen ions by unshocked solarwind[J]. Science Bulletin, 2017, 62: 1669-1672.
[23] Huddleston D, Johnstone A. Relationship between wave energy and free energy from pickupions in the comet Halley environment[J]. Journal of Geophysical Research: Space Physics,1992, 97(A8): 12217-12230.
[24] Huddleston D, Strangeway R, Warnecke J, et al. Ion cyclotron waves in the Io torus during theGalileo encounter: Warm plasma dispersion analysis[J]. Geophysical research letters, 1997, 24(17): 2143-2146.
[25] Gary S P. Electromagnetic ion/ion instabilities and their consequences in space plasmas: Areview[J]. Space Science Reviews, 1991, 56(3-4): 373-415.
[26] Brain D, Bagenal F, Acuna M, et al. Observations of low-frequency electromagnetic plasmawaves upstream from the Martian shock[J]. Journal of Geophysical Research: Space Physics,2002, 107(A6): SMP-9.
[27] Mazelle C, Winterhalter D, Sauer K, et al. Bow shock and upstream phenomena at Mars[J].Space Science Reviews, 2004, 111(1): 115-181.
[28] Schmid D, Narita Y, Plaschke F, et al. Pick-up ion cyclotron waves around Mercury[J]. Geophysical Research Letters, 2021.
[29] Delva M, Zhang T L, Volwerk M, et al. First upstream proton cyclotron wave observations atVenus[J]. Geophysical Research Letters, 2008, 35.
[30] Leisner J, Russell C, Dougherty M, et al. Ion cyclotron waves in Saturn’s E ring: Initial Cassiniobservations[J]. Geophysical Research Letters, 2006, 33(11).
[31] Leisner J, Russell C, Wei H, et al. Probing Saturn’s ion cyclotron waves on high-inclinationorbits: Lessons for wave generation[J]. Journal of Geophysical Research: Space Physics, 2011,116(A9).
[32] Volwerk M, Kivelson M, Khurana K. Wave activity in Europa’s wake: Implications for ionpickup[J]. Journal of Geophysical Research: Space Physics, 2001, 106(A11): 26033-26048.
[33] Tsurutani B T, Smith E J. Strong hydromagnetic turbulence associated with comet GiacobiniZinner[J]. Geophysical research letters, 1986, 13(3): 259-262.
[34] Johnstone A, Glassmeier K, Acuna M, et al. Waves in the magnetic field and solar wind flowoutside the bow shock at comet Halley[C]// ESLAB Symposium on the Exploration of Halley’sComet: volume 250. 1986: 277.
[35] Glassmeier K H, Coates A, Acuna M, et al. Spectral characteristics of low-frequency plasmaturbulence upstream of comet P/Halley[J]. Journal of Geophysical Research: Space Physics,1989, 94(A1): 37-48.
[36] Mazelle C, Neubauer F M. Discrete wave packets at the proton cyclotron frequency at cometP/Halley[J]. Geophysical Research Letters, 2013, 20(2): 153-156.
[37] Jian L K, Wei H Y, Russell C T, et al. Electromagnetic waves near the proton cyclotron frequency: STEREO observations[J]. Astrophysical Journal, 2014, 786(2): 123.
[38] Barabash S, Lundin R. Reflected ions near Mars: PHOBOS-2 observations[J]. Geophysicalresearch letters, 1993, 20(9): 787-790.
[39] Bader A, Stenberg Wieser G, André M, et al. Proton temperature anisotropies in the plasmaenvironment of Venus[J]. Journal of Geophysical Research: Space Physics, 2019, 124(5): 3312-3330.
[40] Madanian H, Schwartz S J, Halekas J S, et al. Nonstationary quasiperpendicular shock and ionreflection at Mars[J]. Geophysical Research Letters, 2020, 47(11): e2020GL088309.
