Zobrazeno 1 - 10
of 44
pro vyhledávání: '"Ernesto Aguilar-Rodriguez"'
Autor:
Esmeralda Romero-Hernandez, Federico Salinas-Samaniego, Olusegun F. Jonah, Ernesto Aguilar-Rodriguez, Mario Rodriguez-Martinez, Giorgio Arlan da Silva Picanço, Clezio M. Denardini, Carlos Alberto Guerrero-Peña, Rogelio Aguirre-Gutierrez, Flor Araceli Garcia-Castillo, Sandra Ayala, Eduardo Perez-Tijerina, Maria A. Sergeeva, Juan Americo Gonzalez-Esparza
Publikováno v:
Atmosphere, Vol 15, Iss 8, p 894 (2024)
We present a statistical study of some physical properties of medium-scale traveling ionospheric disturbances (MSTIDs) registered over the Mexican territory during 2018 and 2019 (solar minimum). The analysis is based on total electron content (TEC) a
Externí odkaz:
https://doaj.org/article/d060b371d93144aea725344cfe91fd6c
Autor:
Maria A. Sergeeva, Juan Americo Gonzalez-Esparza, Victor Jose Gatica-Acevedo, Luis Xavier Gonzalez, Pedro Corona-Romero, Ernesto Aguilar-Rodriguez, Angela Melgarejo-Morales, Isaac David Orrala-Legorreta, Julio Cesar Mejia-Ambriz, Jose Juan Gonzalez-Aviles
Publikováno v:
Remote Sensing, Vol 15, Iss 19, p 4839 (2023)
Space Weather (SW) hazards are discussed in terms of the operation of national SW services and global SW centers for the International Civil Aviation Organization (ICAO). The definition of threshold values of monitored parameters which are used to id
Externí odkaz:
https://doaj.org/article/c7e2fea585fb4d51be1c21410b9d9eac
Autor:
Maria A. Sergeeva, Olga A. Maltseva, Artem M. Vesnin, Donat V. Blagoveshchensky, Victor J. Gatica-Acevedo, J. Americo Gonzalez-Esparza, Aleksandr G. Chernov, Isaac D. Orrala-Legorreta, Angela Melgarejo-Morales, Luis Xavier Gonzalez, Mario Rodriguez-Martinez, Ernesto Aguilar-Rodriguez, Ernesto Andrade-Mascote, Pablo Villanueva
Publikováno v:
Remote Sensing, Vol 15, Iss 2, p 397 (2023)
Manifestations of two solar flares of March 2022 were studied over Mexico. The flare effects in the lower ionosphere had a ~3 min delay from the X1.3-flare onset and ~5 min from the M9.6-flare onset. The maximal impact on the HF signal amplitude was
Externí odkaz:
https://doaj.org/article/30e6ac9a6f8b40fa98c15b01a447177e
Autor:
Maria A. Sergeeva, Vladislav V. Demyanov, Olga A. Maltseva, Artem Mokhnatkin, Mario Rodriguez-Martinez, Raul Gutierrez, Artem M. Vesnin, Victor Jose Gatica-Acevedo, Juan Americo Gonzalez-Esparza, Mark E. Fedorov, Tatiana V. Ishina, Marni Pazos, Luis Xavier Gonzalez, Pedro Corona-Romero, Julio Cesar Mejia-Ambriz, Jose Juan Gonzalez-Aviles, Ernesto Aguilar-Rodriguez, Enrique Cabral-Cano, Blanca Mendoza, Esmeralda Romero-Hernandez, Ramon Caraballo, Isaac David Orrala-Legorreta
Publikováno v:
Atmosphere, Vol 12, Iss 2, p 185 (2021)
Possible ionospheric effects of the Morelian meteoroid that passed and exploded over Mexico on 19 February 2020 (18 February 2020 local time) were estimated. The meteoroid trajectory, velocity and time of occurrence were calculated based on outdoor c
Externí odkaz:
https://doaj.org/article/88e9f470639d491bb9dcf8a08a45af9d
Autor:
Cruz Ernesto Aguilar-Rodriguez, Jorge Flores-Velazquez, Fernando Rojano-Aguilar, Waldo Ojeda-Bustamante, Mauro Iñiguez-Covarrubias
Publikováno v:
Tecnología y ciencias del agua, Vol 11, Iss 4, Pp 27-57 (2020)
Los grados días calor (GDC) son un indicador del crecimiento de un cultivo, que puede ser usado para inferir la duración del ciclo del tomate bajo invernadero. Inferir duración del ciclo de cultivo basado en temperatura supone la posibilidad de pr
Externí odkaz:
https://doaj.org/article/6358d390f8dc42f79bb08ca07a3fd128
Akademický článek
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Publikováno v:
Tecnología y ciencias del agua. :01-32
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4c297488cb583fc35f455a3eae56f6cc
https://doi.org/10.24850/j-tyca-14-5-4
https://doi.org/10.24850/j-tyca-14-5-4
Autor:
Carlos Perez-Alanis, Miho Janvier, Teresa Nieves-Chinchilla, Ernesto Aguilar-Rodriguez, Pascal Dèmoulin, Pedro Corona-Romero
In situ observations of interplanetary (IP) coronal mass ejections (ICMEs) and IP shocks are important to study as they are the main components of the solar activity. Hundreds of IP shocks have been detected by various space missions at different tim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f12e0a2374f0ba2f439d07cf3801a0a2
https://doi.org/10.21203/rs.3.rs-2326987/v1
https://doi.org/10.21203/rs.3.rs-2326987/v1
Akademický článek
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Akademický článek
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K zobrazení výsledku je třeba se přihlásit.
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