On the Plasma-Dust Processes Accompanying Meteor Showers

被引:10
|
作者
Morozova, T. I. [1 ]
Popel, S. I. [1 ]
机构
[1] Russian Acad Sci, Space Res Inst, Moscow 117997, Russia
基金
俄罗斯科学基金会;
关键词
meteors; meteor trail; meteoroid trail; meteor shower; dusty plasma; charging of dust grains; dusty sound waves; electrophonic sounds; dust grains in Earth’ s atmosphere; modulation instability; MODULATIONAL EXCITATION; ACOUSTIC PERTURBATIONS; RADIO-EMISSION; MECHANISM; WAVES; SMOKE;
D O I
10.1134/S1063780X20100074
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
Plasma-dust processes in the Earth's ionosphere related to transit of meteor bodies and spreading of meteor trail are analyzed. Processes that occur in the meteor trail itself and those taking place in the Earth's atmosphere upon transit of a meteor body, along with their influence on observers and operation of various technical systems, are investigated. In particular, mechanisms explaining acoustic phenomena accompanying meteor transit during meteor showers are proposed. The mechanism of formation of dusty plasma in meteoroid trails is described. It is demonstrated that charging of dust particles of the meteoroid material creates conditions for the appearance of dust acoustic waves. Dust acoustic perturbations are driven as a result of development of modulation instability of electromagnetic waves emitted by the meteor trail and have frequencies typical of dust sound (0.003-60 Hz). The reports of witnesses revealed that observers on the Earth can hear low-frequency sounds appearing during meteor showers. It is suggested that the sound reaches the Earth's surface as a result of transfer of oscillations from dust particles to neutrals the concentration of which in the atmosphere is high. The mechanisms of fragmentation of meteor bodies and charging of formed dust particles are analyzed. Characteristic charges of dust fragments for nano- and micrometer-scale particles are estimated. Particles of different shape are considered. The growth rates that give rise to modulation excitation of low-frequency dust acoustic perturbations are calculated. Conditions leading to development of a modulation instability are found.
引用
收藏
页码:1075 / 1088
页数:14
相关论文
共 50 条
  • [41] Multi-station Video Orbits of Minor Meteor Showers
    José M. Madiedo
    Josep M. Trigo-Rodríguez
    Earth, Moon, and Planets, 2008, 102 : 133 - 139
  • [42] Occurrence and Altitude of the Long-Lived Nonspecular Meteor Trails During Meteor Showers at High Latitudes
    Kozlovsky, A.
    Lukianova, R.
    Lester, M.
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2020, 125 (08)
  • [43] Non-extensive statistical analysis of meteor showers and lunar flashes
    Betzler, A. S.
    Borges, E. P.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2015, 447 (01) : 765 - 771
  • [44] Independent identification of meteor showers from the EDMOND and the search for their parent bodies
    Durisova, Silvia
    Toth, Juraj
    Hajdukova, Maria
    PLANETARY AND SPACE SCIENCE, 2023, 236
  • [45] A comparison of ELF/VLF signals generated by different types of meteor showers
    Amir Kayone Lashkari
    Mohammad Javad Kalaee
    Astrophysics and Space Science, 2019, 364
  • [46] New meteor showers identified in the CAMS and SonotaCo meteoroid orbit surveys
    Rudawska, R.
    Jenniskens, P.
    METEOROIDS 2013, 2014, (86): : 217 - 224
  • [47] A new method to predict meteor showers - II. Application to the Leonids
    Vaubaillon, J
    Colas, F
    Jorda, L
    ASTRONOMY & ASTROPHYSICS, 2005, 439 (02) : 761 - 770
  • [48] A comparison of ELF/VLF signals generated by different types of meteor showers
    Lashkari, Amir Kayone
    Kalaee, Mohammad Javad
    ASTROPHYSICS AND SPACE SCIENCE, 2019, 364 (07)
  • [49] Meteor showers of comet C/1917 F1 Mellish
    Veres, P.
    Kornos, L.
    Toth, J.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2011, 412 (01) : 511 - 521
  • [50] Meteor showers of comet C/1964 N1 (Ikeya)
    Neslusan, L.
    Hajdukova, M., Jr.
    ASTRONOMY & ASTROPHYSICS, 2018, 616