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Reference TypeConference Paper (Conference Proceedings)
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Sitemtc-m21d.sid.inpe.br (namespace prefix: upn:44QHRCS)
Identifier8JMKD3MGP3W34T/4AC846E
Repositorysid.inpe.br/mtc-m21d/2023/12.11.13.32
Metadata Repositorysid.inpe.br/mtc-m21d/2023/12.11.13.32.14
Metadata Last Update2024:01.02.17.16.56 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyKieuAMKMBSSCSRKRRBLPS:2023:FiLeSp
TitleFirst leader spectra observation associated with TGFs production at the Telescope Array Surface Detector
Year2023
Access Date2026, Nov. 06
Secondary TypePRE CI
2. Context
Author 1 Kieu, Ny
 2 Abbasi, Rasha
 3 Mazzucco, Davide
 4 Knight, Tyler
 5 Mazich, Joeseph
 6 Bratrud, Grace
 7 Saba, Marcelo Magalhães Fares
 8 Silva, Diego Rhamon da
 9 Cruz, Ivan Toucedo
10 Stanley, Mark A.
11 Rison, Wiallim
12 Krehbiel, Paul R.
13 Rodeheffer, Dan
14 Remnington, Jackson
15 Belz, John
16 LeVon, Ryan
17 Petrizze, Alex
18 Smout, Kieran
Resume Identifier 1
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 7 8JMKD3MGP5W/3C9JHP6
Group 1
 2
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 5
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 7 DISSM-CGCT-INPE-MCTI-GOV-BR
 8 CST-CST-DIPGR-INPE-MCTI-GOV-BR
 9 CST-CST-DIPGR-INPE-MCTI-GOV-BR
Affiliation 1 Loyola University Chicago
 2 Loyola University Chicago
 3 Loyola University Chicago
 4 Loyola University Chicago
 5 Loyola University Chicago
 6 Loyola University Chicago
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10 New Mexico Institute of Mining and Technology
11 New Mexico Tech
12 New Mexico Tech
13 New Mexico Tech
14 Oak Ridge National Laboratory
15 University of Utah
16 University of Utah
17 University of Utah
18 University of Utah
Author e-Mail Address 1
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 7 marcelo.saba@inpe.br
 8 diego.silva@inpe.br
 9 ivan.cruz@inpe.br
Conference NameAGU FAll Meeting
Conference LocationSan Francisco, CA
Date11-15 Dec. 2023
PublisherAGU
Book TitleProceedings
Host Collectionurlib.net/www/2021/06.04.03.40 upn:44QHRCS
History (UTC)2023-12-11 13:32:14 :: simone -> administrator ::
2024-01-02 17:16:56 :: administrator -> simone :: 2023
3. Content and structure
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Content Stagecompleted
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Content TypeExternal Contribution
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AbstractIn this work we report the first observation of time-resolved leader spectra associated with Terrestrial Gamma Ray Flashes (TGFs) at the Telescope Array Surface Detector (TASD). The TASD is a ground-based surface detector primarily designed to observe ultra-high energy cosmic rays. The TASD site is equipped with various lightning detection systems, including the Lightning Mapping Array (LMA), Fast Electric Field Change Sensor Antenna (FA), high-resolution Interferometers (INFTs), and the high-speeds camera Phantom v2012 and v711. These systems, along with the TASD, have successfully detected several TGFs in conjunction with thunderstorm-generated lightning discharges. In addition to the optical emissions of leaders associated with TGFs observed by the high-speed camera, we also aim to study spectroscopic analysis of these emissions. From these analyses, we can identify the chemical features, their time dependence, and the differences between leaders with and without TGF productions. To do this, we installed a spectroscopic system next to the high-speed camera. The system includes a grism placed in front of a high-speed camera Phantom v711 mounted by a 14 mm lens. The v711 camera recorded images at 29,900 frames per second, with a spectral resolution of 2 nm per pixel, covering a spectral range from 400 to 900 nm. In this work, we will present detailed analyses of the first leader spectra observed simultaneously with Gamma-ray emission. We have recorded ten spectral images around the TGF emission which showed the changing in the chemical components of the leader before, during, and after the TGF production between 400-900 nm. We also report here the calibration process which was applied for both leader and return stroke of spectral images.
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Languageen
User Groupsimone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/449U4PL
8JMKD3MGPCW/46KUATE
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