Add to ORKGWe discuss the observations of two eruptive prominences, and the formation of condensations during the phenomena. The density and intensity variations of the condensations are analyzed spectroscopically in one of the events. Some hypotheses about the magnetic field configuration have been used in order to explain the observational data. The paper in full will be published in Solar Physics.Asociación Argentina de Astronomí
A number of space and ground-based observations give evidence that the eruptive prominences, coronal...
Softcover, DIN A4In this dissertation, the structure, dynamics and evolution of two quiescent promin...
We study 14 cases of dynamic “disparition brusque” (DBd), the sudden disappearance of quiescent fila...
We discuss the observations of two eruptive prominences, and the formation of condensations during t...
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...
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...
Solar radio burst on 408 MHz are not completely correlated, with burst on other frequencies, it give...
Solar radio burst on 408 MHz are not completely correlated, with burst on other frequencies, it give...
This volume presents the latest research results on solar prominences, including new developments on...
In this dissertation, we have studied the structure, dynamics and evolution of two quiescent promine...
In this dissertation, we have studied the structure, dynamics and evolution of two quiescent promine...
A number of space and ground-based observations give evidence that the eruptive prominences, coronal...
Softcover, DIN A4In this dissertation, the structure, dynamics and evolution of two quiescent promin...
We study 14 cases of dynamic “disparition brusque” (DBd), the sudden disappearance of quiescent fila...
We discuss the observations of two eruptive prominences, and the formation of condensations during t...
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...
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...
Solar radio burst on 408 MHz are not completely correlated, with burst on other frequencies, it give...
Solar radio burst on 408 MHz are not completely correlated, with burst on other frequencies, it give...
This volume presents the latest research results on solar prominences, including new developments on...
In this dissertation, we have studied the structure, dynamics and evolution of two quiescent promine...
In this dissertation, we have studied the structure, dynamics and evolution of two quiescent promine...
A number of space and ground-based observations give evidence that the eruptive prominences, coronal...
Softcover, DIN A4In this dissertation, the structure, dynamics and evolution of two quiescent promin...
We study 14 cases of dynamic “disparition brusque” (DBd), the sudden disappearance of quiescent fila...