| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | plutao.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | J8LNKAN8RW/3C63NS8 |
| Repository | dpi.inpe.br/plutao/2012/06.21.19.04 |
| Last Update | 2012:10.17.18.59.56 (UTC) marciana |
| Metadata Repository | dpi.inpe.br/plutao/2012/06.21.19.04.39 |
| Metadata Last Update | 2020:09.09.10.51.06 (UTC) marciana |
| DOI | 10.1029/2011RS004794 |
| ISSN | 0048-6604 |
| Label | lattes: 0505123426174183 12 WilliamsKBSNABCDHLSTS:2012:RoHa |
| Citation Key | WilliamsKBSNABCDHLSTS:2012:RoHa |
| Title | Resolution of the sprite polarity paradox: The role of halos  |
| Project | Hungarian Scientific Research Fund (OTKA:K72474); NSF (AGS-1010657); National Science Foundation (ATM-0842751); Office of Naval Research (N00014090443) |
| Year | 2012 |
| Access Date | 2024, May 19 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 1313 KiB |
| 2. Context | |
| Author | 1 Williams, E. 2 Kuo, C. -L. 3 Bór, J. 4 Sátori, G. 5 Newsome, Robert 6 Adachi, Toru 7 Boldi, Robert 8 Chen, A. 9 Downes, Eric 10 Hsu, R. R. 11 Lyons, W. 12 Saba, Marcelo Magalhães Fares 13 Taylor, M. 14 Su, H T |
| Resume Identifier | 1 2 3 4 5 6 7 8 9 10 11 12 8JMKD3MGP5W/3C9JHP6 |
| Group | 1 2 3 4 5 6 7 8 9 10 11 12 CST-CST-INPE-MCTI-GOV-BR |
| Affiliation | 1 Parsons Laboratory, Massachusetts Institute of Technology, Cambridge, MA 02139, United States 2 Department of Physics, National Chen Kung University, Tainan 70101, Taiwan 3 Research Centre for Astronomy and Earth Sciences, GGI, Hungarian Academy of Sciences, Csatkai u. 6-8, Sopron, Hungary 4 Research Centre for Astronomy and Earth Sciences, GGI, Hungarian Academy of Sciences, Csatkai u. 6-8, Sopron, Hungary 5 STAR Laboratory, Department of Electrical Engineering, Stanford University, Stanford, CA 94305, United States 6 STAR Laboratory, Department of Electrical Engineering, Stanford University, Stanford, CA 94305, United States 7 Faculty of Engineering, Design, and Information Technology, University of Bahrain Polytechnic, PO Box 33349, Isa Town, Bahrain 8 Department of Physics, National Chen Kung University, Tainan 70101, Taiwan 9 Parsons Laboratory, Massachusetts Institute of Technology, Cambridge, MA 02139, United States 10 Department of Physics, National Chen Kung University, Tainan 70101, Taiwan 11 FMA Research, Inc., 46050 Weld County Rd. 13, Ft. Collins, CO 80524, United States 12 Instituto Nacional de Pesquisas Espaciais (INPE) 13 Center for Atmospheric and Space Sciences, Utah State University, Ogden, UT 84322-4405, United States 14 Department of Physics, National Chen Kung University, Tainan 70101, Taiwan |
| Author e-Mail Address | 1 2 3 4 5 6 7 8 9 10 11 12 marcelo.saba@inpe.br |
| e-Mail Address | marcelo.saba@inpe.br |
| Journal | Radio Science |
| Volume | 47 |
| Number | 2 |
| Pages | 1-12 |
| Secondary Mark | B1_GEOCIÊNCIAS |
| History (UTC) | 2012-06-22 00:11:00 :: lattes -> secretaria.cpa@dir.inpe.br :: 2012 2012-10-17 18:59:56 :: secretaria.cpa@dir.inpe.br -> administrator :: 2012 2018-06-05 00:01:45 :: administrator -> marciana :: 2012 2020-09-09 10:51:06 :: marciana -> simone :: 2012 |
| 3. Content and structure | |
| Is the master or a copy? | is the master |
| Content Stage | completed |
| Transferable | 1 |
| Content Type | External Contribution |
| Version Type | publisher |
| Keywords | electrical engineering radio halo |
| Abstract | This study revisits the sprite polarity paradox, first manifest by observations that exceptional cloud-to-ground flashes with negative polarity generally did not produce detectable sprites. The paradox is here resolved by the Transient Luminous Event (TLE) known as the halo, which on account of its inferior brightness (0.3 MR versus 1.5 MR) and substantially shorter duration (1 ms versus 10-100 ms) in comparison with the sprite, is not readily detectable in ground-based video cameras with standard field duration (16.7-20 ms). Observations with improved temporal resolution (ISUAL (Imager of Sprites and Upper Atmospheric Lightnings) from space and PIPER (Photometric Imager of Precipitated Electron Radiation) observations from the ground) provide evidence that flashes with negative polarity dominate the global halo population, and that the halo numbers are more than sufficient to account for the previously missing TLEs. The evidence for lightning polarity-dependent TLEs (sprites, positive and halos, negative) is attributable to the well established but incompletely understood contrast in the behavior of negative and positive lightning flashes to ground. Copyright 2012 by the American Geophysical Union. |
| Area | CEA |
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > COCST > Resolution of the... |
| doc Directory Content | access |
| source Directory Content | there are no files |
| agreement Directory Content | there are no files |
| 4. Conditions of access and use | |
| data URL | http://urlib.net/ibi/J8LNKAN8RW/3C63NS8 |
| zipped data URL | http://urlib.net/zip/J8LNKAN8RW/3C63NS8 |
| Language | pt |
| Target File | Williams 2012 sprite polarity paradox.pdf |
| User Group | administrator lattes secretaria.cpa@dir.inpe.br simone |
| Visibility | shown |
| Archiving Policy | denypublisher6 allowfinaldraft |
| Read Permission | allow from all |
| Update Permission | not transferred |
| 5. Allied materials | |
| Next Higher Units | 8JMKD3MGPCW/3F3T29H |
| Citing Item List | sid.inpe.br/mtc-m21/2012/07.13.14.54.40 1 |
| Dissemination | WEBSCI; AGU; MGA; COMPENDEX. |
| Host Collection | dpi.inpe.br/plutao@80/2008/08.19.15.01 |
| 6. Notes | |
| Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress readergroup rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url |
| 7. Description control | |
| e-Mail (login) | simone |
| update | |