[41] Crawford G K, Strangeway R J, Russell C T. VLF emissions in the Venus foreshock: Comparisonwith terrestrial observations[J]. Journal of Geophysical Research: Space Physics, 1993, 98(A9):15305-15317.
[42] Liu D, Rong Z, Gao J, et al. Statistical properties of solar wind upstream of Mars: MAVENobservations[J]. The Astrophysical Journal, 2021, 911(2): 113.
[43] Lee C, Hara T, Halekas J, et al. MAVEN observations of the solar cycle 24 space weatherconditions at Mars[J]. Journal of Geophysical Research: Space Physics, 2017, 122(3): 2768-2794.
[44] Romanelli N, Bertucci C, Gomez D, et al. Proton cyclotron waves upstream from Mars: observations from Mars global surveyor[J]. Planetary and Space Science, 2013, 76: 1-9.
[45] Romanelli N, Mazelle C, Chaufray J Y, et al. Proton cyclotron waves occurrence rate upstreamfrom Mars observed by MAVEN: Associated variability of the Martian upper atmosphere[J].Journal of Geophysical Research: Space Physics, 2016, 121(11): 11-113.
[46] Halekas J S. Seasonal variability of the hydrogen exosphere of Mars[J]. Journal of GeophysicalResearch: Planets, 2017, 122(5).
[47] Rahmati A, Larson D E, Cravens T E, et al. Seasonal variability of neutral escape from Marsas derived from MAVEN pickup ion observations[J]. Journal of Geophysical Research Planets,2018.
[48] Romeo O, Romanelli N, Espley J, et al. Variability of upstream proton cyclotron wave propertiesand occurrence at Mars observed by MAVEN[J]. Journal of Geophysical Research: SpacePhysics, 2021, 126(2): e2020JA028616.
[49] Liu D, Yao Z H, Wei Y, et al. Upstream proton cyclotron waves: occurrence and amplitudedependence on IMF cone angle at Mars —from MAVEN observations[J]. Earth and PlanetaryPhysics, 2020, 4.
[50] Mazelle C, Neubauer F M. Discrete wave packets at the proton cyclotron frequency at cometP/Halley[J]. Geophysical research letters, 1993, 20(2): 153-156.
[51] Brinca A. Cometary linear instabilities: From profusion to perspective: volume 61[M]. American Geophysical Union (AGU), 1991: 211-221.
[52] Watanabe Y, Terasawa T. On the excitation mechanism of the low-frequency upstream waves[J].Journal of Geophysical Research: Space Physics, 1984, 89(A8): 6623-6630.
[53] Cowee M, Winske D, Russell C, et al. 1D hybrid simulations of planetary ion-pickup: Energypartition[J]. Geophysical research letters, 2007, 34(2).
[54] Cowee M, Gary S, Wei H. Pickup ions and ion cyclotron wave amplitudes upstream of Mars:First results from the 1D hybrid simulation[J]. Geophysical research letters, 2012, 39(8).
[55] Cowee M, Gary S. Electromagnetic ion cyclotron wave generation by planetary pickup ions:One-dimensional hybrid simulations at sub-alfvénic pickup velocities[J]. Journal of Geophysical Research: Space Physics, 2012, 117(A6).
[56] Wu C S, Davidson R. Electromagnetic instabilities produced by neutral-particle ionization ininterplanetary space[J]. Journal of Geophysical Research, 1972, 77(28): 5399-5406.
[57] Rahmati A, Cravens T, Nagy A, et al. Pickup ion measurements by MAVEN: A diagnosticof photochemical oxygen escape from Mars[J]. Geophysical Research Letters, 2014, 41(14):4812-4818.
[58] Gary S P. Theory of space plasma microinstabilities[M]. Cambridge University Press, 1993.
[59] Perraut S, Roux A, Robert P, et al. A systematic study of ULF waves above FH+ from GEOS1 and 2 measurements and their relationships with proton ring distributions[J]. Journal of Geophysical Research: Space Physics, 1982, 87(A8): 6219-6236.
