TY - JOUR
T1 - ISUAL-Observed Blue Luminous Events
T2 - The Associated Sferics
AU - Chou, Jung Kuang
AU - Hsu, Rue Ron
AU - Su, Han Tzong
AU - Chen, Alfred Bing Chih
AU - Kuo, Cheng Ling
AU - Huang, Sung Ming
AU - Chang, Shu Chun
AU - Peng, Kang Ming
AU - Wu, Yen Jung
N1 - Funding Information:
We would like to thank Gaopeng Lu and Steven A. Cummer for providing the LF- detecting system. We thank Gaopeng Lu and Hongbo Zhang for fruitful dis cussions on the LF sferics. We would like to express our gratitude to the Lulin Observatory, National Central University, for hosting our ULF station and to the Cingcao Elementary School and Tucheng Senior High School for hosting our ELF/VLF and LF station. This work was supported in part by National Space Organization (NSPO) and Ministry of Science and Technology (MOST) in Taiwan under grants NSPO-S-106010, MOST 102-2112-M-006 -017 -MY3, MOST 104-2111-M-006 -005 -MY2, MOST 105-2112-M-006-013-MY2, MOST 105-2119-M-006-026, MOST 105-2111-M-006-002, MOST 106-2111-M-006-002-, and MOST 106-2119-M-006-021-. The ISUAL data used in this paper are available by request ([email protected] or [email protected]). The pre vious ISUAL data distribution website (http://sprite.phys.ncku.edu.tw/en/ about-cdf-distribution) will merge with the NSPO satellite database (http://for-mosat.tw/nspo_esok/index.php) after March 2018. The ISUAL data will be available on request from the new data distribution system. The sferics data used in this paper are directly available after a request is made to authors J. K. C ([email protected]) or A. B. C ([email protected]).
PY - 2018/4
Y1 - 2018/4
N2 - The blue luminous events (BLEs) recorded by ISUAL (Imager of Sprites and Upper Atmospheric Lightning) radiate unambiguous middle ultraviolet to blue emissions (230–450 nm) but contain dim red emissions (623–754 nm). The BLE appears to be dot-like on one ISUAL image with an integration time of 29 ms. A few BLEs develop upward into blue jets/starters or type II gigantic jets (GJs). The associated sferics of the BLEs in the extremely low frequency to very low frequency band and in the low-frequency band exhibit similar patterns to the narrow bipolar events (NBEs) identified in the very low frequency and low-frequency band. The ISUAL BLEs are conjectured to be the accompanied light emissions of the NBEs. Both upward and downward propagating current obtained from the associated sferics of the BLEs have been found. The source heights of the six BLEs related to negative NBEs are estimated in the range of 16.2–17.8 km. These six events are suggested to occur between the upper positive charge layer and the negative screen charge layer on the top of the normally electrified thunderstorm. The six blue starters, one blue jet, and one type II GJ are inferred to be positive upward discharges from their associated sferics in the extremely low frequency to very low frequency band. Based on the simultaneous radio and optical observations, a NBE is conjectured to be the initiation discharge with rapidly flowing current within the thunderstorm, while a blue jet/starter or a type II GJ is suggested to be the ensuing discharge with slowly varying current propagating upward from the thunderstorm.
AB - The blue luminous events (BLEs) recorded by ISUAL (Imager of Sprites and Upper Atmospheric Lightning) radiate unambiguous middle ultraviolet to blue emissions (230–450 nm) but contain dim red emissions (623–754 nm). The BLE appears to be dot-like on one ISUAL image with an integration time of 29 ms. A few BLEs develop upward into blue jets/starters or type II gigantic jets (GJs). The associated sferics of the BLEs in the extremely low frequency to very low frequency band and in the low-frequency band exhibit similar patterns to the narrow bipolar events (NBEs) identified in the very low frequency and low-frequency band. The ISUAL BLEs are conjectured to be the accompanied light emissions of the NBEs. Both upward and downward propagating current obtained from the associated sferics of the BLEs have been found. The source heights of the six BLEs related to negative NBEs are estimated in the range of 16.2–17.8 km. These six events are suggested to occur between the upper positive charge layer and the negative screen charge layer on the top of the normally electrified thunderstorm. The six blue starters, one blue jet, and one type II GJ are inferred to be positive upward discharges from their associated sferics in the extremely low frequency to very low frequency band. Based on the simultaneous radio and optical observations, a NBE is conjectured to be the initiation discharge with rapidly flowing current within the thunderstorm, while a blue jet/starter or a type II GJ is suggested to be the ensuing discharge with slowly varying current propagating upward from the thunderstorm.
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U2 - 10.1002/2017JA024793
DO - 10.1002/2017JA024793
M3 - Article
AN - SCOPUS:85045755529
SN - 2169-9402
VL - 123
SP - 3063
EP - 3077
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 4
ER -