Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Teresita Heredia"'
Autor:
Ana G. Elías, Teresita Heredia
Publikováno v:
Geofísica Internacional, Vol 43, Iss 1, Pp 119-124 (2004)
The diurnal variation of peak electron density, NmF2, of five stations for different seasons, solar maximum conditions and quiet magnetic activity (Kp ≤ 3) is analyzed in terms of the ExB drift velocity at the equator. The stations analyzed are Kod
Externí odkaz:
https://doaj.org/article/3e476afc03ab4270b463fa3da6d796a0
Autor:
Teresita Heredia, Ana G. Elías
Publikováno v:
Geofísica Internacional, Vol 43, Iss 1, Pp 119-124 (2004)
Se analiza la variación diurna de la densidad máxima de electrones en la ionosfera, NmF2, medida en cinco estaciones, para diferentes estaciones del año, máxima actividad solar y baja actividad magnética (Kp ≤ 3) en función de la velocidad de
Externí odkaz:
https://doaj.org/article/4dcf7068fa484dd29b116d7516dc8c19
Autor:
Willie Soon, Rodolfo Gustavo Cionco, Ana G. Elias, Teresita Heredia, Flavia Marcela Bazzano, Franco Dario Medina
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 193:105094
Precipitation and temperature over Tucuman (26.8°S, 65.2°W), a province located in the Northwestern region of Argentina, is analyzed for the interval 1889–2018 in search of any plausible statistical associations with impacts and responses from so
Autor:
Teresita Heredia, Ana G. Elias
Publikováno v:
Advances in Space Research. 51:1883-1892
The precipitation over Tucuman (26.8°S; 65.2°W), which is representative of the Northwestern region of Argentina, is analyzed in search of an association with solar and geomagnetic activity, with the purpose of contributing to the controversial iss
Autor:
Teresita Heredia, Ana G. Elias
The precipitation over Tucuman (26.8°S, 65.2°W), Argentina, and Sidney (33.8°S, 151.2°E), Australia, present similar long-term variation patterns. In this work anthropogenic and solar forcings are analyzed as possible drivers of this behavior. Du
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::471f02de39ad14e8aba35d866571deba
https://www.sciencedirect.com/science/article/pii/S0273117715008637
https://www.sciencedirect.com/science/article/pii/S0273117715008637
Publikováno v:
Radio Science. 29:831-838
The total electron content (TEC) of the ionosphere is a parameter of great importance for the systems which use transionospheric radiowaves and for the checking of the validity of ionospheric models. It is known that the highest TEC values in the wor
Publikováno v:
Geofísica Internacional. 39:93-95
Hay indicios de que la irradiancia solar total (TSI) podría presentar las mismas variaciones a largo plazo que la longitud del ciclo (SCL). Esta variación corresponde a la periodicidad de 80-90 años, llamada el ciclo de Gleissberg. Se espera que c
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
The trend of the peak height of the ionospheric F2 layer, hmF2, during three solar cycles (1957?1986) at Tucuman (26.9°S, 65.4°W), station located at the southern peak of the equatorial anomaly, has been estimated. hmF2 was calculated from M(3000),
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5b7a5d76040d3467abf5dd6e3d963a2e
https://www.sciencedirect.com/science/article/pii/S147470650200044X/pdfft?md5=5072fe6c46c68cc42794f3da59797421&pid=1-s2.0-S147470650200044X-main.pdf
https://www.sciencedirect.com/science/article/pii/S147470650200044X/pdfft?md5=5072fe6c46c68cc42794f3da59797421&pid=1-s2.0-S147470650200044X-main.pdf