STATISTICAL ANALYSIS OF LANGMUIR WAVES ASSOCIATED WITH TYPE III RADIO BURSTS: II. SIMULATION AND INTERPRETATION OF THE WAVE ENERGY DISTRIBUTIONS

被引:0
|
作者
Maksimovic, M. [1 ]
Vidojevic, S. [1 ,2 ]
Zaslavsky, A. [1 ]
机构
[1] Univ Paris Diderot, Univ Paris 06, CNRS, Observ Paris,LESIA,UPMC, F-92195 Meudon, France
[2] Univ Belgrade, Fac Math, Belgrade 11000, Serbia
关键词
solar wind; physical processes: plasmas; Langmuir waves;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have modeled electrostatic Langmuir waves by an electric field, consisting of superposition of Gaussian wave packets with several probability distributions of amplitudes and with several Poisson distributions of wave packets. The outcome of the model is that the WIND satellite observations, especially in the low frequency domain (the WAVES experiment), do not allow to conclude whether the input wave amplitude distributions are closer to the log-normal than to the Pearson type I or uniform. The average number of wave packets in 1 s is found to be between 0.1 and 50. Therefore, there is a clear need to measure Langmuir wave energy distributions directly at the waveform level, not a posteriori in the spectral domain. This is planned to be implemented on the RPW (Radio and Plasma Wave Analyzer) instrument in the Solar Orbiter mission.
引用
收藏
页码:600 / 603
页数:4
相关论文
共 50 条
  • [21] PRELIMINARY ANALYSIS OF TYPE III RADIO BURSTS FROM STEREO/WAVES DATA
    Vidojevic, S.
    Maksimovic, M.
    PROCEEDINGS OF THE XV NATIONAL CONFERENCE OF ASTRONOMERS OF SERBIA, 2009, 86 : 287 - +
  • [22] ULYSSES-GALILEO OBSERVATIONS OF TYPE-III RADIO-BURSTS AND ASSOCIATED IN-SITU ELECTRONS AND LANGMUIR-WAVES
    REINER, MJ
    ANDERSON, KA
    ROELOF, E
    ARMSTRONG, T
    HOSPODARSKY, GB
    FAINBERG, J
    STONE, RG
    LANZEROTTI, L
    GURNETT, DA
    PHILLIPS, JL
    FORSYTH, R
    SPACE SCIENCE REVIEWS, 1995, 72 (1-2) : 261 - 266
  • [23] Statistical analysis of characteristics of classified type II radio bursts and their associated solar energetic particle events
    Zhu Cong
    Ding Liu-Guan
    Zhou Kun-Lun
    Qian Tian-Qi
    ACTA PHYSICA SINICA, 2021, 70 (09)
  • [24] Statistical Characteristics on SEPs, Radio-Loud CMEs, Low Frequency Type II and Type III Radio Bursts Associated with Impulsive and Gradual Flares
    P. Pappa Kalaivani
    A. Shanmugaraju
    O. Prakash
    R.-S. Kim
    Earth, Moon, and Planets, 2020, 123 : 61 - 85
  • [25] Statistical Characteristics on SEPs, Radio-Loud CMEs, Low Frequency Type II and Type III Radio Bursts Associated with Impulsive and Gradual Flares
    Kalaivani, P. Pappa
    Shanmugaraju, A.
    Prakash, O.
    Kim, R-S
    EARTH MOON AND PLANETS, 2020, 123 (3-4): : 61 - 85
  • [26] Simulation on solar type II radio bursts associated with corona mass ejections
    Sakai, JI
    Mori, T
    Saito, S
    ASTRONOMY & ASTROPHYSICS, 2005, 442 (02) : 687 - 692
  • [27] Type II radio bursts: 1. New entirely analytic formalism for the electron beams, Langmuir waves, and radio emission
    Schmidt, J. M.
    Cairns, Iver H.
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2012, 117
  • [28] Solar type II radio bursts associated with CME expansions as shown by EUV waves
    Cunha-Silva, R. D.
    Fernandes, F. C. R.
    Selhorst, C. L.
    ASTRONOMY & ASTROPHYSICS, 2015, 578
  • [29] High frequency ion sound waves associated with Langmuir waves in type III radio burst source regions
    Thejappa, G
    MacDowall, RJ
    NONLINEAR PROCESSES IN GEOPHYSICS, 2004, 11 (03) : 411 - 420
  • [30] Analysis of Type II and Type III Radio Bursts Associated with SEPs from Non-Interacting/Interacting Radio-Loud CMEs
    P. Pappa Kalaivani
    O. Prakash
    A. Shanmugaraju
    Li Feng
    Lei Lu
    Weigun Gan
    G. Michalek
    Astrophysics, 2021, 64 : 327 - 344