[60] Min K, Liu K, Gary S P. Proton velocity ring-driven instabilities and their dependence on thering speed: Linear theory[J]. Journal of Geophysical Research: Space Physics, 2017, 122(8):7891-7906.
[61] Gary S P, Smith C W, Lee M A, et al. Electromagnetic ion beam instabilities[J]. The Physicsof fluids, 1984, 27(7): 1852-1862.
[62] Halekas J, Ruhunusiri S, Harada Y, et al. Structure, dynamics, and seasonal variability of theMars-solar wind interaction: MAVEN Solar Wind Ion Analyzer in-flight performance and science results[J]. Journal of Geophysical Research: Space Physics, 2017, 122(1): 547-578.
[63] Rahmati A, Larson D, Cravens T, et al. MAVEN measured oxygen and hydrogen pickup ions:Probing the Martian exosphere and neutral escape[J]. Journal of Geophysical Research: SpacePhysics, 2017, 122(3): 3689-3706.
[64] Killen K, Omidi N, Krauss-Varban D, et al. Linear and nonlinear properties of ULF waves drivenby ring-beam distribution functions[J]. Journal of Geophysical Research: Space Physics, 1995,100(A4): 5835-5852.
[65] Gary S P, Madland C D. Electromagnetic ion instabilities in a cometary environment[J]. Journalof Geophysical Research: Space Physics, 1988, 93(A1): 235-241.
[66] Dong Y, Fang X, Brain D A, et al. Strong plume fluxes at Mars observed by MAVEN: Animportant planetary ion escape channel[J]. Geophysical Research Letters, 2016, 42(21): 8942-8950.
[67] Gurnett D A, Bhattacharjee A. Introduction to plasma physics: With space and laboratoryapplications[M]. Cambridge university press, 2005.
[68] Stix T H, Scott F. The theory of plasma waves[J]. American Journal of Physics, 1963, 31(10):816-816.
[69] Matthaeus W H, Goldstein M L. Measurement of the rugged invariants of magnetohydrodynamic turbulence in the solar wind[J]. Journal of Geophysical Research: Space Physics, 1982,87(A8): 6011-6028.
[70] Smith C W, Goldstein M L, Matthaeus W H. Turbulence analysis of the Jovian upstream wavephenomenon[J]. Journal of Geophysical Research: Space Physics, 1983, 88(A7): 5581-5593.
[71] Winske D, Yin L, Omidi N, et al. Hybrid simulation codes: Past, present and future—a tutorial[M]. Berlin, Heidelberg: Springer Berlin Heidelberg, 2003: 136-165.
[72] Harned D S. Quasineutral hybrid simulation of macroscopic plasma phenomena[J]. Journal ofComputational Physics, 1982, 47(3): 452-462.
[73] Kunz M W, Stone J M, Bai X N. Pegasus: A new hybrid-kinetic particle-in-cell code for astrophysical plasma dynamics[J]. Journal of Computational Physics, 2014, 259: 154-174.
[74] Matthews A P. Current advance method and cyclic leapfrog for 2D multispecies hybrid plasmasimulations[J]. Journal of Computational Physics, 1994, 112(1): 102-116.
[75] Terasawa T, Hoshino M, Sakai J I, et al. Decay instability of finite-amplitude circularly polarized Alfvén waves: A numerical simulation of stimulated Brillouin scattering[J]. Journal ofGeophysical Research: Space Physics, 1986, 91(A4): 4171-4187.
[76] Büchner J, Dum C, Scholer M. Space plasma simulation: volume 615[M]. Springer Science &Business Media, 2003.
[77] Langdon A B. Analysis of the time integration in plasma simulation[J]. Journal of Computational Physics, 1979, 30(2): 202-221.
[78] Yee K, et al. Numerical solution of initial boundary value problems involving Maxwell’s equations in isotropic media[J]. IEEE Trans. Antenna Propagation, 1966, 14(302).
