| 1. Identity statement | ||||
| Reference Type | Conference Paper (Conference Proceedings) | |||
| Site | mtc-m21d.sid.inpe.br | |||
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identifier | 8JMKD3MGP3W34T/4878DDP | |||
| Repository | sid.inpe.br/mtc-m21d/2022/12.13.17.41 | |||
| Metadata Repository | sid.inpe.br/mtc-m21d/2022/12.13.17.41.34 | |||
| Metadata Last Update | 2023:01.03.16.46.27 (UTC) administrator | |||
| Secondary Key | INPE--PRE/ | |||
| Citation Key | AbbasiBSKRKRRSMLSOBHP:2022:OpCoTe | |||
| Title | The Optical Counterpart of Terrestrial Gamma-ray Flashes Observations at the Telescope Array Detector  | |||
| Year | 2022 | |||
| Access Date | 2024, May 19 | |||
| Secondary Type | PRE CI | |||
| 2. Context | ||||
| Author | 1 Abbasi, Racha 2 Belz, John 3 Saba, Marcelo Magalhães Fares 4 Krehbiel, Paul R. 5 Remington, Jackson 6 Kieu, Ny 7 da, Silva Diego Rhamon Reis 8 Rison, William 9 Rodeheffer, Dan 10 Stanley, Mark A. 11 Mazich, Joeseph 12 LeVon, Ryan 13 Smout, Kieran 14 O'Brien, Kaleigh 15 Bratrud, Gradce 16 Husseini, Nour 17 Petrizze, Alex | |||
| Resume Identifier | 1 2 3 8JMKD3MGP5W/3C9JHP6 | |||
| Group | 1 2 3 DISSM-CGCT-INPE-MCTI-GOV-BR 4 5 6 7 MET-MET-DIPGR-INPE-MCTI-GOV-BR | |||
| Affiliation | 1 Loyola University Chicago 2 University of Utah 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 New Mexico Tech 5 University of Utah 6 Loyola University Chicago 7 Instituto Nacional de Pesquisas Espaciais (INPE) 8 New Mexico Tech 9 New Mexico Tech 10 New Mexico Institute of Mining and Technology 11 Loyola University Chicago 12 University of Utah 13 University of Utah 14 Loyola University Chicago 15 Loyola University Chicago 16 IMSA 17 University of Utah | |||
| Author e-Mail Address | 1 2 3 marcelosaba@gmail.com 4 5 6 7 dieggo522@hotmail.com | |||
| Conference Name | AGU Fall Meeting | |||
| Conference Location | Chicago, IL | |||
| Date | 12-16 Dec. 2022 | |||
| Publisher | AGU | |||
| History (UTC) | 2022-12-13 17:41:34 :: simone -> administrator :: 2023-01-03 16:46:27 :: administrator -> simone :: 2022 | |||
| 3. Content and structure | ||||
| Is the master or a copy? | is the master | |||
| Content Stage | completed | |||
| Transferable | 1 | |||
| Content Type | External Contribution | |||
| Abstract | This work presents the observations of the optical counterpart of a downward-directed terrestrial gamma ray flashes at the Telescope Array (TA) detector. The Telescope Array detector is located in the southwestern desert of the State of Utah. The combination of size and elevation makes it a unique tool that allows us to study thunderstorms. Currently it is the largest ultra-high energy cosmic ray experiment in the Northern Hemisphere. The surface detector array part of the TA experiment, used in these observations, is composed of 507 scintillator detectors on a 1.2 km square grid covering a 700-kilometer square in area, 1400 m above sea level. Previous downward-directed Terrestrial Gamma-ray Flashes (TGFs) observations, using the 700 km2 Telescope Array Surface Detector (TASD), established that observed lightning-correlated energetic particles are downward-directed gamma-ray showers. Moreover, these downward-directed gamma-ray showers were found to be correlated with the early leader and the initial burst pulse stage of cloud-to-ground lightning. In this work, we use the TASD detector, together with a high-speed video camera, in conjunction with the suite of lightning instruments at the TASD site, to report on the optical emission of downward-directed terrestrial gamma ray flashes. The suite of gamma and lightning instruments, timing resolution, and source proximity offers us an unprecedented look at the TGF phenomena. The optical emission observations, together with in-progress efforts, should allow us to better understand which runaway electron production model is responsible for gamma-ray production in the atmosphere. Results from this study allow us to further the understanding of the initiation and propagation mechanism of terrestrial gamma ray flashes. In addition will allow us to further our ability to compare the most recent satellite optical emissions counterpart of upward-directed TGFs to that of downward-directed TGFs. | |||
| Area | MET | |||
| Arrangement 1 | urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > MET > The Optical Counterpart... | |||
| Arrangement 2 | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCT > The Optical Counterpart... | |||
| doc Directory Content | there are no files | |||
| source Directory Content | there are no files | |||
| agreement Directory Content |
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| 4. Conditions of access and use | ||||
| User Group | simone | |||
| Visibility | shown | |||
| Update Permission | not transferred | |||
| 5. Allied materials | ||||
| Next Higher Units | 8JMKD3MGPCW/3F35TRS 8JMKD3MGPCW/46KUATE | |||
| Host Collection | urlib.net/www/2021/06.04.03.40 | |||
| 6. Notes | ||||
| Empty Fields | archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label language lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisheraddress readergroup readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume | |||
| 7. Description control | ||||
| e-Mail (login) | simone | |||
| update | ||||