Zobrazeno 1 - 10
of 21
pro vyhledávání: '"Jenny Marcela Rodríguez Gómez"'
Autor:
Franciele Carlesso, Jenny Marcela Rodríguez Gómez, Adriany Rodrigues Barbosa, Luis Eduardo Antunes Vieira, Alisson Dal Lago
Publikováno v:
Frontiers in Physics, Vol 10 (2022)
Long and reliable total solar irradiance (TSI) time series is one of the essential parameters for understanding solar contributions to climate change. The minor fluctuations of TSI in long timescales could impact the energy balance. Despite the impro
Externí odkaz:
https://doaj.org/article/edd9fe542ef84208a88aac7ecb4138a5
Publikováno v:
Revista Brasileira de Ensino de Física, Vol 44 (2022)
Las variaciones de la intensidad solar del centro al limbo solar son conocidas en Inglés cómo Center to Limb Variations (CLV) u oscurecimiento del limbo solar. Estas permiten caracterizar diferentes capas de la atmósfera solar, específicamente cu
Externí odkaz:
https://doaj.org/article/2a0261a0d76f42b482e3f5c8ff6073b9
Publikováno v:
Revista Brasileira de Ensino de Física, Vol 43 (2021)
La actividad magnética del Sol domina fenómenos a través del espacio, esto incluye la interacción con los planetas, específicamente sus magnetosferas e ionosferas. Estas interacciones son descritas a través de una disciplina llamada clima espac
Externí odkaz:
https://doaj.org/article/044d60c494b846889e246ef78bc95a48
Publikováno v:
Revista Brasileira de Ensino de Física, Vol 46 (2024)
La radiación solar, específicamente la irradiancia en Extremo Ultravioleta (EUV) es importante porque influencia directamente la atmósfera de la Tierra, por ejemplo el sistema de la Ionosfera-Termosfera-Mesosfera (ITM). Las variaciones en la densi
Externí odkaz:
https://doaj.org/article/6f8836c9bdaa43069bdc33b73f099f6b
Publikováno v:
Biblioteca Digital de Teses e Dissertações do INPEInstituto Nacional de Pesquisas EspaciaisINPE.
The present thesis aims at the study of the plasma parameters in the solar corona, using a flux transport model, force free-field extrapolations, a model of emission and optimization algorithm. The physical-model is based on the assumption that the v
Externí odkaz:
http://urlib.net/sid.inpe.br/mtc-m21b/2017/02.16.21.15
Autor:
Franciele Carlesso, Jenny Marcela Rodríguez Gómez, Luis Eduardo Antunes Vieira, Graziela da Silva Savonov, Luiz Angelo Berni, Lucas Lopes Costa
Publikováno v:
Revista Brasileira de Ensino de Física, Vol 41, Iss 2
Resumo A irradiância solar total (TSI) é definida como a energia emitida pelo Sol por unidade de área e recebida pela Terra. Durante muitos anos essa energia foi considerada constante, no entanto, hoje se sabe que há variações em diferentes esc
Externí odkaz:
https://doaj.org/article/b7a221cb5bb441c999772cbbde23905e
The Spectral Imaging of Coronal Environment (SPICE; SPICE Consortium et al. 2020) provides an extraordinary opportunity to study the chromosphere and transition region using EUV wavelengths, e.g., Ne VIII 770 Å, C III 977 Å, O VI 1032 Å, and Lyman
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d9d8560e099edd066dd08ab3e1b8616e
https://doi.org/10.5194/egusphere-egu23-9380
https://doi.org/10.5194/egusphere-egu23-9380
Publikováno v:
Solar Physics
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=r3c4b2081b22::6b42b1a43e85fbc89d35647e887c8acb
Autor:
Astrid Veronig, Tatiana Podlachikova, Anatoly Petrukovich, Alexander Ruzmaikin, Jenny Marcela Rodríguez Gómez, Joan Feynman
Coronal Mass Ejections (CMEs) and their interplanetary counterparts (ICMEs) are the major sources for strong space weather disturbances. We present a study of statistical properties of fast CMEs (v≥1000 km/s) that occurred during solar cycles 23 an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a76b54f029ab7a92fbb0b67b3df4cf61
https://doi.org/10.5194/egusphere-egu21-3990
https://doi.org/10.5194/egusphere-egu21-3990
Autor:
Tatiana Podladchikova, Anatoly Petrukovich, Alexander Ruzmaikin, Jenny Marcela Rodríguez Gómez, Joan Feynman, Astrid Veronig
Publikováno v:
The Astrophysical Journal
We study the clustering properties of fast Coronal Mass Ejections (CMEs) that occurred during solar cycles 23 and 24. We apply two methods: the Max spectrum method can detect the predominant clusters and the de-clustering threshold time method provid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5719e59fe7715be9d2425b0f14a2b1e8
http://arxiv.org/abs/2006.10404
http://arxiv.org/abs/2006.10404