Add to ORKGEl propósito de este trabajo es el estudio de las estructuras temporales finas (radio-eventos con tiempo característico t <10-1 segundos) de la radioemisión solar. Las observaciones usadas fueron proporcionadas por el polarímetro multicanal de la Estación Basovizza del Observatorio Astronómico de Trieste en las frecuencias de 237, 327, y 408 MHz. Para este estudio fueron seleccionados dos casos de estudio en dependencia del diagrama del patrón de polarización. Fueron seleccionados los radio-eventos de febrero 8 y julio 9 de 1982, ambos asociados a destellos con emisión gamma. Se consideraron sólo eventos con más de 100 unidades de flujo solar. La relación entre la intensidad de los eventos impulsivos y la intensidad del continuo de la radio...
The solar flare phenomenon is one of the powerful events on the Sun that had been discovered in 1859...
International audienceThis paper will review the input of 65 years of radio observations to our unde...
Observations of the solar radio spectrum have been made with high time and frequency resolution. Sp...
Theory and Interpretation of Solar Decimetric Radio Bursts (doctoral thesis) Miroslav Bárta 2002 Abs...
Theory and Interpretation of Solar Decimetric Radio Bursts (doctoral thesis) Miroslav Bárta 2002 Abs...
On étudie les émissions radio transitoires du soleil provenant de l'interaction entre le plasma coro...
Solar radio burst on 408 MHz are not completely correlated, with burst on other frequencies, it give...
Coronal Mass Ejections (CMEs) are well known as one of the most massive eruptions which potentially ...
Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Ci...
The solar flare and Coronal Mass Ejections (CMEs) are well known as one of the most massive eruption...
Solar radio burst on 408 MHz are not completely correlated, with burst on other frequencies, it give...
We present here a brief description of thirteen events of the narrowband solar millisecond radio spi...
We present here a brief description of thirteen events of the narrowband solar millisecond radio spi...
The eruption mechanism of solar flares and type III are currently an extremely active area of resear...
Solar flares observed in the 200 - 400 GHz radio domain may exhibit a slowly varying and time-exten...
The solar flare phenomenon is one of the powerful events on the Sun that had been discovered in 1859...
International audienceThis paper will review the input of 65 years of radio observations to our unde...
Observations of the solar radio spectrum have been made with high time and frequency resolution. Sp...
Theory and Interpretation of Solar Decimetric Radio Bursts (doctoral thesis) Miroslav Bárta 2002 Abs...
Theory and Interpretation of Solar Decimetric Radio Bursts (doctoral thesis) Miroslav Bárta 2002 Abs...
On étudie les émissions radio transitoires du soleil provenant de l'interaction entre le plasma coro...
Solar radio burst on 408 MHz are not completely correlated, with burst on other frequencies, it give...
Coronal Mass Ejections (CMEs) are well known as one of the most massive eruptions which potentially ...
Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Ci...
The solar flare and Coronal Mass Ejections (CMEs) are well known as one of the most massive eruption...
Solar radio burst on 408 MHz are not completely correlated, with burst on other frequencies, it give...
We present here a brief description of thirteen events of the narrowband solar millisecond radio spi...
We present here a brief description of thirteen events of the narrowband solar millisecond radio spi...
The eruption mechanism of solar flares and type III are currently an extremely active area of resear...
Solar flares observed in the 200 - 400 GHz radio domain may exhibit a slowly varying and time-exten...
The solar flare phenomenon is one of the powerful events on the Sun that had been discovered in 1859...
International audienceThis paper will review the input of 65 years of radio observations to our unde...
Observations of the solar radio spectrum have been made with high time and frequency resolution. Sp...