| 1. Identity statement | ||||
| Reference Type | Journal Article | |||
| Site | mtc-m21b.sid.inpe.br | |||
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identifier | 8JMKD3MGP3W34P/3N8LP5P | |||
| Repository | sid.inpe.br/mtc-m21b/2017/01.23.17.23 (restricted access) | |||
| Last Update | 2017:01.23.17.23.38 (UTC) administrator | |||
| Metadata Repository | sid.inpe.br/mtc-m21b/2017/01.23.17.23.38 | |||
| Metadata Last Update | 2018:06.04.02.27.18 (UTC) administrator | |||
| DOI | 10.1007/s11207-016-1043-6 | |||
| ISSN | 0038-0938 1573-093X | |||
| Citation Key | FernandesKCCKMPRV:2017:SpTrSo | |||
| Title | Spectral trends of solar bursts at sub-THz frequencies  | |||
| Year | 2017 | |||
| Access Date | 2024, May 15 | |||
| Type of Work | journal article | |||
| Secondary Type | PRE PI | |||
| Number of Files | 1 | |||
| Size | 782 KiB | |||
| 2. Context | ||||
| Author | 1 Fernandes, L. O. T. 2 Kaufmann, P. 3 Correia, Emília 4 Castro, C. G. Giménez de 5 Kudaka, A. S. 6 Marun, A. 7 Pereyra, P. 8 Raulin, J. P. 9 Valio, A. B. M. | |||
| Resume Identifier | 1 2 3 8JMKD3MGP5W/3C9JH2C | |||
| Group | 1 2 3 DIDAS-CGCEA-INPE-MCTIC-GOV-BR | |||
| Affiliation | 1 Universidade Presbiteriana Mackenzie 2 Universidade Presbiteriana Mackenzie 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 Universidade Presbiteriana Mackenzie 5 Universidade Presbiteriana Mackenzie 6 Instituto de Ciencias Astronómicas, de la Tierra y del Espacio (CONICET) 7 Complejo Astronômico El Leoncito (CONICET) 8 Universidade Presbiteriana Mackenzie 9 Universidade Presbiteriana Mackenzie | |||
| Author e-Mail Address | 1 2 pierrekau@gmail.com 3 ecorreia@craam.mackenzie.br | |||
| Journal | Solar Physics | |||
| Volume | 292 | |||
| Number | 1 | |||
| Secondary Mark | A2_INTERDISCIPLINAR A2_GEOCIÊNCIAS A2_BIOTECNOLOGIA B1_ENGENHARIAS_IV B1_ASTRONOMIA_/_FÍSICA B2_CIÊNCIA_DA_COMPUTAÇÃO | |||
| History (UTC) | 2017-01-23 17:23:38 :: simone -> administrator :: 2017-01-23 17:23:38 :: administrator -> simone :: 2016 2017-01-23 17:26:34 :: simone -> administrator :: 2016 -> 2017 2018-06-04 02:27:18 :: administrator -> simone :: 2017 | |||
| 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 | Solar flares · Sub-THz bursts · Sub-THz atmospheric transmission · Radio-bursts spectra | |||
| Abstract | Previous sub-THz studies were derived from single-event observations. We here analyze for the first time spectral trends for a larger collection of sub-THz bursts. The collection consists of a set of 16 moderate to small impulsive solar radio bursts observed at 0.2 and 0.4 THz by the Solar Submillimeter-wave Telescope (SST) in 2012 2014 at El Leoncito, in the Argentinean Andes. The peak burst spectra included data from new solar patrol radio telescopes (45 and 90 GHz), and were completed with microwave data obtained by the Radio Solar Telescope Network, when available. We critically evaluate errors and uncertainties in sub-THz flux estimates caused by calibration techniques and the corrections for atmospheric transmission, and introduce a new method to obtain a uniform flux scale criterion for all events. The sub-THz bursts were searched during reported GOES soft X-ray events of class C or larger, for periods common to SST observations. Seven out of 16 events exhibit spectral maxima in the range 5 40 GHz with fluxes decaying at sub-THz frequencies (three of them associated to GOES class X, and four to class M). Nine out of 16 events exhibited the sub-THz spectral component. In five of these events, the sub-THz emission fluxes increased with a separate frequency from that of the microwave spectral component (two classified as X and three as M), and four events have only been detected at sub-THz frequencies (three classified as M and one as C). The results suggest that the THz component might be present throughout, with the minimum turnover frequency increasing as a function of the energy of the emitting electrons. The peculiar nature of many sub-THz burst events requires further investigations of bursts that are examined from SST observations alone to better understand these phenomena. | |||
| Area | CEA | |||
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Spectral trends of... | |||
| doc Directory Content | access | |||
| source Directory Content | there are no files | |||
| agreement Directory Content |
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| 4. Conditions of access and use | ||||
| Language | en | |||
| Target File | fernandes-spectral.pdf | |||
| User Group | simone | |||
| Reader Group | administrator simone | |||
| Visibility | shown | |||
| Archiving Policy | denypublisher denyfinaldraft12 | |||
| Read Permission | deny from all and allow from 150.163 | |||
| Update Permission | not transferred | |||
| 5. Allied materials | ||||
| Next Higher Units | 8JMKD3MGPCW/3ETR8EH | |||
| Citing Item List | sid.inpe.br/bibdigital/2013/10.01.00.07 4 | |||
| Dissemination | WEBSCI; PORTALCAPES; SCOPUS. | |||
| Host Collection | sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 | |||
| 6. Notes | ||||
| Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository month nextedition notes orcid pages parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url | |||
| 7. Description control | ||||
| e-Mail (login) | simone | |||
| update | ||||