Add to ORKGSolar radio burst on 408 MHz are not completely correlated, with burst on other frequencies, it gives the possibility of different origin.Asociación Argentina de Astronomí
We present a detailed study of a 1B/M6.9 impulsive flare combining high time resolution (1 ms) and i...
This work shows the different spectral behavior in the H and K region of some characteristic active ...
From the spectral material obtained in the spectroheliograph of San Miguel, between June 1969 and Ap...
Solar radio burst on 408 MHz are not completely correlated, with burst on other frequencies, it give...
A study is presented about the formation of a loop prominence system (LPS) on May 13, 1971. The deve...
A study is presented about the formation of a loop prominence system (LPS) on May 13, 1971. The deve...
A study is presented about the formation of a loop prominence system (LPS) on May 13, 1971. The deve...
Macroscopic velocity fields have been studied in a solar prominence. The spectra and monochromatic i...
Macroscopic velocity fields have been studied in a solar prominence. The spectra and monochromatic i...
Macroscopic velocity fields have been studied in a solar prominence. The spectra and monochromatic i...
We discuss the observations of two eruptive prominences, and the formation of condensations during t...
We discuss the observations of two eruptive prominences, and the formation of condensations during t...
The search of solar bursts recorded in 1968 and 1970 at 408 MHz shows the presence of bursts not cor...
The search of solar bursts recorded in 1968 and 1970 at 408 MHz shows the presence of bursts not cor...
El propósito de este trabajo es el estudio de las estructuras temporales finas (radio-eventos con ti...
We present a detailed study of a 1B/M6.9 impulsive flare combining high time resolution (1 ms) and i...
This work shows the different spectral behavior in the H and K region of some characteristic active ...
From the spectral material obtained in the spectroheliograph of San Miguel, between June 1969 and Ap...
Solar radio burst on 408 MHz are not completely correlated, with burst on other frequencies, it give...
A study is presented about the formation of a loop prominence system (LPS) on May 13, 1971. The deve...
A study is presented about the formation of a loop prominence system (LPS) on May 13, 1971. The deve...
A study is presented about the formation of a loop prominence system (LPS) on May 13, 1971. The deve...
Macroscopic velocity fields have been studied in a solar prominence. The spectra and monochromatic i...
Macroscopic velocity fields have been studied in a solar prominence. The spectra and monochromatic i...
Macroscopic velocity fields have been studied in a solar prominence. The spectra and monochromatic i...
We discuss the observations of two eruptive prominences, and the formation of condensations during t...
We discuss the observations of two eruptive prominences, and the formation of condensations during t...
The search of solar bursts recorded in 1968 and 1970 at 408 MHz shows the presence of bursts not cor...
The search of solar bursts recorded in 1968 and 1970 at 408 MHz shows the presence of bursts not cor...
El propósito de este trabajo es el estudio de las estructuras temporales finas (radio-eventos con ti...
We present a detailed study of a 1B/M6.9 impulsive flare combining high time resolution (1 ms) and i...
This work shows the different spectral behavior in the H and K region of some characteristic active ...
From the spectral material obtained in the spectroheliograph of San Miguel, between June 1969 and Ap...