Different Types of Corona Discharges Associated With High‐Altitude Positive Narrow Bipolar Events Nearby Cloud Top

Author:

Li Dongshuai12ORCID,Luque Alejandro1ORCID,Gordillo‐Vazquez F. J.1ORCID,Pérez‐Invernón F. J.1ORCID,Husbjerg Lasse Skaaning2ORCID,Neubert Torsten2ORCID,Chanrion Olivier2ORCID,Lu Gaopeng3ORCID,Zhang Hongbo4ORCID,Han Jing5,Lehtinen Nikolai G.6ORCID,Østgaard Nikolai6ORCID,Reglero Víctor7ORCID

Affiliation:

1. Instituto de Astrofísica de Andalucía (IAA) CSIC Granada Spain

2. National Space Institute Technical University of Denmark (DTU Space) Kongens Lyngby Denmark

3. CAS Key Laboratory of Geospace Environment University of Science and Technology of China Hefei China

4. Key Laboratory of Middle Atmosphere and Global Environment Observation (LAGEO) Institute of Atmospheric Science Chinese Academy of Sciences Beijing China

5. Hainan Institute of Meteorological Sciences Haikou China

6. Birkeland Centre for Space Science Department of Physics and Technology University of Bergen Bergen Norway

7. Image Processing Laboratory University of Valencia Valencia Spain

Abstract

AbstractSingle‐ and multi‐pulse blue corona discharges are frequently observed in thunderstorm clouds. Although we know they often correlate with Narrow Bipolar Events (NBEs) in Very Low Frequency/Low Frequency radio signals, their physics is not well understood. Here, we report a detailed analysis of different types of blue corona discharges observed by the Atmosphere‐Space Interactions Monitor during an overpass of a thundercloud cell nearby Malaysia. Both single‐ and multi‐pulse blue corona discharges were associated with positive NBEs at the top of the cloud, reaching about 18 km altitude. We find that the primary pulses of multi‐pulse discharges have weaker current moments than the single‐pulse discharges, suggesting that the multi‐pulse discharges either have shorter vertical channels or have weaker currents than the single‐pulse discharges. The subsequent pulse trains of the multi‐pulse discharges delayed some milliseconds are likely from horizontally oriented electrical discharges, but some NBEs, correlated with both single‐and multi‐pulse discharges, include small‐amplitude oscillations within a few microseconds inside their waveforms, which are unresolved in the optical observation and yet to be understood. Furthermore, by jointly analyzing the optical and radio observations, we estimate the photon free mean path at the cloud top to be ∼6 m.

Funder

European Research Council

H2020 Marie Skłodowska-Curie Actions

Ministerio de Asuntos Económicos y Transformación Digital, Gobierno de España

Danmarks Frie Forskningsfond

CAS-SAFEA International Partnership Program for Creative Research Teams

Instituto de Astrofísica de Andalucía

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Geophysics

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