Add to ORKGVarious aspects of solar prominences and the solar corona are discussed. The formation of prominence...
This volume presents the latest research results on solar prominences, including new developments on...
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...
Prominences in the solar corona are a hundredfold cooler and denser than their surroundings, with a ...
The thermal disappearance of solar prominences under strong perturbations due to wave heating, Ohmic...
Quiescent prominences represent a significant challenge to our understanding of the flow of mass and...
Prominence condensation and support, the dynamics of coronal loops, and streamer structure and disco...
This is the author accepted manuscript. The final version is available from American Astronomical So...
A study is presented about the formation of a loop prominence system (LPS) on May 13, 1971. The deve...
Quiescent solar prominences are amongst the most interesting and yet least understood of the phenome...
Context. Prominences are cool, dense clouds suspended within the solar corona. Their in situ formati...
Context. Prominences are cool, dense clouds suspended within the solar corona. Their in situ formati...
A study is presented about the formation of a loop prominence system (LPS) on May 13, 1971. The deve...
Various aspects of solar prominences and the solar corona are discussed. The formation of prominence...
This volume presents the latest research results on solar prominences, including new developments on...
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...
Prominences in the solar corona are a hundredfold cooler and denser than their surroundings, with a ...
The thermal disappearance of solar prominences under strong perturbations due to wave heating, Ohmic...
Quiescent prominences represent a significant challenge to our understanding of the flow of mass and...
Prominence condensation and support, the dynamics of coronal loops, and streamer structure and disco...
This is the author accepted manuscript. The final version is available from American Astronomical So...
A study is presented about the formation of a loop prominence system (LPS) on May 13, 1971. The deve...
Quiescent solar prominences are amongst the most interesting and yet least understood of the phenome...
Context. Prominences are cool, dense clouds suspended within the solar corona. Their in situ formati...
Context. Prominences are cool, dense clouds suspended within the solar corona. Their in situ formati...
A study is presented about the formation of a loop prominence system (LPS) on May 13, 1971. The deve...
Various aspects of solar prominences and the solar corona are discussed. The formation of prominence...
This volume presents the latest research results on solar prominences, including new developments on...
Macroscopic velocity fields have been studied in a solar prominence. The spectra and monochromatic i...