[79] Brain D, Barabash S, Boesswetter A, et al. A comparison of global models for the solar windinteraction with Mars[J]. Icarus, 2010, 206(1): 139-151.
[80] Fried B D, Conte S D. The plasma dispersion function: The Hilbert transform of theGaussian[M]. Academic press, 2015.
[81] Abramowitz M. Handbook of mathematical functions, National Bureau of Standards[J]. Applied mathematics series, 1964(55).
[82] Umeda T, Matsukiyo S, Amano T, et al. A numerical electromagnetic linear dispersion relationfor Maxwellian ring-beam velocity distributions[J]. Physics of Plasmas, 2012, 19(7): 072107.
[83] Gary S P, Gosling J T, Forslund D W. The electromagnetic ion beam instability upstream of theEarth’s bow shock[J]. Journal of Geophysical Research: Space Physics, 1981, 86(A8): 6691-6696.
[84] Gary S P, Madland C D, Tsurutani B T. Electromagnetic ion beam instabilities. ii[J]. Astrophysical Journal, 1985, 28(12): 3691-3695.
[85] Cheng K, Liu K, Mousavi A, et al. Hybrid simulation of proton cyclotron waves upstream ofMars generated by pickup ion beam distribution[J]. Geophysical Research Letters, 2023, 50(11): e2023GL103180.
[86] Gary S P, Hinata S, Madland C D, et al. The development of shell-like distributions fromnewborn cometary ions[J]. Geophysical research letters, 1986, 13(13): 1364-1367.
[87] Winske D, Quest K. Electromagnetic ion beam instabilities: Comparison of one-and twodimensional simulations[J]. Journal of Geophysical Research: Space Physics, 1986, 91(A8):8789-8797.
[88] Ruhunusiri S, Halekas J, Connerney J, et al. MAVEN observation of an obliquely propagatinglow-frequency wave upstream of Mars[J]. Journal of Geophysical Research: Space Physics,2016, 121(3): 2374-2389.
[89] Goldstein M, Wong H, Glassmeier K. Generation of low-frequency waves at comet Halley[J].Journal of Geophysical Research: Space Physics, 1990, 95(A2): 947-955.
[90] Smith C W, Goldstein M L, Gary S P, et al. Beam-driven ion cyclotron harmonic resonancesin the terrestrial foreshock[J]. Journal of Geophysical Research: Space Physics, 1985, 90(A2):1429-1434.
[91] Kodera K, Gendrin R, de Villedary C. Complex representation of a polarized signal and itsapplication to the analysis of ulf waves[J]. Journal of Geophysical Research, 1977, 82(7): 1245-1255.
[92] Hu Y, Denton R. Two-dimensional hybrid code simulation of electromagnetic ion cyclotronwaves in a dipole magnetic field[J]. Journal of Geophysical Research: Space Physics, 2009,114(A12).
[93] Hu Y, Denton R, Johnson J. Two-dimensional hybrid code simulation of electromagnetic ioncyclotron waves of multi-ion plasmas in a dipole magnetic field[J]. Journal of GeophysicalResearch: Space Physics, 2010, 115(A9).
[94] Min K, Liu K, Denton R E, et al. Two-dimensional hybrid particle-in-cell simulations of magnetosonic waves in the dipole magnetic field: On a constant L-Shell[J]. Journal of GeophysicalResearch: Space Physics, 2020, 125(10): e2020JA028414.
[95] Mousavi A, Liu K, Sadeghzadeh S. Particle-in-cell simulations of high-frequency waves drivenby pickup ion ring-beam distributions in the outer heliosheath[J]. Monthly Notices of the RoyalAstronomical Society, 2022, 512(3): 4291-4297.
[96] Akimoto K, Winske D. Ion-acoustic-like waves excited by the reflected ions at the Earth’s bowshock[J]. Journal of Geophysical Research: Space Physics, 1985, 90(A12): 12095-12103.
