Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.creator | González, L. X. | - |
| dc.creator | Valdés Galicia, J. F. | - |
| dc.creator | Sanchez, Federico Andrés | - |
| dc.creator | Muraki, Y. | - |
| dc.creator | Sako, T. | - |
| dc.creator | Watanabe, K. | - |
| dc.creator | Matsubara, Y. | - |
| dc.creator | Nagai, Y. | - |
| dc.creator | Shibata, S. | - |
| dc.creator | Sakai, T. | - |
| dc.creator | Musalem, O. | - |
| dc.creator | Hurtado, A. | - |
| dc.date | 2018-04-05T13:54:53Z | - |
| dc.date | 2018-04-05T13:54:53Z | - |
| dc.date | 2015-11 | - |
| dc.date | 2018-03-27T15:14:10Z | - |
| dc.date.accessioned | 2019-04-29T15:48:25Z | - |
| dc.date.available | 2019-04-29T15:48:25Z | - |
| dc.date.issued | 2015-11 | - |
| dc.identifier | González, L. X.; Valdés Galicia, J. F.; Sanchez, Federico Andrés; Muraki, Y.; Sako, T.; et al.; Re-evaluation of the neutron emission from the solar flare of 2005 September 7, detected by the solar neutron telescope at Sierra Negra; IOP Publishing; Astrophysical Journal; 814; 2; 11-2015; 1-7 | - |
| dc.identifier | 0004-637X | - |
| dc.identifier | http://hdl.handle.net/11336/40810 | - |
| dc.identifier | CONICET Digital | - |
| dc.identifier | CONICET | - |
| dc.identifier.uri | http://rodna.bn.gov.ar:8080/jspui/handle/bnmm/302551 | - |
| dc.description | The X17.0 solar flare of 2005 September 7 released high-energy neutrons that were detected by the Solar Neutron Telescope (SNT) at Sierra Negra, Mexico. In three separate and independent studies of this solar neutron event, several of its unique characteristics were studied; in particular, a power-law energy spectra was estimated. In this paper, we present an alternative analysis, based on improved numerical simulations of the detector using GEANT4, and a different technique for processing the SNT data. The results indicate that the spectral index that best fits the neutron flux is around 3, in agreement with previous works. Based on the numerically calculated neutron energy deposition on the SNT, we confirm that the detected neutrons might have reached an energy of 1 GeV, which implies that 10 GeV protons were probably produced; these could not be observed at Earth, as their parent flare was an east limb event. | - |
| dc.description | Fil: González, L. X.. Universidad Nacional Autónoma de México; México | - |
| dc.description | Fil: Valdés Galicia, J. F.. Universidad Nacional Autónoma de México; México | - |
| dc.description | Fil: Sanchez, Federico Andrés. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Pque. Centenario. Instituto de Tecnología en Detección y Astroparticulas. Comisión Nacional de Energía Atómica. Instituto de Tecnología en Detección y Astroparticulas. Universidad Nacional de San Martín. Instituto de Tecnología en Detección y Astroparticulas; Argentina | - |
| dc.description | Fil: Muraki, Y.. Nagoya University; Japón | - |
| dc.description | Fil: Sako, T.. Nagoya University; Japón | - |
| dc.description | Fil: Watanabe, K.. Institute of Space and Astronautical Science; Japón | - |
| dc.description | Fil: Matsubara, Y.. Nagoya University; Japón | - |
| dc.description | Fil: Nagai, Y.. Nagoya University; Japón | - |
| dc.description | Fil: Shibata, S.. Chubu University; Japón | - |
| dc.description | Fil: Sakai, T.. Nihon University; Japón | - |
| dc.description | Fil: Musalem, O.. Universidad Nacional Autónoma de México; México | - |
| dc.description | Fil: Hurtado, A.. Universidad Nacional Autónoma de México; México | - |
| dc.format | application/pdf | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.publisher | IOP Publishing | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1088/0004-637X/814/2/136 | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/814/2/136/meta | - |
| dc.rights | info:eu-repo/semantics/restrictedAccess | - |
| dc.rights | https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ | - |
| dc.source | reponame:CONICET Digital (CONICET) | - |
| dc.source | instname:Consejo Nacional de Investigaciones Científicas y Técnicas | - |
| dc.source | instacron:CONICET | - |
| dc.source.uri | http://hdl.handle.net/11336/30946 | - |
| dc.subject | Solar flares | - |
| dc.subject | Astronomía | - |
| dc.subject | Ciencias Físicas | - |
| dc.subject | CIENCIAS NATURALES Y EXACTAS | - |
| dc.title | Re-evaluation of the neutron emission from the solar flare of 2005 September 7, detected by the solar neutron telescope at Sierra Negra | - |
| dc.type | info:eu-repo/semantics/article | - |
| dc.type | info:eu-repo/semantics/publishedVersion | - |
| dc.type | info:ar-repo/semantics/articulo | - |
| Aparece en las colecciones: | CONICET | |
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