Implications of Multiple Corona Bursts in Lightning Processes for Radio Frequency Interferometer Observations

被引:5
|
作者
Liu, Ningyu [1 ,2 ]
Scholten, Olaf [3 ]
Dwyer, Joseph R. [1 ,2 ]
Hare, Brian M. [3 ]
Sterpka, Christopher F. [1 ,2 ]
Tilles, Julia N. [4 ]
Lind, Frank D. [5 ]
机构
[1] Univ New Hampshire, Dept Phys & Astron, Durham, NH 03824 USA
[2] Univ New Hampshire, Astron & Space Sci Ctr EOS, Durham, NH 03824 USA
[3] Univ Groningen, Kapteyn Astron Inst, Groningen, Netherlands
[4] Sandia Natl Labs, Albuquerque, NM 87185 USA
[5] MIT, Haystack Observ, Westford, MA 01886 USA
关键词
lightning; radio interferometer; imaging; streamers; corona bursts; VHF; STREAMERS; BREAKDOWN; LOCATION; VHF;
D O I
10.1029/2021GL097367
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Recent observations from LOFAR indicate that multiple, spatially distributed corona bursts can occur in lightning processes with a timescale of 10 microseconds. The close proximity of the corona bursts in space and time poses a great observation challenge for short-baseline (typically <= 100 m) radio interferometers. This paper reports simulations to show the interferometry results that would be obtained with such an interferometer. In particular, spatially-separated corona bursts at fixed locations may be seen as a fast (>10(7) m/s) propagating source with large power variation if the resolution of the instrument is greater than the spatial separation of the bursts. The implications and suggestions for lightning interferometry studies are discussed in the paper.
引用
收藏
页数:9
相关论文
共 50 条
  • [41] A Toy Model for the Time-Frequency Structure of Fast Radio Bursts: Implications for the CHIME/FRB Burst Dichotomy
    Metzger, Brian D.
    Sridhar, Navin
    Margalit, Ben
    Beniamini, Paz
    Sironi, Lorenzo
    ASTROPHYSICAL JOURNAL, 2022, 925 (02):
  • [42] Discrepancy between the Low-frequency Cutoffs of Type III Radio Bursts Based on Simultaneous Observations by WIND and PSP
    Ma, Bing
    Chen, Ling
    Wu, Dejin
    Pulupa, Marc
    Bale, Stuart D.
    ASTROPHYSICAL JOURNAL LETTERS, 2022, 932 (02)
  • [43] The Halo CME Event Of 23 October 1997 – Low-Frequency Radio Observations Of The Pre-Event Corona
    R. Ramesh
    Solar Physics, 2000, 196 : 213 - 220
  • [44] A Low-Frequency (30 – 110 MHz) Antenna System for Observations of Polarized Radio Emission from the Solar Corona
    R. Ramesh
    C. Kathiravan
    M. S. SundaraRajan
    Indrajit V. Barve
    C. V. Sastry
    Solar Physics, 2008, 253 : 319 - 327
  • [45] Radio Occultation Observations of the Solar Corona Over 1.60-1.86 R⊙: Faraday Rotation and Frequency Shift Analysis
    Wexler, David B.
    Hollweg, Joseph, V
    Efimov, Anatoli, I
    Song, Paul
    Jensen, Elizabeth A.
    Lionello, Roberto
    Vierinen, Juha
    Coster, Anthea J.
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2019, 124 (10) : 7761 - 7777
  • [46] The halo CME event of 23 October 1997 - Low-frequency radio observations of the pre-event corona
    Ramesh, R
    SOLAR PHYSICS, 2000, 196 (01) : 213 - 220
  • [47] FURTHER OBSERVATIONS OF MULTIPLE-QUANTUM TRANSITIONS - SATURATION EFFECTS IN RADIO-FREQUENCY TRANSITIONS
    KUSCH, P
    PHYSICAL REVIEW, 1956, 101 (02): : 627 - 636
  • [48] A Low-Frequency (30-110 MHz) Antenna System for Observations of Polarized Radio Emission from the Solar Corona
    Ramesh, R.
    Kathiravan, C.
    SundaraRajan, M. S.
    Barve, Indrajit V.
    Sastry, C. V.
    SOLAR PHYSICS, 2008, 253 (1-2) : 319 - 327
  • [49] 3D Radio Frequency Mapping and Polarization Observations Show Lightning Flashes Were Ignited by Cosmic-Ray Showers
    Shao, Xuan-Min
    Jensen, Daniel P.
    Ho, Cheng
    Caffrey, Michael P.
    Raby, Eric Y.
    Graham, Paul S.
    Haynes, W. Brian
    Blaine, William G.
    JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 2025, 130 (05)
  • [50] LOW-FREQUENCY OBSERVATIONS OF POLARIZED EMISSION FROM LONG-LIVED NON-THERMAL RADIO SOURCES IN THE SOLAR CORONA
    Ramesh, R.
    Kathiravan, C.
    Narayanan, A. Satya
    ASTROPHYSICAL JOURNAL, 2011, 734 (01):