[97] Akimoto K, Omidi N. The generation of broadband electrostatic noise by an ion beam in themagnetotail[J]. Geophysical Research Letters, 1986, 13(2): 97-100.
[98] Gary S P, Omidi N. The ion-ion acoustic instability[J]. Journal of Plasma Physics, 1987, 37(1):45–61.
[99] Fuselier S A, Gary S P, Thomsen M F, et al. Ion beams and the ion/ion acoustic instabilityupstream from the Earth’s bow shock[J]. Journal of Geophysical Research: Space Physics,1987, 92(A5): 4740-4744.
[100] Romeo O M, Romanelli N, Espley J R, et al. Variability of upstream proton cyclotron waveproperties and occurrence at Mars observed by MAVEN[J]. Journal of Geophysical Research:Space Physics, 2021, 126(2): e2020JA028616.
[101] Thorne R M, Tsurutani B T. Resonant interactions between cometary ions and low frequencyelectromagnetic waves[J]. Planetary and Space Science, 1987, 35(12): 1501-1511.
[102] Gary S P, Madland C D. Electromagnetic ion instabilities in a cometary environment[J]. Journalof Geophysical Research: Space Physics, 1988, 93(A1): 235-241.
[103] Meredith N P, Horne R B, Anderson R R. Survey of magnetosonic waves and proton ringdistributions in the Earth’s inner magnetosphere[J]. Journal of Geophysical Research: SpacePhysics, 2008, 113(A6).
[104] Xiao F, Zhou Q, He Z, et al. Magnetosonic wave instability by proton ring distributions: Simultaneous data and modeling[J]. Journal of Geophysical Research: Space Physics, 2013, 118(7): 4053-4058.
[105] Min K, Liu K. Proton velocity ring-driven instabilities in the inner magnetosphere: Lineartheory and particle-in-cell simulations[J]. Journal of Geophysical Research: Space Physics,2016, 121(1): 475-491.
[106] Mousavi A, Liu K, Min K. Mirror instability driven by pickup ions in the outer heliosheath[J].The Astrophysical Journal, 2020, 901(2): 167.
[107] Liu K, Möbius E, Gary S P, et al. Pickup proton instabilities and scattering in the distant solarwind and the outer heliosheath: Hybrid simulations[J]. Journal of Geophysical Research: SpacePhysics, 2012, 117(A10).
[108] Summerlin E J, Viñas A F, Moore T E, et al. On the stability of pick-up ion ring distributionsin the outer heliosheath[J]. The Astrophysical Journal, 2014, 793(2): 93.
[109] Collinson G, Halekas J, Grebowsky J, et al. A hot flow anomaly at Mars[J]. GeophysicalResearch Letters, 2015, 42(21): 9121-9127.
[110] Collinson G, Wilson III L B, Omidi N, et al. Solar wind induced waves in the skies of Mars:Ionospheric compression, energization, and escape resulting from the impact of ultralow frequency magnetosonic waves generated upstream of the Martian bow shock[J]. Journal of Geophysical Research: Space Physics, 2018, 123(9): 7241-7256.
[111] Halekas J S, McFadden J P, Connerney J E P, et al. Time-dispersed ion signatures observedin the Martian magnetosphere by MAVEN[J]. Geophysical Research Letters, 2015, 42(21):8910-8916.
[112] Fowler C M, Andersson L, Halekas J, et al. Electric and magnetic variations in the near-Marsenvironment[J]. Journal of Geophysical Research: Space Physics, 2017, 122(8): 8536-8559.
[113] Fowler C M, Andersson L, Ergun R E, et al. MAVEN observations of solar wind-driven magnetosonic waves heating the Martian dayside ionosphere[J]. Journal of Geophysical Research:Space Physics, 2018, 123(5): 4129-4149.
[114] Liu D, Rong Z, Gao J, et al. Statistical properties of solar wind upstream of Mars: MAVENobservations[J]. The Astrophysical Journal, 2021, 911(2): 113.
[115] Liu K. Particle-in-cell simulations of particle energization in the auroral region[D]. CornellUniversity, New York, 2007.
[116] Min K, Liu K. Contributions of mirror and ion bernstein instabilities to the scattering of pickupions in the outer heliosheath[J]. The Astrophysical Journal, 2018, 852(1): 39.
[117] Gary S P. The mirror and ion cyclotron anisotropy instabilities[J]. Journal of GeophysicalResearch: Space Physics, 1992, 97(A6): 8519-8529.
[118] Wei H, Cowee M, Russell C, et al. Ion cyclotron waves at Mars: Occurrence and wave properties[J]. Journal of Geophysical Research: Space Physics, 2014, 119(7): 5244-5258.
[119] Liu D, Yao Z, Wei Y, et al. Upstream proton cyclotron waves: Occurrence and amplitudedependence on IMF cone angle at Mars—from MAVEN observations[J]. Earth and PlanetaryPhysics, 2020, 4(1): 51-61.
[120] Florinski V, Zank G, Heerikhuisen J, et al. Stability of a pickup ion ring-beam population in theouter heliosheath: Implications for the IBEX ribbon[J]. The Astrophysical Journal, 2010, 719(2): 1097.
[121] Cowee M, Gary S, Wei H, et al. An explanation for the lack of ion cyclotron wave generation bypickup ions at Titan: 1-D hybrid simulation results[J]. Journal of Geophysical Research: SpacePhysics, 2010, 115(A10).
[122] Mousavi A, Liu K, Sadeghzadeh S. Stability analysis of the pickup ion ring-beam distributionsin the outer heliosheath[J]. Monthly Notices of the Royal Astronomical Society, 2021, 506(3):3662-3668.
[123] Mousavi A, Liu K, Sadeghzadeh S. Hybrid simulations of the ring-beam instabilities driven bythe pickup ions in the outer heliosheath[J]. Monthly Notices of the Royal Astronomical Society,2022, 510(1): 1031-1042.
[124] Summerlin E J, Viñas A F, Moore T E, et al. On the stability of pick-up ion ring distributionsin the outer heliosheath[J]. The Astrophysical Journal, 2014, 793(2): 93.
[125] Florinski V, Heerikhuisen J, Niemiec J, et al. The IBEX ribbon and the pickup ion ring stabilityin the outer heliosheath. I. Theory and hybrid simulations[J]. The Astrophysical Journal, 2016,826(2): 197.
[126] Press W H, Teukolsky S A, Vetterling W T, et al. Numerical recipes 3rd edition: The art ofscientific computing[M]. Cambridge university press, 2007.
[127] Brinca A L, Tsurutani B T. On the polarization, compression and nonoscillatory behavior ofhydromagnetic waves associated with pickup ions[J]. Geophysical Research Letters, 1987, 14(5): 495-498.
[128] Brinca A L, Tsurutani B T. Unusual characteristics of electromagnetic waves excited bycometary newborn ions with large perpendicular energies[C]// Grewing M, Praderie F, Reinhard R. Exploration of Halley’s Comet. Berlin, Heidelberg: Springer Berlin Heidelberg, 1988:311-319.
[129] Isenberg P A, Lee M A, Hollweg J V. The kinetic shell model of coronal heating and accelerationby ion cyclotron waves: 1. Outward propagating waves[J]. Journal of Geophysical Research:Space Physics, 2001, 106(A4): 5649-5660.
[130] Isenberg P A, Lee M A. A dispersive analysis of bispherical pickup ion distributions[J]. Journalof Geophysical Research: Space Physics, 1996, 101(A5): 11055-11066.
[131] Stix T. Waves in plasmas: volume 26[M]. American Institute of Physics Melville, NY, 1992: 6.
[132] Verniero J, Chandran B, Larson D, et al. Strong perpendicular velocity-space diffusion in protonbeams observed by parker solar probe[J]. The Astrophysical Journal, 2022, 924(2): 112.
[133] Bell T. Nonlinear Alfvén waves in a Vlasov plasma[J]. The Physics of Fluids, 1965, 8(10):1829-1839.
[134] Wang Z, Zhai H, Gao Z, et al. Gyrophase bunched ions in the plasma sheet[J]. Advances inSpace Research, 2017, 59(1): 274-282.
[135] Eastman T E, Anderson R R, Frank L A, et al. Upstream particles observed in the Earth’sforeshock region[J]. Journal of Geophysical Research: Space Physics, 1981, 86(A6): 4379-4395.
[136] Gurgiolo C, Parks G, Mauk B, et al. Non-E×B ordered ion beams upstream of the Earth’s bowshock[J]. Journal of Geophysical Research: Space Physics, 1981, 86(A6): 4415-4424.
[137] Gosling J, Thomsen M, Bame S, et al. Evidence for specularly reflected ions upstream from thequasi-parallel bow shock[J]. Geophysical Research Letters, 1982, 9(12): 1333-1336.
[138] Paschmann G, Sckopke N, Bame S, et al. Observations of gyrating ions in the foot of the nearlyperpendicular bow shock[J]. Geophysical Research Letters, 1982, 9(8): 881-884.
[139] Gurgiolo C, Parks G, Mauk B. Upstream gyrophase bunched ions: A mechanism for creation atthe bow shook and the growth of velocity space structure through gyrophase mixing[J]. Journalof Geophysical Research: Space Physics, 1983, 88(A11): 9093-9100.
[140] Gedalin M. Shock heating of directly transmitted ions[J]. The Astrophysical Journal, 2021, 912(2): 82.
[141] Thomsen M, Gosling J, Bame S, et al. Ion and electron heating at collisionless shocks nearthe critical Mach number[J]. Journal of Geophysical Research: Space Physics, 1985, 90(A1):137-148.
[142] Fuselier S, Thomsen M, Gosling J, et al. Gyrating and intermediate ion distributions upstreamfrom the Earth’s bow shock[J]. Journal of Geophysical Research: Space Physics, 1986, 91(A1):91-99.
[143] Burgess D, Schwartz S. The dynamics and upstream distributions of ions reflected at the Earth’sbow shock[J]. Journal of Geophysical Research: Space Physics, 1984, 89(A9): 7407-7422.
[144] Gurgiolo C, Wong H, Winske D. Low and high frequency waves generated by gyrophasebunched ions at oblique shocks[J]. Geophysical research letters, 1993, 20(9): 783-786.
[145] Meziane K, Mazelle C, Lin R, et al. Three-dimensional observations of gyrating ion distributions far upstream from the Earth’s bow shock and their association with low-frequencywaves[J]. Journal of Geophysical Research: Space Physics, 2001, 106(A4): 5731-5742.
[146] Hoshino M, Terasawa T. Numerical study of the upstream wave excitation mechanism: 1.Nonlinear phase bunching of beam ions[J]. Journal of Geophysical Research: Space Physics,1985, 90(A1): 57-64.
[147] Romanelli N, Mazelle C, Meziane K. Nonlinear wave-particle interaction: Implications fornewborn planetary and backstreaming proton velocity distribution functions[J]. Journal of Geophysical Research: Space Physics, 2018, 123(2): 1100-1117.
[148] Gary S P, Thomsen M F, Fuselier S A. Electromagnetic instabilities and gyrophase-bunchedparticles[J]. The Physics of fluids, 1986, 29(2): 531-535.
[149] Gary S P, Tokar R L. The second-order theory of electromagnetic hot ion beam instabilities[J].Journal of Geophysical Research: Space Physics, 1985, 90(A1): 65-72.
[150] Bortnik J, Thorne R, Omidi N. Nonlinear evolution of EMIC waves in a uniform magnetic field:2. Test-particle scattering[J]. Journal of Geophysical Research: Space Physics, 2010, 115(A12).